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- galaxies: high-redshift (11)
- gamma rays: stars (11)
- geochronology (11)
- gravitational waves (11)
- hysteresis (11)
- identification (11)
- image processing (11)
- individual-based model (11)
- infants (11)
- ion mobility spectrometry (11)
- lakes (11)
- lamin (11)
- landslide (11)
- late bilinguals (11)
- lidar (11)
- literature review (11)
- local adaptation (11)
- local government (11)
- metabarcoding (11)
- metathesis (11)
- microcystin (11)
- microplastics (11)
- monsoon (11)
- palaeogenomics (11)
- phosphorus (11)
- photocatalysis (11)
- photoluminescence (11)
- plasmas (11)
- postural control (11)
- public management (11)
- rape (11)
- regional history (11)
- rehabilitation (11)
- renewable energy (11)
- retrieval (11)
- ring-opening polymerization (11)
- salivary gland (11)
- simulations (11)
- social cognition (11)
- speech and language therapy (11)
- speech production (11)
- stars: winds (11)
- statistics (11)
- sulfur (11)
- transfer (11)
- vegetation (11)
- water balance (11)
- ADHD (10)
- Aimé Bonpland (10)
- Anxiety (10)
- Apis mellifera (10)
- Archiv (10)
- Atmosphäre (10)
- Big Data (10)
- Bilingualismus (10)
- Blockchain (10)
- Briefedition und -korrespondenz (10)
- Centrosome (10)
- Christentum (10)
- Cortisol (10)
- Database (10)
- Datenschutz (10)
- Deutsche Literatur der Frühen Neuzeit (10)
- Diatoms (10)
- Doping (10)
- Drama (10)
- Eastern Europe (10)
- Electromyography (10)
- FGF21 (10)
- Finanzkrise (10)
- Franconia (10)
- Franken (10)
- GDR (10)
- Genetics (10)
- Great Britain (10)
- Großbritannien (10)
- Hasso-Plattner-Institut (10)
- Indien (10)
- Inflammation (10)
- Intertextualität (10)
- Inversion (10)
- Ion mobility spectrometry (10)
- Ionic liquids (10)
- Japan (10)
- Kant (10)
- Kinetics (10)
- Kolumbien (10)
- Korruption (10)
- Kuba (10)
- Künstliche Intelligenz (10)
- Manganese (10)
- Mars (10)
- MiSpEx (10)
- Militär / Geschichte (10)
- Model (10)
- Modelling (10)
- Myodes glareolus (10)
- Narcissism (10)
- Naturgefahren (10)
- Nichtlineare Dynamik (10)
- Numerical cognition (10)
- Ostracoda (10)
- Paleoclimate (10)
- Paläoklima (10)
- Pflanzengeographie (10)
- Phylogeny (10)
- Physical activity (10)
- Physik (10)
- Pleistocene (10)
- Polizeisoziologie (10)
- Privacy (10)
- Privatisierung (10)
- Quality of life (10)
- Reflexionskompetenz (10)
- Resilience (10)
- Rhetorik (10)
- Schulforschung (10)
- Southeast Asia (10)
- Stability (10)
- Statistical seismology (10)
- Stoffwechsel (10)
- Strategie (10)
- Sun: photosphere (10)
- Terrorismus (10)
- Türkei (10)
- United Nations (10)
- Visualization (10)
- Wilhelm von Humboldt (10)
- X-ray diffraction (10)
- Zeitreihenanalyse (10)
- Zentralasien (10)
- accountability (10)
- adipose tissue (10)
- atomic force microscopy (10)
- back pain (10)
- biophysics (10)
- carbon nitride (10)
- chaos (10)
- child (10)
- climate change adaptation (10)
- cluster expansion (10)
- clustering (10)
- co-citation analysis (10)
- community (10)
- complex networks (10)
- complexity (10)
- correlation (10)
- crisis (10)
- crystallization (10)
- cue-based retrieval (10)
- diatoms (10)
- discourse analysis (10)
- elderly (10)
- exhaustivity (10)
- extreme events (10)
- fitness (10)
- food (10)
- frequency (10)
- freshwater (10)
- gamma rays: ISM (10)
- gamma-ray burst: general (10)
- gene (10)
- genomics (10)
- grazing (10)
- human capital (10)
- human rights (10)
- immigration (10)
- ionic liquid (10)
- justice sensitivity (10)
- language production (10)
- leadership (10)
- light pollution (10)
- living cells (10)
- luminescence (10)
- magnetosphere (10)
- manganese (10)
- masked priming (10)
- mental arithmetic (10)
- metabolic syndrome (10)
- methodology (10)
- microsatellites (10)
- middle childhood (10)
- mitigation (10)
- molybdenum cofactor (10)
- motor control (10)
- movement ecology (10)
- nonlinear dynamics (10)
- numerische Modellierung (10)
- operational momentum (10)
- peptide (10)
- peptides (10)
- phenotypic plasticity (10)
- phosphorylation (10)
- plasma (10)
- potassium (10)
- privacy (10)
- productivity (10)
- protein folding (10)
- quantum dots (10)
- representation (10)
- ruthenium (10)
- scene viewing (10)
- second language (10)
- senescence (10)
- stars (10)
- stars: AGB and post-AGB (10)
- strength (10)
- surface plasmon resonance (10)
- systematic literature review (10)
- taxonomy (10)
- techniques: imaging spectroscopy (10)
- techniques: photometric (10)
- technology (10)
- training load (10)
- water quality (10)
- öffentliche Verwaltung (10)
- α-amylase/trypsin inhibitors (10)
- 20th century (9)
- Albert (9)
- Algorithms (9)
- Antarctica (9)
- Astronomie (9)
- BPMN (9)
- Bacteria (9)
- Bildungswissenschaften (9)
- Biogeography (9)
- Brachionus calyciflorus (9)
- Camus (9)
- Cauchy problem (9)
- Chaos (9)
- Cold War (9)
- Coordination (9)
- Coping (9)
- Deep Learning (9)
- Design Thinking (9)
- Diskussion-Unterricht (9)
- East Germany (9)
- Ecuador (9)
- Entwicklungszusammenarbeit (9)
- Ernährung (9)
- Eye tracking (9)
- Fragmentation (9)
- Frauen (9)
- Geographie-Didaktik (9)
- Geographie-Studium (9)
- Geographie-Unterricht (9)
- Gold (9)
- Hasso Plattner Institute (9)
- Himalayas (9)
- Holozän (9)
- ISM: structure (9)
- Indian summer monsoon (9)
- Infancy (9)
- Information structure (9)
- Insulin resistance (9)
- Interactional Linguistics (9)
- Kartographie (9)
- Kohlenstoff (9)
- Konstruktivismus (9)
- Konversationsanalyse (9)
- Kooperation (9)
- Language (9)
- Lidar (9)
- Mass spectrometry (9)
- Metabolomics (9)
- Metzler Handbuch 2.0 (9)
- Modell (9)
- Modernisierung (9)
- Morphology (9)
- Naturwissenschaft (9)
- Netzwerke (9)
- Oxidative stress (9)
- PHREEQC (9)
- Paris Agreement (9)
- Pregnancy (9)
- Principal component analysis (9)
- Prosodie (9)
- Protein (9)
- Public Management (9)
- Quaternary (9)
- Randomized controlled trial (9)
- Rezeptionsgeschichte (9)
- Russian (9)
- SAXS (9)
- Schulentwicklung (9)
- Selen (9)
- Soil (9)
- Sprachverarbeitung (9)
- Strategies (9)
- Subduction (9)
- Sun: chromosphere (9)
- Sustainability (9)
- Synthetic methods (9)
- Systembiologie (9)
- Theologie (9)
- Theorie (9)
- Transkriptionsfaktoren (9)
- Translation (9)
- Ukraine (9)
- Umweltschutz (9)
- Verhalten (9)
- Vesikel (9)
- Vorhersage (9)
- Wave propagation (9)
- Weiterbildung (9)
- Weltbegriff (9)
- Weltbewusstsein (9)
- Wissensmanagement (9)
- World Bank (9)
- administration (9)
- adolescent (9)
- allometry (9)
- antibody (9)
- authoritarianism (9)
- biofilm (9)
- biomineralization (9)
- block copolymer (9)
- business process management (9)
- cardiovascular disease (9)
- cell adhesion (9)
- charge transfer (9)
- chromatin (9)
- clefts (9)
- comparison (9)
- conservation genetics (9)
- coronary artery disease (9)
- cosmology: observations (9)
- cultural science (9)
- dark ages, reionization, first stars (9)
- decision making (9)
- deutsche Außenpolitik (9)
- diet (9)
- digital health (9)
- disturbance (9)
- dopamine (9)
- ecosystems (9)
- educational sciences (9)
- efficiency (9)
- electron transfer (9)
- elliptic operators (9)
- embodiment (9)
- ethnicity (9)
- executive function (9)
- executive functions (9)
- films (9)
- flexibility (9)
- forest management (9)
- galaxies: interactions (9)
- geophysics (9)
- gold nanoparticles (9)
- human behaviour (9)
- human physical conditioning (9)
- hybridization (9)
- inclusive education (9)
- inhibition (9)
- insect (9)
- intelligence (9)
- international organizations (9)
- isometric muscle action (9)
- kitchen (9)
- kitchen culture (9)
- locality (9)
- membrane (9)
- methods (9)
- microscopy (9)
- moderne jüdische Geschichte (9)
- mtDNA (9)
- organic chemistry (9)
- organization (9)
- osteoporosis (9)
- overweight (9)
- perpetration (9)
- persistence (9)
- phylogeography (9)
- physiology (9)
- polyunsaturated fatty acids (9)
- polyzwitterion (9)
- population (9)
- preparedness (9)
- preview benefit (9)
- professional development (9)
- proteomics (9)
- public health (9)
- race (9)
- reactive transport (9)
- reinforcement learning (9)
- relation historique (9)
- resources (9)
- responses (9)
- sea-level rise (9)
- seed dispersal (9)
- selection (9)
- self-esteem (9)
- self-regulation (9)
- sexual scripts (9)
- signal transduction (9)
- site effects (9)
- skills (9)
- slavic countries (9)
- social inclusion (9)
- soil (9)
- spatial-numerical associations (9)
- species richness (9)
- starch metabolism (9)
- stars: rotation (9)
- structure (9)
- surface chemistry (9)
- surface modification (9)
- suspended sediment (9)
- teaching (9)
- techniques: polarimetric (9)
- virtual reality (9)
- visualization (9)
- waves (9)
- weather (9)
- Öffentliche Verwaltung (9)
- 1814-1831 (8)
- ACT-R (8)
- AFLP (8)
- Alcohol dependence (8)
- Anatolia (8)
- Anpassung (8)
- Arbeitsgedächtnis (8)
- Arenes (8)
- Assessment (8)
- Astrophysik (8)
- Australien (8)
- Austria (8)
- BMI (8)
- Biographie (8)
- Biomaterial (8)
- Biophysik (8)
- Bombina bombina (8)
- Brownian motion (8)
- Bürgerbeteiligung (8)
- Campylomormyrus (8)
- Carbohydrates (8)
- Childhood (8)
- Colombia (8)
- Competition (8)
- Computational modeling (8)
- Connectivity (8)
- Cosmogenic nuclides (8)
- DFT calculations (8)
- Datenintegration (8)
- Deformation (8)
- Degradation (8)
- Dezentralisierung (8)
- Direct electron transfer (8)
- Discussion (8)
- Diskursanalyse (8)
- E-Government (8)
- E. coli (8)
- East Africa (8)
- Ecology (8)
- Ecosystem services (8)
- Emotionen (8)
- Englischunterricht (8)
- Enthusiasmus (8)
- Epigenetics (8)
- Erinnerungskultur (8)
- Fluoreszenz (8)
- Foreign policy (8)
- Forschungsdatenmanagement (8)
- Forschungskolleg (8)
- Forschungsprojekte (8)
- Friedrich Wilhelm III. (8)
- Future SOC Lab (8)
- Galaxien (8)
- Geochronology (8)
- Geography Education (8)
- Geschlecht (8)
- Geschäftsprozessmanagement (8)
- Grammatik (8)
- Gravitationswellen (8)
- Holocaust (8)
- Human Rights (8)
- In-Memory Technologie (8)
- Individual differences (8)
- Information Structure (8)
- Interaktion (8)
- Internationale Beziehungen (8)
- Inverse theory (8)
- Johann Gottfried Herder (8)
- Jugendforschung (8)
- Kapitalismus (8)
- Klausurtagung (8)
- Klimaanpassung (8)
- Komplexität (8)
- Korrespondenz (8)
- Krise (8)
- Kulturvergleich (8)
- Landsat (8)
- Landslide (8)
- Last Glacial Maximum (8)
- Latein (8)
- Lateinunterricht (8)
- Lepus europaeus (8)
- Ludwig Leichhardt (8)
- MOOCs (8)
- Mannheim Study of Children at Risk (8)
- Menschenrecht (8)
- Metabolism (8)
- Microtus arvalis (8)
- Mikrobiologie (8)
- Mobilität (8)
- Moderne (8)
- Monitoring (8)
- Movement (8)
- Multicore Architekturen (8)
- NICS (8)
- Namibia (8)
- Nutrition (8)
- Optimization (8)
- Overweight (8)
- PCA (8)
- PUFA (8)
- Paläoklimatologie (8)
- Patterns (8)
- Phosphorus (8)
- Photochemie (8)
- Photosynthese (8)
- Phytoplankton (8)
- Polyelektrolyt (8)
- Polyelektrolyte (8)
- Prediction (8)
- Prevention (8)
- Realpolitik (8)
- Recht (8)
- Security (8)
- Semantik (8)
- Sentence comprehension (8)
- Service-oriented Systems Engineering (8)
- Sphingolipids (8)
- Sport (8)
- Sprachkontakt (8)
- Subduktion (8)
- Sun: filaments, prominences (8)
- Systemtheorie (8)
- TAVI (8)
- Tacitus (8)
- Taxonomy (8)
- Tectonics (8)
- Theoretical calculations (8)
- Thermokarst (8)
- Through-space NMR shieldings (TSNMRS) (8)
- Validation (8)
- Verwaltungsreform (8)
- Vitamin A (8)
- Wahlen (8)
- X-ray refraction (8)
- X-ray structure (8)
- Younger Dryas (8)
- Zeitgenossen (8)
- Zentraleuropa (8)
- Zooplankton (8)
- acceleration (8)
- acculturation (8)
- algae (8)
- alien species (8)
- amerikanische Reisetagebücher (8)
- arithmetic (8)
- astrophysics (8)
- attitude (8)
- attitudes (8)
- auxin (8)
- bicameralism (8)
- biomaterial (8)
- brain (8)
- cAMP (8)
- carbon cycle (8)
- cardiovascular diseases (8)
- cells (8)
- cellulose (8)
- chemistry (8)
- chemotaxis (8)
- chronic kidney disease (8)
- climate impacts (8)
- climate variability (8)
- cloud (8)
- coherence (8)
- competence (8)
- complex systems (8)
- consistency (8)
- control (8)
- convection (8)
- conversation analysis (8)
- cortisol (8)
- cytotoxicity (8)
- data integration (8)
- data profiling (8)
- density functional calculations (8)
- dielectrophoresis (8)
- digitale Medien (8)
- dissociative electron attachment (8)
- distribution (8)
- electrospinning (8)
- energy (8)
- energy policy (8)
- energy storage (8)
- enzymes (8)
- ethics (8)
- experiments (8)
- feminism (8)
- fiscal policy (8)
- flow (8)
- food web (8)
- force (8)
- fractional Brownian motion (8)
- galaxies (8)
- gamma-rays: galaxies (8)
- gender differences (8)
- genetics (8)
- geochemistry (8)
- grain size (8)
- graphene (8)
- home range (8)
- hypertension (8)
- imaging (8)
- immobilization (8)
- inference (8)
- injury risk (8)
- instability (8)
- institutions (8)
- insurance (8)
- isomerization (8)
- land use change (8)
- landscape of fear (8)
- language contact (8)
- light (8)
- major depressive disorder (8)
- malnutrition (8)
- mathematical modeling (8)
- mathematische Modellierung (8)
- maximal isometric Adaptive Force (8)
- meaning (8)
- measurement (8)
- mechanisms (8)
- mechanobiology (8)
- media violence (8)
- membranes (8)
- metabolite profiling (8)
- methane (8)
- microfluidics (8)
- microstructure (8)
- microtubules (8)
- military (8)
- mobility (8)
- modality (8)
- morphological processing (8)
- muscle (8)
- music (8)
- nanocomposite (8)
- narcissism (8)
- natural language processing (8)
- natural products (8)
- neuromuscular control (8)
- neuroplasticity (8)
- noise (8)
- nuclear envelope (8)
- nuclear lamina (8)
- numerical relativity (8)
- numerical simulation (8)
- outflows (8)
- pain (8)
- parliamentary government (8)
- perceptual span (8)
- phonological awareness (8)
- physics (8)
- plankton (8)
- plasmonics (8)
- polarization (8)
- policy (8)
- polyelectrolyte (8)
- production control (8)
- programming (8)
- pronouns (8)
- propensity score matching (8)
- psychotherapy training (8)
- public sector (8)
- quality (8)
- quality assurance (8)
- quantification (8)
- quasars: general (8)
- reanalysis (8)
- recombination (8)
- reproducibility (8)
- residual stress (8)
- restoration (8)
- risk perception (8)
- rotation (8)
- sedimentary ancient DNA (8)
- snow (8)
- solar cells (8)
- spatial frequencies (8)
- stars: activity (8)
- stars: emission-line, Be (8)
- stars: kinematics and dynamics (8)
- sustainable development (8)
- teaching quality (8)
- thermokarst (8)
- time series (8)
- time-series (8)
- tracking (8)
- treeline (8)
- trends (8)
- trust (8)
- ultrafast (8)
- urbanization (8)
- ventral striatum (8)
- verification (8)
- vitamin A (8)
- wh-questions (8)
- work (8)
- yellow flags (8)
- Abrüstung (7)
- Algeria (7)
- Anisotropy (7)
- Anisotropy effect (7)
- Antike (7)
- Antisemitismus (7)
- Apoptosis (7)
- Aromaticity (7)
- Balance (7)
- Bewegung (7)
- Blockcopolymere (7)
- Botanik (7)
- Brasilien (7)
- C. elegans (7)
- CO2 (7)
- COVID-19 pandemic (7)
- Capsella (7)
- Clusteranalyse (7)
- Complex networks (7)
- Complexity (7)
- Crustal structure (7)
- Cytotoxicity (7)
- DNA damage (7)
- DNA radiation damage (7)
- Decision-making (7)
- Dekonstruktion (7)
- Democracy (7)
- Demokratisierung (7)
- Design (7)
- Deutschdidaktik (7)
- Diabetes (7)
- Digitale Plattformen (7)
- Dirac operator (7)
- Diskriminierung (7)
- Diskurs (7)
- Disturbance (7)
- Earthquake hazards (7)
- East African Rift System (7)
- Egypt (7)
- Emulsion (7)
- Erziehungswissenschaften (7)
- Eurokrise (7)
- Eutrophication (7)
- Fokus (7)
- Forschendes Lernen (7)
- Forschungsreisen (7)
- Freiheit (7)
- Föderalismus (7)
- Führung (7)
- Geochemistry (7)
- Geopolitik (7)
- Georgien (7)
- Gesundheit (7)
- Global change (7)
- Greenland (7)
- Groundwater (7)
- Herrschaft (7)
- Hertzsprung-Russell and C-M diagrams (7)
- Higher education (7)
- Humboldt Digital Library (7)
- Humboldtian Science (7)
- Indian Summer Monsoon (7)
- Inspiration (7)
- Interaction (7)
- Interest (7)
- Interoception (7)
- Italien (7)
- Japanese (7)
- K-theory (7)
- Kalman filter (7)
- Kalter Krieg (7)
- Kiezdeutsch (7)
- Klimaschutz (7)
- Klimaänderung (7)
- Kompetenzen (7)
- Krieg (7)
- LCSM (7)
- Land use change (7)
- Landnutzung (7)
- Landschaftsmalerei (7)
- Landwirtschaft (7)
- Leadership (7)
- Leguminosae (7)
- Lehrer (7)
- LiDAR (7)
- Logik (7)
- Longitudinal study (7)
- Low German (7)
- Lumineszenz (7)
- Machtpolitik (7)
- Magnetismus (7)
- Massenspektrometrie (7)
- Mekong Delta (7)
- Memory (7)
- Microtubules (7)
- Molecular dynamics (7)
- Molecularly imprinted polymers (7)
- Molybdenum cofactor (7)
- Mongolia (7)
- Monsoon (7)
- Monsun (7)
- Mortality (7)
- Muscle strength (7)
- Musik (7)
- Musikunterricht (7)
- Nachlass (7)
- Nanostruktur (7)
- Naturgeschichte (7)
- Naturphilosophie (7)
- Naturschutz (7)
- Neoliberalismus (7)
- Neotektonik (7)
- Netzwerk (7)
- Niederdeutsch (7)
- Norway (7)
- Nutrients (7)
- O-antigen (7)
- PBPK (7)
- Palaeoclimate (7)
- Paleolimnology (7)
- Palästina (7)
- Parteien (7)
- Perception (7)
- Phylogeography (7)
- Polymerchemie (7)
- Polymers (7)
- Praxissemester (7)
- Prevalence (7)
- Professionsorientierung (7)
- Prozessmodellierung (7)
- Prunus avium L. (7)
- Pseudomonas aeruginosa (7)
- RIXS (7)
- Reading motivation (7)
- Regulierung (7)
- Remote sensing (7)
- Resistance training (7)
- Resozialisierung (7)
- Return to work (7)
- Rheologie (7)
- Ring current effect (7)
- Risiko (7)
- Seasonality (7)
- Security Policy (7)
- Seesedimente (7)
- Smalltalk (7)
- Soil moisture (7)
- Solanaceae (7)
- Sprachwandel (7)
- Sprachwissenschaft (7)
- Starch metabolism (7)
- Steuerung (7)
- Stickstoff (7)
- Survey (7)
- Svalbard (7)
- Switzerland (7)
- Synthesis (7)
- Südafrika (7)
- Tagebuch (7)
- Teacher training (7)
- Theory (7)
- Tien Shan (7)
- Time series (7)
- Time series analysis (7)
- Tolkien (7)
- Transfer (7)
- Twitter (7)
- Uncertainty (7)
- Unsicherheit (7)
- Unsicherheiten (7)
- Vegetation (7)
- Verwaltungsmodernisierung (7)
- Vietnamese (7)
- Vulnerabilität (7)
- Walking (7)
- Wasser (7)
- Water (7)
- Water quality (7)
- X-rays: ISM (7)
- Youth (7)
- Zinc (7)
- Zivilgesellschaft (7)
- academic achievement (7)
- acquisition (7)
- age of acquisition (7)
- aggregation (7)
- air pollution (7)
- algorithms (7)
- alignment (7)
- allostatic load (7)
- amino acids (7)
- amygdala (7)
- anthropometry (7)
- apoptosis (7)
- arctic (7)
- articulation (7)
- augmented reality (7)
- autonomy (7)
- bias (7)
- binaries: eclipsing (7)
- biogenic amines (7)
- birth weight (7)
- business processes (7)
- bystander (7)
- calibration (7)
- catalogs (7)
- change (7)
- charge generation (7)
- children and adolescents (7)
- circadian clock (7)
- circulation (7)
- circumstellar matter (7)
- cities (7)
- classical reception (7)
- climate-change mitigation (7)
- coastal erosion (7)
- cognitive development (7)
- colonialism (7)
- community ecology (7)
- complexes (7)
- computer games (7)
- corruption (7)
- cyber aggression (7)
- data (7)
- databases (7)
- defense (7)
- density (7)
- depressive symptoms (7)
- developmental dyscalculia (7)
- dietary patterns (7)
- discrepancy principle (7)
- duplicate detection (7)
- dust (7)
- ecological modelling (7)
- ecosystem functioning (7)
- effectiveness (7)
- ensemble Kalman filter (7)
- enzyme (7)
- enzyme catalysis (7)
- eutrophication (7)
- exercise therapy (7)
- extinction (7)
- extraction (7)
- extreme rainfall (7)
- fiction (7)
- first passage time (7)
- flood (7)
- floodplain (7)
- fluorescence correlation spectroscopy (7)
- food webs (7)
- function (7)
- functional magnetic resonance imaging (7)
- galaxies: dwarf (7)
- galaxies: starburst (7)
- gene flow (7)
- global (7)
- global warming (7)
- gravity (7)
- habitat (7)
- heart (7)
- heterogeneous catalysis (7)
- holocene (7)
- human impact (7)
- hydrolysis (7)
- ideology (7)
- imaging spectroscopy (7)
- income (7)
- infrared: stars (7)
- insula (7)
- international law (7)
- interoceptive awareness (7)
- isotopes (7)
- jumping (7)
- kardiologische Rehabilitation (7)
- kinematics (7)
- knowledge (7)
- land-use change (7)
- last glacial maximum (7)
- law (7)
- life history (7)
- lipid metabolism (7)
- low-energy electrons (7)
- magnetism (7)
- manifolds with singularities (7)
- memory retrieval (7)
- mental disorders (7)
- metaanalysis (7)
- metabolic networks (7)
- metaphor (7)
- miRNA (7)
- microbial ecology (7)
- minerals (7)
- mixed methods (7)
- modern Jewish history (7)
- moment tensor (7)
- myocardial infarction (7)
- nanostructure (7)
- neotectonics (7)
- neutron diffraction (7)
- next generation sequencing (7)
- nitrogen deposition (7)
- nonergodicity (7)
- nucleus (7)
- number (7)
- numerical simulations (7)
- openHPI (7)
- organic matter (7)
- organic photovoltaics (7)
- orthography (7)
- oscillations (7)
- oxygen (7)
- pH (7)
- palaeoecology (7)
- paleoecology (7)
- pandemic (7)
- parafoveal processing (7)
- parameter estimation (7)
- parents (7)
- pathogens (7)
- perturbation (7)
- phase transition (7)
- phase transitions (7)
- phenomenology (7)
- photoelectron spectroscopy (7)
- planetary nebulae: general (7)
- planets and satellites: rings (7)
- plant diversity (7)
- plyometric training (7)
- pollution (7)
- polyelectrolytes (7)
- porous materials (7)
- predator-prey dynamics (7)
- presidential government (7)
- production (7)
- pronoun resolution (7)
- prosodic boundary cues (7)
- proteasome (7)
- protection (7)
- pseudodifferential operators (7)
- pulsars: general (7)
- racism (7)
- radiocarbon (7)
- reconstruction (7)
- reduction (7)
- repair (7)
- retinol (7)
- rheology (7)
- roughness (7)
- scale development (7)
- scattering (7)
- screening (7)
- secular trend (7)
- sediment transport (7)
- seismic hazard (7)
- serotonin (7)
- shape-memory effect (7)
- sharing economy (7)
- silicon (7)
- size (7)
- soccer (7)
- social rejection (7)
- social support (7)
- socioeconomic status (7)
- software engineering (7)
- soil erosion (7)
- solar wind (7)
- sorption (7)
- speciation (7)
- spelling (7)
- stabile Isotope (7)
- standardization (7)
- stars: late-type (7)
- structure elucidation (7)
- sunspots (7)
- surfactants (7)
- surveillance (7)
- tVNS (7)
- taste (7)
- techniques: image processing (7)
- thermoresponsiv (7)
- thermoresponsive polymers (7)
- tomato (7)
- tomography (7)
- tools (7)
- topography (7)
- trunk (7)
- ultrafast dynamics (7)
- ultrasound (7)
- uncertainty analysis (7)
- unemployment (7)
- uplift (7)
- variation (7)
- vesicles (7)
- video analysis (7)
- water management (7)
- wh-in-situ (7)
- working memory capacity (7)
- world literature (7)
- youth sports (7)
- Ästhetik (7)
- öffentlicher Sektor (7)
- 1800 (6)
- 19th century (6)
- 3D (6)
- 3D visualization (6)
- AFM (6)
- Absorption (6)
- Acceleration (6)
- Adhäsion (6)
- Ageing (6)
- Agency (6)
- Alaska (6)
- Alps (6)
- Antibiotikaresistenz (6)
- Antikörper (6)
- Antwortmengenprogrammierung (6)
- Aristoteles (6)
- Arsenolipids (6)
- Atomwaffen (6)
- Aufmerksamkeit (6)
- Bakterien (6)
- Bayesian data analysis (6)
- Berühren (6)
- Bewegungsökologie (6)
- Bioelectrocatalysis (6)
- Biogenic amine (6)
- Blockcopolymer (6)
- Boden (6)
- Brief (6)
- C-reactive protein (6)
- Cardiovascular diseases (6)
- Caribbean (6)
- Centrosom (6)
- Chemotaxis (6)
- Chimborazo (6)
- Chloroplast (6)
- Chytridiomycota (6)
- Click chemistry (6)
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- Computational modelling (6)
- Computerspiele (6)
- Copper (6)
- Cystic fibrosis (6)
- Daniel Kehlmann (6)
- Data assimilation (6)
- Deep learning (6)
- Deutschunterricht (6)
- Dielektrophorese (6)
- Digitale Medien (6)
- Disarmament (6)
- Diversity (6)
- Dynamic NMR (6)
- Dynamik (6)
- EEG/ERP (6)
- Effizienz (6)
- Electrical conductivity (6)
- Ellenberg indicator values (6)
- Eltern (6)
- Emotions (6)
- Energy (6)
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- Erinnerung (6)
- Ethics (6)
- European hare (6)
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- H II regions (6)
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- Organisation (6)
- Oxygen heterocycles (6)
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- Pavlovian-to-instrumental transfer (6)
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- Predictors (6)
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- Sexual scripts (6)
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- Sibirien (6)
- Software (6)
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- Solanum tuberosum (6)
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- Starkregen (6)
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- abstract concepts (6)
- acid ceramidase (6)
- administrative reform (6)
- admixture (6)
- agreement (6)
- alexithymia (6)
- animal movement (6)
- antioxidants (6)
- architecture (6)
- assembly (6)
- athletes (6)
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- big data (6)
- biodegradable polymers (6)
- biosensors (6)
- black holes (6)
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- body (6)
- bryophytes (6)
- capitalism (6)
- carbon sequestration (6)
- cardiorespiratory fitness (6)
- cartel (6)
- case study (6)
- cell-free protein synthesis (6)
- change detection (6)
- characteristics (6)
- chemical modification (6)
- chloroplast (6)
- climate mitigation (6)
- cluster analysis (6)
- co-limitation (6)
- collaboration (6)
- collective memory (6)
- collusion (6)
- community effect (6)
- constraints (6)
- contrast (6)
- coping (6)
- copolymers (6)
- corpus study (6)
- costs (6)
- crisis management (6)
- crown compounds (6)
- crystal-structure (6)
- cultural diversity (6)
- cultural studies (6)
- cyber victimization (6)
- cyber-physical systems (6)
- cyberhate (6)
- cytoskeleton (6)
- design (6)
- development cooperation (6)
- diabetic nephropathy (6)
- dialogue (6)
- diffuse radiation (6)
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- digitale Bildung (6)
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- domestication (6)
- droughts (6)
- dust, extinction (6)
- early warning (6)
- eclogite (6)
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- eicosapentaenoic acid (6)
- electrons (6)
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- extension (6)
- eye movement (6)
- fNIRS (6)
- fabrication (6)
- facilitation (6)
- federalism (6)
- fertilization (6)
- financial markets (6)
- first passage (6)
- first-passage time (6)
- flooding (6)
- fluorescent dyes (6)
- foreland basin (6)
- formal semantics (6)
- galaxies: abundances (6)
- galaxy evolution (6)
- gamma-ray astronomy (6)
- gamma-rays: general (6)
- gas (6)
- gelatin (6)
- general relativity (6)
- genes (6)
- geodynamics (6)
- geology (6)
- geometric Brownian motion (6)
- givenness (6)
- giving-up density (6)
- glutathione peroxidase (6)
- grammar (6)
- green chemistry (6)
- habituation (6)
- heart rate variability (6)
- heat (6)
- heat stress (6)
- heterocycles (6)
- history and philosophy of astronomy (6)
- holding capacity (6)
- honey bee (6)
- honeybee (6)
- hybrid materials (6)
- hybridization capture (6)
- hydrogen (6)
- hydrologische Modellierung (6)
- impacts (6)
- implicit (6)
- indianische Kunst (6)
- infancy (6)
- infection (6)
- influenza (6)
- information (6)
- injury (6)
- interfaces (6)
- international relations (6)
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- intertextuality (6)
- introgression (6)
- invasive species (6)
- knowledge transfer (6)
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- mapping (6)
- maturation (6)
- mechanism (6)
- melt inclusions (6)
- mental simulation (6)
- metabolites (6)
- methods: analytical (6)
- micelles (6)
- microarray (6)
- microbial activity (6)
- microbial communities (6)
- microbial diversity (6)
- mind wandering (6)
- molecular modeling (6)
- molecular motors (6)
- molecular rods (6)
- multicore architectures (6)
- muscle power (6)
- nanoparticle (6)
- narration (6)
- negation (6)
- network analysis (6)
- neurodegeneration (6)
- new public management (6)
- non-fullerene acceptors (6)
- nonlinear (6)
- nucleation (6)
- numerical development (6)
- optimization (6)
- organic semiconductors (6)
- p53 (6)
- palaeoclimate (6)
- parameters (6)
- pattern formation (6)
- perovskite (6)
- perpetrator (6)
- phenology (6)
- phonetics (6)
- phosphate (6)
- phylogenetic diversity (6)
- picture naming (6)
- piezoelectricity (6)
- planning (6)
- plant (6)
- plants (6)
- political equality (6)
- polypeptide (6)
- polyphenols (6)
- polystyrene (6)
- polyzwitterions (6)
- population density (6)
- porosity (6)
- porous carbon (6)
- postural stability (6)
- pragmatics (6)
- predictability (6)
- preferential flow (6)
- pregnancy (6)
- presupposition (6)
- probiotics (6)
- process mining (6)
- professional knowledge (6)
- projections (6)
- protein adsorption (6)
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- quantum chemical calculations (6)
- questionnaire (6)
- radical polymerization (6)
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- rampage (6)
- randomized controlled trial (6)
- rat (6)
- reciprocal class (6)
- relative index (6)
- reproduction (6)
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- retinol-binding protein 4 (6)
- return to work (6)
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- risk factor (6)
- running (6)
- saccades (6)
- salinity gradient (6)
- scrambling (6)
- sedaDNA (6)
- self-concept (6)
- self-healing (6)
- sensitivity analysis (6)
- sensor (6)
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- sex (6)
- silver nanoparticles (6)
- social comparison (6)
- sodium (6)
- software (6)
- software development (6)
- soil organic carbon (6)
- spectra (6)
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- stars: magnetic fields (6)
- state (6)
- stimuli-sensitive polymers (6)
- stochastic differential equations (6)
- stroke (6)
- structural equation modeling (6)
- sucrose (6)
- sulfite oxidase (6)
- support vector machine (6)
- surface relief grating (6)
- surgery (6)
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- tailspike protein (6)
- teacher (6)
- teachers (6)
- tendinopathy (6)
- thaliana (6)
- therapist competence (6)
- therapy (6)
- thermodynamics (6)
- tourism (6)
- trade-offs (6)
- training adaptation (6)
- traits (6)
- transcription (6)
- transcriptional memory (6)
- transcriptome (6)
- tundra (6)
- type 2 diabetes mellitus (6)
- typology (6)
- user experience (6)
- vesicle (6)
- visions of democracy (6)
- walking (6)
- weight loss (6)
- wetlands (6)
- young adults (6)
- zebrafish (6)
- 3D point clouds (5)
- AC electrokinetics (5)
- ALAN (5)
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- Affiliation (5)
- African Humid Period (5)
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- Atiyah-Patodi-Singer theory (5)
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- Cyanobakterien (5)
- DNS (5)
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- Dictyostelium discoideum (5)
- Die Vermessung der Welt (5)
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- Finanzmärkte (5)
- Fire-bellied toad (5)
- Flow cytometry (5)
- Flow-Erleben (5)
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- Fluoreszenzmikroskopie (5)
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- Frailty (5)
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- Graph theory (5)
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- Ground reaction force (5)
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- Holding isometric muscle action (5)
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- Imaging (5)
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- Kompetenz (5)
- Korrosion (5)
- Kunst (5)
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- uncertainties (5)
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- upconversion (5)
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- 4 (4)
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- conversion (4)
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- covariance (4)
- creep (4)
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- deformation (4)
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- deposition (4)
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- distributed systems (4)
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- dog (4)
- downscaling (4)
- dropout (4)
- drylands (4)
- dual-process (4)
- dyadic coping (4)
- dye (4)
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- dynamic capabilities (4)
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- effect (4)
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- elite athlete (4)
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- emissions (4)
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- employment policy (4)
- empowerment (4)
- endophytes (4)
- endurance exercise (4)
- enhancement (4)
- entanglement (4)
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- environmental economics (4)
- environmental filtering (4)
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- equifinality (4)
- errata, addenda (4)
- ethnic differences (4)
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- evaluative study (4)
- evaporites (4)
- event-related brain potentials (4)
- everyday life (4)
- evolutionary history (4)
- exchange (4)
- exercise intensity (4)
- expansion microscopy (4)
- experimental design (4)
- exploratory-behavior (4)
- extracellular matrix (4)
- eye-movement monitoring (4)
- face perception (4)
- fatty acid metabolism (4)
- fatty-acids (4)
- fault (4)
- faults (4)
- feature selection (4)
- fence ecology (4)
- ferroelectrets (4)
- ferroelectric polymers (4)
- ferroelectricity (4)
- financial crisis (4)
- financial institutions (4)
- finger counting (4)
- first language acquisition (4)
- first-passage (4)
- fiscal federalism (4)
- fixation durations (4)
- flavonoid (4)
- floral scent (4)
- flower development (4)
- fluctuating light (4)
- fluid inclusions (4)
- focal adhesion (4)
- food neophilia (4)
- forest (4)
- formal verification (4)
- forschendes Lernen (4)
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- framework (4)
- frequency analysis (4)
- friendship (4)
- frustration (4)
- functional response (4)
- fundamental frequency (4)
- fungi (4)
- galaxies: star formation (4)
- garden-path effect (4)
- gaze-contingent displays (4)
- gene regulatory networks (4)
- genealogy (4)
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- holding isometric muscle action (HIMA) (4)
- hormones (4)
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- ill-posed problem (4)
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- lactate (4)
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- large-scale structure of Universe (4)
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- left periphery (4)
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- lexicon (4)
- lichens (4)
- life satisfaction (4)
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- light variability (4)
- line: identification (4)
- linear hypersubstitution (4)
- linear mixed models (4)
- lipidomics (4)
- literacy acquisition (4)
- loading rate (4)
- locomotion (4)
- locus coeruleus (4)
- long-distance dispersal (4)
- low-back-pain (4)
- lower critical solution temperature (4)
- lutein (4)
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- mammals (4)
- manifold with singularities (4)
- manufacturing (4)
- masculinity (4)
- mass (4)
- mathematics education (4)
- mathematics instruction (4)
- meadow (4)
- measurement invariance (4)
- mechanical tendinous oscillations (4)
- media use (4)
- memory effects (4)
- mesenchymal stem cells (4)
- mesoporous materials (4)
- metabolic engineering (4)
- metabolic regulation (4)
- metabolite (4)
- metadata (4)
- metagenomics (4)
- meteorological drought (4)
- methods: statistical (4)
- methyl orange (4)
- methylene blue (4)
- methylmercury (4)
- micro-CT (4)
- microRNA (4)
- microlensing (4)
- mid-temperature transition (4)
- mild cognitive impairment (4)
- mitochondrial DNA (4)
- mitosis (4)
- mixtures (4)
- mobile links (4)
- model-driven engineering (4)
- modular production (4)
- molecular evolution (4)
- molecules (4)
- monoclonal antibody (4)
- mood (4)
- morality (4)
- morphogenesis (4)
- motivational interviewing (4)
- mowing (4)
- multi-level system (4)
- multilevel analysis (4)
- multivariate statistics (4)
- muscle oxygen saturation (4)
- music information retrieval (4)
- musikpädagogische Forschung (4)
- n-alkanes (4)
- nachhaltige Chemie (4)
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- nanotriangles (4)
- national identity (4)
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- neutrinos (4)
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- next generation sequencing (NGS) (4)
- nominalization (4)
- non-alcoholic fatty liver disease (4)
- non-linear dynamics (4)
- non-native speakers (4)
- non-photorealistic rendering (4)
- nonlinear operator (4)
- noun (4)
- numerical (4)
- numerical model (4)
- ocean (4)
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- ocean color remote sensing (4)
- online discrimination (4)
- online learning (4)
- ontogeny (4)
- open data (4)
- open-circuit voltage (4)
- operating systems (4)
- optimal foraging (4)
- optimal transport (4)
- organ size (4)
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- organische Chemie (4)
- organische Halbleiter (4)
- osmotic-pressure (4)
- osteoblast (4)
- other-race effect (4)
- outcomes (4)
- paleoaltimetry (4)
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- paleolimnology (4)
- parafoveal-on-foveal effect (4)
- part 1 (4)
- partial clone (4)
- partial least squares (4)
- particle acceleration (4)
- parties (4)
- pathway (4)
- patient education (4)
- peace (4)
- people (4)
- performance information (4)
- performance management (4)
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- permafrost thaw (4)
- persulfide (4)
- phase (4)
- phase dynamics (4)
- phase oscillators (4)
- phenols (4)
- phenotyping (4)
- phosphatidylserine (4)
- phospholipids (4)
- photoelectron (4)
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- photoisomerization (4)
- photon density wave spectroscopy (4)
- photooxygenation (4)
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- physiological consequences (4)
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- picture-word interference (4)
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- potato (4)
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- precursor (4)
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- proactivity (4)
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- problem-solving (4)
- process (4)
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- properties (4)
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- qualitative Analyse (4)
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- receptor (4)
- recollection (4)
- recombinant inbred line (4)
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- recurrence plot (4)
- redox (4)
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- region (4)
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- relatedness (4)
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- 'eta' invariant (3)
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Komplexe Systeme reichen von "harten", physikalischen, wie Klimaphysik, Turbulenz in Fluiden oder Plasmen bis zu so genannten "weichen", wie man sie in der Biologie, der Physik weicher Materie, Soziologie oder Ökonomie findet. Die Ausbildung von Verständnis zu einem solchen System beinhaltet eine Beschreibung in Form von Statistiken und schlussendlich mathematischen Gleichungen. Moderne Datenanalyse stellt eine große Menge von Werkzeugen zur Analyse von Komplexität auf verschiedenen Beschreibungsebenen bereit. In diesem Kurs werden statistische Methoden mit einem Schwerpunkt auf dynamischen Systemen diskutiert und eingeübt. Auf der methodischen Seite werden lineare und nichtlineare Ansätze behandelt, inklusive der Standard-Werkzeuge der deskriptiven und schlussfolgernden Statistik, Wavelet Analyse, Nichtparametrische Regression und der Schätzung nichtlinearer Maße wie fraktaler Dimensionen, Entropien und Komplexitätsmaßen. Auf der Modellierungsseite werden deterministische und stochastische Systeme, Chaos, Skalierung und das Entstehen von Komplexität durch Wechselwirkung diskutiert - sowohl für diskrete als auch für ausgedehnte Systeme. Die beiden Ansätze werden durch Systemanalyse jeweils passender Beispiele vereint.
Komplexe Systeme reichen von "harten", physikalischen, wie Klimaphysik, Turbulenz in Fluiden oder Plasmen bis zu so genannten "weichen", wie man sie in der Biologie, der Physik weicher Materie, Soziologie oder Ökonomie findet. Die Ausbildung von Verständnis zu einem solchen System beinhaltet eine Beschreibung in Form von Statistiken und schlussendlich mathematischen Gleichungen. Moderne Datenanalyse stellt eine große Menge von Werkzeugen zur Analyse von Komplexität auf verschiedenen Beschreibungsebenen bereit. In diesem Kurs werden statistische Methoden mit einem Schwerpunkt auf dynamischen Systemen diskutiert und eingeübt. Auf der methodischen Seite werden lineare und nichtlineare Ansätze behandelt, inklusive der Standard-Werkzeuge der deskriptiven und schlussfolgernden Statistik, Wavelet Analyse, Nichtparametrische Regression und der Schätzung nichtlinearer Maße wie fraktaler Dimensionen, Entropien und Komplexitätsmaßen. Auf der Modellierungsseite werden deterministische und stochastische Systeme, Chaos, Skalierung und das Entstehen von Komplexität durch Wechselwirkung diskutiert - sowohl für diskrete als auch für ausgedehnte Systeme. Die beiden Ansätze werden durch Systemanalyse jeweils passender Beispiele vereint.
We investigate localized periodic solutions (breathers) in a lattice of parametrically driven, nonlinear dissipative oscillators. These breathers are demonstrated to be exponentially localized, with two characteristic localization lengths. The crossover between the two lengths is shown to be related to the transition in the phase of the lattice oscillations.
We prove the existence of nonlinear localized time-periodic solutions in a chain of symplectic mappings with nearest neighbour coupling. This is a class of systems whose behaviour can be seen as representation of a lattice of pendula. The effect of discrete time changes the mathematical as well as the numerical procedures. Applying the discrete version of Floquet theory eases and clarifies the procedure of proving the existence of the localized time-periodic solutions. As an extension of the concept of rotobreathers one can produce solutions which rotate at every site of the lattice. To consider these we use a general definition of localization.
A key technology for large eddy simulation (LES) of complex flows is an appropriate wall modeling strategy. In this paper we apply for the first time a fully nonparametric procedure for the estimation of generalized additive models (GAM) by conditional statistics. As a database, we use DNS and wall-resolved LES data of plane channel flow for Reynolds numbers, Re = 2800, 4000 (DNS) and 10,935, 22,776 (LES). The statistical method applied is a quantitative tool for the identification of important model terms, allowing for an identification of some of the near-wall physics. The results are given as nonparametric functions which cannot be attained by other methods. We investigated a generalized model which includes Schumann's and Piomelli et al.'s model. A strong influence of the pressure gradient in the viscous sublayer is found; for larger wall distances the spanwise pressure gradient even dominates the tau(w,zy). component. The first a posteriori LES results are given.
Im Februar und März 2007 wurde vom Geographischen Institut der Universität eine Exkursion nach Neuseeland durchgeführt. Der hier vorliegende Bericht bezieht sich auf diese Exkursion. Im ersten Teil wird durch 17 Protokolle der Exkursionsverlauf wiedergegeben. Im zweiten Teil befassen sich sechs Texte näher mit je einem thematischen Aspekt der Exkursion. Autoren der Protokolle und der thematischen Texte sind die Teilnehmerinnen und Teilnehmer der Exkursion. Zum ersten Teil des Berichts – der Exkursionsverlauf Im ersten Teil dieses Berichtes wird der Verlauf der Exkursion Neuseeland 2007 des Geographischen Instituts der Universität Potsdam durch Tagesprotokolle dargestellt. Die Exkursion begann am 14. Februar 2007 in Auckland und endete am 4. März 2007 in Christchurch. Während dieser 19 Tage wurden verschiedene Orte auf der neuseeländischen Nord- und Südinsel aufgesucht, wobei die Exkursionsgruppe verschiedene Aspekte der neuseeländischen Gesellschaft aus einer humangeographischen Perspektive studierte. Im Mittelpunkt standen die Themen historische und jüngere Migration nach Neuseeland, Maori, Milchwirtschaft, Holzwirtschaft und Tourismus in Neuseeland. Die Tagesprotokolle machen deutlich, dass die Exkursion weniger in einer thematisch-systematischen Art und Weise durchgeführt wurde. Statt dessen erfolgte das Aufsuchen exemplarischer Orte, an denen Beobachtungen und darüber hinausgehende Erkundungen stattfanden. Die entsprechenden Aussagen sind in den Protokollen wiedergegeben, schwerpunktmäßig wird dabei folgendes angesprochen: Der erste Exkursionstag, das war der 14. Februar 2007, wurde für den Besuch des Geographischen Institutes der Auckland University genutzt. Dort wurde zum Beispiel eine Diskussionsrunde mit den beiden Humangeographen Richard Le Heron und Gordon Winder veranstaltet. Auch die folgenden zwei Tage verbrachten die Exkursionsgruppe in Auckland, wobei sie sich im »Auckland Museum« über die neuseeländische Geschichte und insbesondere über die Kultur der Maori informierte. Mit einem Maori-Guide unternahmen die Teilnehmer eine Stadtführung durch Auckland, wobei ebenfalls das Leben der Maori im Fokus stand. Außerdem besuchten sie eine private Einwanderungsagentur und führten in Kleingruppen Expertengespräche zum Thema »Migration und Integration in Neuseeland« durch. Am 17. Februar erkundeten die Exkursionsteilnehmer drei Orte in der näheren Umgebung Aucklands. Zunächst begaben sie sich zum Otara Market, einem Wochenmarkt der Pacific Islanders, der immer samstags in Otara abgehalten wird. Anschließend ging es weiter an die westliche Küste, wo sie unter Führung einer Rangerin durch den Muriwai-Regionalpark wanderten. Auf der Rückfahrt nach Auckland machten sie Halt in Soljan’s Winzerei, wo der Betrieb vorgestellt wurde und Wein verkosten werden konnte. Am 18. Februar verließ die Exkursionsgruppe Auckland in Richtung Norden, um zum Ort Puhoi zu gelangen. Dort beschäftigten sich die Teilnehmer mit den sogenannten Bohemians, die einst aus Böhmen nach Neuseeland auswanderten und deren Traditionen dort auch heute noch (zumindest teilweise) gepflegt werden. Am nächsten Tag fuhren sie weiter nach Pahia, dem nördlichsten Aufenthaltsort während der Exkursion. Auf dem Weg dorthin machten sie einen Umweg über Matakohe, wo das Kauri-Museum und der Tane Mahuta, der größte Kauribaum Neuseelands, besichtigt wurden. Am 20. Februar stand vormittags die Beschäftigung mit der Geschichte Neuseelands auf dem Tagesplan. Hierfür besuchte die Exkursionsgruppe die Waitangi Treaty Grounds. Dort informierten sich die Teilnehmer über den Vertrag von Waitangi und darüber, welche Folgen dieser für das Leben der Maori hatte. Am Nachmittag stand das Thema Tourismus im Mittelpunkt. Die Exkursionsteilnehmer machten sich mit einem Teil des touristischen Angebots vertraut, indem sie eine Bootstour durch die Bay of Islands unternahmen. Am 21. Februar fuhr die Gruppe in die Hamilton-Region, wo sie sich auch die folgenden zwei Tage aufhielt. Auf dem Weg dorthin wurde ein Zwischenstopp in Kawakawa und an den Whangarei Falls eingelegt. In Hamilton war die Exkursionsgruppe Gast im Geographischen Institut der Waikato University und im Waikato Migrant Resource Centre. Außerdem stand das Thema Milchwirtschaft auf dem Programm. Hierfür besichtigten die Teilnehmer das Unternehmen AmBreed, welches die Grundlage für die Aufzucht von Hochleistungsmilchkühen bereitstellt – nämlich das Bullensperma. Außerdem konnten sie sich über die Organisation und Probleme einer Milchfarm informieren. Darüber hinaus gestalteten in der Waikato-Region wohnende Nachfahren der böhmischen Einwanderer ein Abendprogramm für die Exkursionsgruppe. Den 24. Februar verbrachten die Teilnehmer im Gebiet von Rotorua. Dort durchkreuzten sie das Thermal Wonderland, in dem heiße Quellen und Geysire sowie die dadurch geschaffenen Oberflächengegebenheiten studiert werden können. Die heißen Quellen werden hier auch zur Energiegewinnung herangezogen, wovon sich die Exkursionsteilnehmer bei einer Besichtigung der Geothermal Power Station of Warakei überzeugen konnten. Auf der Fahrt zum Tongariro Nationalpark bewunderten sie die Huka Falls und machten Halt am Lake Taupo, dem größten See Neuseelands. Im Nationalpark unternahmen sie am 26. Februar eine Wanderung. Tags darauf fuhren sie weiter über Marton nach Wellington, der Hauptstadt Neuseelands. Dort war nachmittags sowie am 28. Februar Gelegenheit, die Stadt zu erkunden, unter anderem auf einer Stadtführung mit Prof. Bredlich. Daneben erfuhr man bei einem Besuch des neuseeländischen Nationalmuseums Te Papa viel Wissenswertes über Gesellschaft und Geschichte Neuseelands. Am 1. März überquerten sie mit der Fähre die Cookstraße, um zur Südinsel zu gelangen. Den Nachmittag dieses Tages verbrachte die Exkursionsgruppe in Upper Moutere, wo sie sich mit der Einwanderung Deutscher in der Region Nelson befasste Am Tag darauf fuhren die Teilnehmer zur Westküste und beschäftigten sich mit den Landschaftsformen der Südalpen und der Küste sowie mit der Frage, welche wirtschaftliche Rolle diese Region einst spielte und welche sie heute einnimmt. Am 3. März überquerten sie die Südalpen über den Athur’s Pass und kamen am Nachmittag in Christchurch an. Am nächsten Tag erlebten sie eine Besichtigungstour durch die größte Stadt der Südinsel unter Leitung von Prof. Parson vom Institut für Geographie der Universität von Canterbury. Dabei standen insbesondere Fragen des städtischen Wandels im Mittelpunkt, welcher mit den ökonomischen Reformen seit Ende der 80er Jahre des letzten Jahrhunderts einherging. Damit endete am 4. März die Exkursion in Christchurch. Zum zweiten Teil des Berichts – die thematischen Texte Neben dem Gewinn eines ersten Eindrucks vor Ort bietet eine Exkursion als Form der Erkundung eines Landes durchaus auch die Gelegenheit, kritisch über gesellschaftliche Vorgänge zu reflektieren. Über solche Reflexionen geben die Darstellungen im zweiten Teil dieses Exkursionsberichtes Aufschluss. Das Spektrum der in den Texten aufgegriffenen Themen reicht dabei von physisch-geographischen Gegebenheiten, über Land- und Forstwirtschaft, die Maori bis zu bevölkerungsgeographischen Fragestellungen zur Migration und Integration in Neuseeland. Dem zu Grunde liegt ein – in der Geographie lange verwurzeltes – holistisches Verständnis der Disziplin. In den Berichten findet die zentrale Debatte in der Geographie um die Bedeutung und das Zusammenspiel von globalen, regionsunabhängigen und lokalen, regionsspezifischen Faktoren (»Glokalisierung«) an vielen Stellen ihren Ausdruck. Da während der Exkursion Einblick in verschiedenste Bereiche des Lebens in Neuseeland gewonnen werden konnten, ist es im thematischen zweiten Teil des Berichts vorrangiges Ziel, einen guten Überblick über Neuseeland und seine Bevölkerung zu geben. Dabei überwiegt ein beschreibender Charakter der Texte, gleichzeitig sollen aber auch zentrale Veränderungen und Herausforderungen für die neuseeländische Gesellschaft angesprochen, Erklärungsansätze gegeben und Lösungsstrategien aufgewiesen werden. Im Einzelnen ist der thematische Teil folgendermaßen aufgebaut: Zu Beginn widmet sich Anja Lehmann den Maori und beleuchtet Geschichte, Kultur und heutige Situation der indigenen Bevölkerung Neuseelands. Anschließend gehen Katharina Popig und Manuel Hundt in ihrem Text auf die frühe europäische Einwanderung nach Neuseeland, insbesondere auf die Rolle der deutschen bzw. böhmischen Einwanderer, ein. Im darauf folgenden Text zeigt Manuel Hundt die sich verändernden Muster in der jüngeren Migration auf und beleuchtet Fragen der Integration in Neuseeland, wobei insbesondere auf die Rolle der Pacific Islanders eingegangen wird. Dann folgt der Text von Lilli Maier. Sie beschäftigt sich mit Fragen des Tourismus und schildert die Gestalt des Fremdenverkehrs und seine Bedeutung für die neuseeländische Wirtschaft. Natalia Kiselgof gibt einen Überblick sowohl über physisch-geographische Aspekte und den Naturraum Neuseelands als auch über die Struktur der neuseeländischen Landwirtschaft, bevor Sören Sturm die Forstwirtschaft Neuseelands einer kritischen Analyse unterzieht.
The power of apology
(2010)
As digital media infiltrate an increasingly greater proportion of our lives, concern about the possibility of various forms of technology addictions has emerged. For technology addiction, researchers have developed a variety of self-reported scales in areas such as Internet, smartphones, videogames, social network sites (SNS) or television. However, no uniform criteria or definition exists for technology addiction. Utilized dimensions of technology addiction, to measure specific outcomes, lack a conceptual standard. Therefore, linkages between technology areas dimensions have not been examined in a broader way by the research community, in order to develop a uniform technology addiction scale.
In this regard, firstly, a theoretical model was developed in order to extract common technology dimensions. Secondly, a systematic literature review in the areas of Internet, smartphone, video games and SNS was conducted in order to extract the dimensions used. To identify relevant studies, nine databases (GoogleScholar, ScienceDirect, PubMed, EmeraldInsight, Wiley, SpringerLink, ACM, iEEE and JSTOR) were searched, producing 4698 results, and 50 studies met the inclusion criteria. Thirdly, the developed theoretical model was utilized in order to determine the dimension in each of the identified scales.
Based on analysis of the dimensional distributions, the findings suggest that there are common dimensions across areas of technology such as “compulsive use” and “negative outcomes” but also differences in dimensions across areas such as “social comfort” and “mood regulation”, which are more used in the area of SNS. Moreover, new dimensions such as “cognitive absorption” or “utility and function loss" for technology addiction were extracted, which should be considered as these have not yet been researched in a broader way. In addition, no gold standard for the conceptual criteria or definition for technology addiction has been developed yet.
Enterprise Resource Planning (ERP) system customization is often necessary because companies have unique processes that provide their competitive advantage. Despite new technological advances such as cloud computing or model-driven development, technical ERP customization options are either outdated or ambiguously formulated in the scientific literature. Using a systematic literature review (SLR) that analyzes 137 definitions from 26 papers, the result is an analysis and aggregation of technical customization types by providing clearance and aligning with future organizational needs. The results show a shift from ERP code modification in on-premises systems to interface and integration customization in cloud ERP systems, as well as emerging technological opportunities as a way for customers and key users to perform system customization. The study contributes by providing a clear understanding of given customization types and assisting ERP users and vendors in making customization decisions.
The internet offers citizens new possibilities to participate in political communication by setting topics on the agenda of public discussion that are neglected by the conventional media. The article examines if and how the topics of the new emerging political public on the web differ from the topics generated by traditional media. The empirical analysis reveals that the topics are mostly the same. However, the analysis also shows that a clear separate public sphere exists that deals with topics outside the political mainstream.
This article documents the addition of 283 microsatellite marker loci to the Molecular Ecology Resources Database. Loci were developed for the following species: Agalinis acuta; Ambrosia artemisiifolia; Berula erecta; Casuarius casuarius; Cercospora zeae-maydis; Chorthippus parallelus; Conyza canadensis; Cotesia sesamiae; Epinephelus acanthistius; Ficedula hypoleuca; Grindelia hirsutula; Guadua angustifolia; Leucadendron rubrum; Maritrema novaezealandensis; Meretrix meretrix; Nilaparvata lugens; Oxyeleotris marmoratus; Phoxinus neogaeus; Pristomyrmex punctatus; Pseudobagrus brevicorpus; Seiridium cardinale; Stenopsyche marmorata; Tetranychus evansi and Xerus inauris. These loci were cross-tested on the following species: Agalinis decemloba; Agalinis tenella; Agalinis obtusifolia; Agalinis setacea; Agalinis skinneriana; Cercospora zeina; Cercospora kikuchii; Cercospora sorghi; Mycosphaerella graminicola; Setosphaeria turcica; Magnaporthe oryzae; Cotesia flavipes; Cotesia marginiventris; Grindelia Xpaludosa; Grindelia chiloensis; Grindelia fastigiata; Grindelia lanceolata; Grindelia squarrosa; Leucadendron coniferum; Leucadendron salicifolium; Leucadendron tinctum; Leucadendron meridianum; Laodelphax striatellus; Sogatella furcifera; Phoxinus eos; Phoxinus rigidus; Phoxinus brevispinosus; Phoxinus bicolor; Tetranychus urticae; Tetranychus turkestani; Tetranychus ludeni; Tetranychus neocaledonicus; Tetranychus amicus; Amphitetranychus viennensis; Eotetranychus rubiphilus; Eotetranychus tiliarium; Oligonychus perseae; Panonychus citri; Bryobia rubrioculus; Schizonobia bundi; Petrobia harti; Xerus princeps; Spermophilus tridecemlineatus and Sciurus carolinensis.
Indoor mesocosm experiments were conducted to test for potential climate change effects on the spring succession of Baltic Sea plankton. Two different temperature (Delta 0 A degrees C and Delta 6 A degrees C) and three light scenarios (62, 57 and 49 % of the natural surface light intensity on sunny days), mimicking increasing cloudiness as predicted for warmer winters in the Baltic Sea region, were simulated. By combining experimental and modeling approaches, we were able to test for a potential dietary mismatch between phytoplankton and zooplankton. Two general predator-prey models, one representing the community as a tri-trophic food chain and one as a 5-guild food web were applied to test for the consequences of different temperature sensitivities of heterotrophic components of the plankton. During the experiments, we observed reduced time-lags between the peaks of phytoplankton and protozoan biomass in response to warming. Microzooplankton peak biomass was reached by 2.5 day A degrees C-1 earlier and occurred almost synchronously with biomass peaks of phytoplankton in the warm mesocosms (Delta 6 A degrees C). The peak magnitudes of microzooplankton biomass remained unaffected by temperature, and growth rates of microzooplankton were higher at Delta 6 A degrees C (mu(a dagger 0 A degrees C) = 0.12 day(-1) and mu(a dagger 6 A degrees C) = 0.25 day(-1)). Furthermore, warming induced a shift in microzooplankton phenology leading to a faster species turnover and a shorter window of microzooplankton occurrence. Moderate differences in the light levels had no significant effect on the time-lags between autotrophic and heterotrophic biomass and on the timing, biomass maxima and growth rate of microzooplankton biomass. Both models predicted reduced time-lags between the biomass peaks of phytoplankton and its predators (both microzooplankton and copepods) with warming. The reduction of time-lags increased with increasing Q(10) values of copepods and protozoans in the tritrophic food chain. Indirect trophic effects modified this pattern in the 5-guild food web. Our study shows that instead of a mismatch, warming might lead to a stronger match between protist grazers and their prey altering in turn the transfer of matter and energy toward higher trophic levels.
A series of polystyrene-block-poly(1,2-butadiene)-block-poly(2-vinyl-pyridine) (SBV) triblock terpolymers were used to prepare blends with symmetric polystyrene-block-poly(2-vinylpyridine) (SV) and poly(2-vinylpyridine)-block-poly- (cyclohexyl methacrylate) (VC) diblock copolymers. Morphological characterization was carried out by transmission electron microscopy. These triblock terpolymers self-assemble into various core-shell type or lamellar morphologies. In the SBV/SV blends, macrophase separation between the two block copolymers, continuous centrosymmetric lamellae and stacks of non-centrosymmetric lamellae with anti-parallel orientation were found. In the blends of SBV/VC, macrophase separation was never observed, what is due to the specific interactions between S and C domains. These systems showed among other morphologies also a cylindrical morphology in which rings surround the cylinders
We present results from multiwavelength observations of the BL Lacertae object 1ES 1741 + 196, including results in the very high energy gamma-ray regime using the Very Energetic Radiation Imaging Telescope Array System (VERITAS). The VERITAS time-averaged spectrum, measured above 180 GeV, is well modelled by a power law with a spectral index of 2.7 +/- 0.7(stat) +/- 0.2(syst). The integral flux above 180 GeV is (3.9 +/- 0.8(stat) +/- 1.0(syst)) x 10(-8) m(-2) s(-1), corresponding to 1.6 per cent of the Crab nebula flux on average. The multiwavelength spectral energy distribution of the source suggests that 1ES 1741+196 is an extreme-high-frequency-peaked BL Lacertae object. The observations analysed in this paper extend over a period of six years, during which time no strong flares were observed in any band. This analysis is therefore one of the few characterizations of a blazar in a non-flaring state.
Discovery of Very-high-energy Emission from RGB J2243+203 and Derivation of Its Redshift Upper Limit
(2017)
Very-high-energy (VHE; > 100 GeV) gamma-ray emission from the blazar RGB J2243+203 was discovered with the VERITAS Cherenkov telescope array, during the period between 2014 December 21 and 24. The VERITAS energy spectrum from this source can be fitted by a power law with a photon index of 4.6 +/- 0.5, and a flux normalization at 0.15 TeV of (6.3 +/- 1.1) x 10(-10) cm(-2) s(-1) TeV-1. The integrated Fermi-LAT flux from 1 to 100 GeV during the VERITAS detection is (4.1 +/- 0.8) x 10(-8) cm(-2) s(-1), which is an order of magnitude larger than the four-year-averaged flux in the same energy range reported in the 3FGL catalog, (4.0 +/- 0.1 x 10(-9) cm(-2) s(-1)). The detection with VERITAS triggered observations in the X-ray band with the Swift-XRT. However, due to scheduling constraints Swift-XRT observations were performed 67 hr after the VERITAS detection, rather than simultaneously with the VERITAS observations. The observed X-ray energy spectrum between 2 and 10 keV can be fitted with a power law with a spectral index of 2.7 +/- 0.2, and the integrated photon flux in the same energy band is (3.6 +/- 0.6) x 10(-13) cm(-2) s(-1). EBL-model-dependent upper limits of the blazar redshift have been derived. Depending on the EBL model used, the upper limit varies in the range from z < 0.9 to z < 1.1.
The F-type star KIC. 8462852 has recently been identified as an exceptional target for search for extraterrestrial intelligence (SETI) observations. We describe an analysis methodology for optical SETI, which we have used to analyze nine hours of serendipitous archival observations of KIC. 8462852 made with the VERITAS gamma-ray observatory between 2009 and 2015. No evidence of pulsed optical beacons, above a pulse intensity at the Earth of approximately 1 photon m(-2), is found. We also discuss the potential use of imaging atmospheric Cherenkov telescope arrays in searching for extremely short duration optical transients in general.
B2 1215+30 is a BL-Lac-type blazar that was first detected at TeV energies by the MAGIC atmospheric Cherenkov telescopes and subsequently confirmed by the Very Energetic Radiation Imaging Telescope Array System (VERITAS) observatory with data collected between 2009 and 2012. In 2014 February 08, VERITAS detected a large-amplitude flare from B2. 1215+30 during routine monitoring observations of the blazar 1ES. 1218+304, located in the same field of view. The TeV flux reached 2.4 times the Crab Nebula flux with a variability timescale of <3.6 hr. Multiwavelength observations with Fermi-LAT, Swift, and the Tuorla Observatory revealed a correlated high GeV flux state and no significant optical counterpart to the flare, with a spectral energy distribution where the gamma-ray luminosity exceeds the synchrotron luminosity. When interpreted in the framework of a onezone leptonic model, the observed emission implies a high degree of beaming, with Doppler factor delta > 10, and an electron population with spectral index p < 2.3.
We present results from deep observations toward the Cygnus region using 300 hr of very high energy (VHE)gamma-ray data taken with the VERITAS Cerenkov telescope array and over 7 yr of high-energy.-ray data taken with the Fermi satellite at an energy above 1 GeV. As the brightest region of diffuse gamma-ray emission in the northern sky, the Cygnus region provides a promising area to probe the origins of cosmic rays. We report the identification of a potential Fermi-LAT counterpart to VER J2031+415 (TeV J2032+4130) and resolve the extended VHE source VER J2019+368 into two source candidates (VER J2018+367* and VER J2020+368*) and characterize their energy spectra. The Fermi-LAT morphology of 3FGL J2021.0+4031e (the Gamma Cygni supernova remnant) was examined, and a region of enhanced emission coincident with VER J2019+407 was identified and jointly fit with the VERITAS data. By modeling 3FGL J2015.6+3709 as two sources, one located at the location of the pulsar wind nebula CTB 87 and one at the quasar QSO J2015+371, a continuous spectrum from 1 GeV to 10 TeV was extracted for VER J2016+371 (CTB 87). An additional 71 locations coincident with Fermi-LAT sources and other potential objects of interest were tested for VHE gamma-ray emission, with no emission detected and upper limits on the differential flux placed at an average of 2.3% of the Crab Nebula flux. We interpret these observations in a multiwavelength context and present the most detailed gamma-ray view of the region to date.
The extragalactic background light (EBL), a diffuse photon field in the optical and infrared range, is a record of radiative processes over the universe?s history. Spectral measurements of blazars at very high energies (>100 GeV) enable the reconstruction of the spectral energy distribution (SED) of the EBL, as the blazar spectra are modified by redshift- and energy-dependent interactions of the gamma-ray photons with the EBL. The spectra of 14 VERITAS-detected blazars are included in a new measurement of the EBL SED that is independent of EBL SED models. The resulting SED covers an EBL wavelength range of 0.56?56 ?m, and is in good agreement with lower limits obtained by assuming that the EBL is entirely due to radiation from cataloged galaxies.
On 2017 September 22, the IceCube Neutrino Observatory reported the detection of the high-energy neutrino event IC 170922A, of potential astrophysical origin. It was soon determined that the neutrino direction was consistent with the location of the gamma-ray blazar TXS 0506+056. (3FGL J0509.4+ 0541), which was in an elevated gamma-ray emission state as measured by the Fermi satellite. Very Energetic Radiation Imaging Telescope Array System (VERITAS) observations of the neutrino/blazar region started on 2017 September 23 in response to the neutrino alert and continued through 2018 February 6. While no significant very-high-energy (VHE; E > 100 GeV) emission was observed from the blazar by VERITAS in the two-week period immediately following the IceCube alert, TXS 0506+ 056 was detected by VERITAS with a significance of 5.8 standard deviations (sigma) in the full 35 hr data set. The average photon flux of the source during this period was (8.9 +/- 1.6). x. 10(-12) cm(-2) s(-1), or 1.6% of the Crab Nebula flux, above an energy threshold of 110 GeV, with a soft spectral index of 4.8. +/-. 1.3.
VERITAS and Fermi-LAT Observations of TeV Gamma-Ray Sources Discovered by HAWC in the 2HWC Catalog
(2018)
The High Altitude Water Cherenkov (HAWC) collaboration recently published their 2HWC catalog, listing 39 very high energy (VHE; >100 GeV) gamma-ray sources based on 507 days of observation. Among these, 19 sources are not associated with previously known teraelectronvolt (TeV) gamma-ray sources. We have studied 14 of these sources without known counterparts with VERITAS and Fermi-LAT. VERITAS detected weak gamma-ray emission in the 1 TeV-30 TeV band in the region of DA 495, a pulsar wind nebula coinciding with 2HWC J1953+294, confirming the discovery of the source by HAWC. We did not find any counterpart for the selected 14 new HAWC sources from our analysis of Fermi-LAT data for energies higher than 10 GeV. During the search, we detected gigaelectronvolt (GeV) gamma-ray emission coincident with a known TeV pulsar wind nebula, SNR G54.1+0.3 (VER J1930+188), and a 2HWC source, 2HWC J1930+188. The fluxes for isolated, steady sources in the 2HWC catalog are generally in good agreement with those measured by imaging atmospheric Cherenkov telescopes. However, the VERITAS fluxes for SNR G54.1+0.3, DA 495, and TeV J2032+4130 are lower than those measured by HAWC, and several new HAWC sources are not detected by VERITAS. This is likely due to a change in spectral shape, source extension, or the influence of diffuse emission in the source region.
On 2015 March 23, the Very Energetic Radiation Imaging Telescope Array System (VERITAS) responded to a Swift-Burst Alert Telescope (BAT) detection of a gamma-ray burst, with observations beginning 270 s after the onset of BAT emission, and only 135 s after the main BAT emission peak. No statistically significant signal is detected above 140 GeV. The VERITAS upper limit on the fluence in a 40-minute integration corresponds to about 1% of the prompt fluence. Our limit is particularly significant because the very-high-energy (VHE) observation started only similar to 2 minutes after the prompt emission peaked, and Fermi-Large Area Telescope observations of numerous other bursts have revealed that the high-energy emission is typically delayed relative to the prompt radiation and lasts significantly longer. Also, the proximity of GRB 150323A (z = 0.593) limits the attenuation by the extragalactic background light to similar to 50% at 100-200 GeV. We conclude that GRB 150323A had an intrinsically very weak high-energy afterglow, or that the GeV spectrum had a turnover below similar to 100 GeV. If the GRB exploded into the stellar wind of a massive progenitor, the VHE non-detection constrains the wind density parameter to be A greater than or similar to 3 x 10(11) g . cm(-1), consistent with a standard Wolf-Rayet progenitor. Alternatively, the VHE emission from the blast wave would be weak in a very tenuous medium such as the interstellar medium, which therefore cannot be ruled out as the environment of GRB 150323A.
Combined with measurements made by very-long-baseline interferometry, the observations of fast TeV gamma-ray flares probe the structure and emission mechanism of blazar jets. However, only a handful of such flares have been detected to date, and only within the last few years have these flares been observed from lower-frequency-peaked BL. Lac objects and flat-spectrum radio quasars. We report on a fast TeV gamma-ray flare from the blazar BL. Lacertae observed by the Very Energetic Radiation Imaging Telescope Array System (VERITAS). with a rise time of similar to 2.3 hr and a decay time of similar to 36 min. The peak flux above 200 GeV is (4.2 +/- 0.6) x 10(-6) photon m(-2) s(-1) measured with a 4-minute-binned light curve, corresponding to similar to 180% of the flux that is observed from the Crab Nebula above the same energy threshold. Variability contemporaneous with the TeV gamma-ray flare was observed in GeV gamma-ray, X-ray, and optical flux, as well as in optical and radio polarization. Additionally, a possible moving emission feature with superluminal apparent velocity was identified in Very Long Baseline Array observations at 43 GHz, potentially passing the radio core of the jet around the time of the gamma-ray flare. We discuss the constraints on the size, Lorentz factor, and location of the emitting region of the flare, and the interpretations with several theoretical models that invoke relativistic plasma passing stationary shocks.
We report on observations of the pulsar/Be star binary system PSR J2032+4127/MT91 213 in the energy range between 100 GeV and 20 TeV with the Very Energetic Radiation Imaging Telescope Array and Major Atmospheric Gamma Imaging Cherenkov telescope arrays. The binary orbit has a period of approximately 50 years, with the most recent periastron occurring on 2017 November 13. Our observations span from 18 months prior to periastron to one month after. A new point-like gamma-ray source is detected, coincident with the location of PSR J2032+4127/MT91 213. The gamma-ray light curve and spectrum are well characterized over the periastron passage. The flux is variable over at least an order of magnitude, peaking at periastron, thus providing a firm association of the TeV source with the pulsar/Be star system. Observations prior to periastron show a cutoff in the spectrum at an energy around 0.5 TeV. This result adds a new member to the small population of known TeV binaries, and it identifies only the second source of this class in which the nature and properties of the compact object are firmly established. We compare the gamma-ray results with the light curve measured with the X-ray Telescope on board the Neil Gehrels Swift Observatory and with the predictions of recent theoretical models of the system. We conclude that significant revision of the models is required to explain the details of the emission that we have observed, and we discuss the relationship between the binary system and the overlapping steady extended source, TeV J2032+4130.
We characterize finite-time thermodynamic processes of multidimensional quadratic overdamped systems.
Analytic expressions are provided for heat, work, and dissipation for any evolution of the system covariance matrix.
The Bures-Wasserstein metric between covariance matrices naturally emerges as the local quantifier of dissipation.
General principles of how to apply these geometric tools to identify optimal protocols are discussed.
Focusing on the relevant slow-driving limit, we show how these results can be used to analyze cases in which the experimental control over the system is partial.
Dieser Beitrag stellt das Lehr-Lern-Konzept zur Kompetenzförderung im Software Engineering im Studiengang Mechatronik der Hochschule Aschaffenburg dar. Dieses Konzept ist mehrstufig mit Vorlesungs-, Seminar- und Projektsequenzen. Dabei werden Herausforderungen und Verbesserungspotentiale identifiziert und dargestellt. Abschließend wird ein Überblick gegeben, wie im Rahmen eines gerade gestarteten Forschungsprojektes Lehr-Lernkonzepte weiterentwickelt werden können.
This case study evaluates the suitability of radar-based quantitative precipitation estimates (QPEs) for the simulation of streamflow in the Marikina River Basin (MRB), the Philippines. Hourly radar-based QPEs were produced from reflectivity that had been observed by an S-band radar located about 90 km from the MRB. Radar data processing and precipitation estimation were carried out using the open source library wradlib. To assess the added value of the radar-based QPE, we used spatially interpolated rain gauge observations (gauge-only (GO) product) as a benchmark. Rain gauge observations were also used to quantify rainfall estimation errors at the point scale. At the point scale, the radar-based QPE outperformed the GO product in 2012, while for 2013, the performance was similar. For both periods, estimation errors substantially increased from daily to the hourly accumulation intervals. Despite this fact, both rainfall estimation methods allowed for a good representation of observed streamflow when used to force a hydrological simulation model of the MRB. Furthermore, the results of the hydrological simulation were consistent with rainfall verification at the point scale: the radar-based QPE performed better than the GO product in 2012, and equivalently in 2013. Altogether, we could demonstrate that, in terms of streamflow simulation, the radar-based QPE can perform as good as or even better than the GO product - even for a basin such as the MRB which has a comparatively dense rain gauge network. This suggests good prospects for using radar-based QPE to simulate and forecast streamflow in other parts of the Philippines where rain gauge networks are not as dense.
Die vorliegende Arbeit trägt den Titel: Intellektuellen-Rolle in Günter Grass Werken : „Die Plebejer proben den Aufstand“(1966), „Örtlich betäubt“(1969), „Aus dem Tagebuch einer Schnecke“(1972), und „Ein weites Feld“(1995).
Das erste Kapitel befasst sich insgesamt mit drei Haupttiteln
II. Der Intellektuelle
II.1 Das allgemeine Umfeld
In diesem Teil der Dissertation sollen Aussagen getroffen werden, die auf folgende und weitere Fragen eine Antwort geben: Was ist ein Intellektueller? Wie kam der Begriff zustande? Gibt es Unterschiede zwischen den Intellektuellen und wie werden sie eingeteilt?
II.2 Das deutsche Umfeld
Die Behandlung des Nazisystems und dessen historische Hintergründe vermittelt bedeutsame Lehren. Aber wozu braucht man diese Lehren? Gibt es Spuren von Nationalsozialismus heutzutage? Wo waren die Intellektuellen bei der Bildung des Nationalsozialismus? Ist der Nationalsozialismus erst mit Hitler aufgetaucht? Wenn zuvor, in welcher Phase hat er sich im Bewusstsein der Deutschen verankert? Ob theoretische bzw. geistige Tendenzen dazu beigetragen haben?
II.3 Das Bild von Grass als Intellektueller
II.3.1 Positionierung
Eine Hauptthese für Grass intellektuelle Positionierung wird durch die Verbindung zwischen Grass’ Grundkonzeption der gesellschaftspolitischen Intellektualität und der Gruppe 47 ermittelt. Dann bezweckt die Behandlung von Grass Bild nach Erscheinen seines autobiographischen Werks: „Beim Häuten der Zwiebel“ (2006), dass seine Intellektualität nicht nur aus dem positiven, sondern auch aus dem negativen Profil beleuchtet wird.
Aus der Darstellung zahlreicher Ansichten von Günter Grass werden fünf thematische Kernpunkte als Konzepte behandelt. Unter jedem Konzept sollen spezifische Vorschläge zur gesellschaftlichen Positionierung aufgezeigt werden.
II.3.2 Grass’ politische Merkmale
Es handelt sich hier um die intellektuellen Charaktereigenschaften. Dadurch kommen manche Fragen zu Wort: Hat Günter Grass gesellschaftliche Aktivitäten? Hat er die Voraussetzungen dafür? Wie ist der Umfang seiner Aktivitäten? Hat die Gruppe 47 Einfluss auf Grass intellektuelle Merkmale? Steht bei Grass eine Methode der gesellschaftspolitischen Arbeit zur Verfügung?
Dann wird die politische Sprache von Günter Grass und ihre Wirkung auf den Rezipienten untersucht. Danach wird nach Grass’ Auffassung von der Revision gefragt und ob sie mit seiner Auffassung der Aufklärung zusammenpasst. Darauf wird die Funktion der Revision in seinem literarischen Werk und in seiner gesellschaftspolitischen Aktivität gezeigt.
Abschließend werden die Argumente seiner Intellektualität untersucht:
Wie hat Grass’ gesellschaftspolitische Aktivität den konkreten politischen Rahmen berücksichtigt? Um diese Frage zu beantworten, muss der Zusammenhang zwischen Politik und Moral verdeutlicht werden.
III. Historischer Kontext und Inhalt der Werke
Unter diesem Titel wird erstens der historische Zusammenhang der untersuchten Werke skizziert. Dann werden meistens durch Argumente aus jedem Werk selbst nicht nur der Kern des Werkes und sein Handlungsverlauf, sondern auch die dafür angewandte Methode dargestellt.
IV. Bezug der untersuchten Werke zu konkreten gesellschaftspolitischen Fragen
IV.1 Interaktionswege des Intellektuellen mit der Gesellschaft, vor allem beim Wandel gesellschaftspolitischer Prozesse
Zentralkonzepte des ersten Werkes sind: Vermittlung, Engagement, Solidarität und die Aktualität als Maßstab. Diese werden durch zwei Konzepte des zweiten Werkes: Appell an Generationen beim Wechsel und Zusammenhaltsprinzip an Revision gebunden, sowie durch die Behandlung vom Prozess der Meinungsbildung im vierten Werk ausgearbeitet.
IV.2 Thematische Aspekte zur Vermeidung eines Naziregimes
Aus den thematischen Perspektiven der drei letzten Werke geht eine bunte Sammlung intellektueller Konzepte aus, die zur Bekämpfung von Nazivorsprünge verwendet werden können.
V. Pädagogische Strategien der untersuchten Werke
Die pädagogischen Aspekte der untersuchten Werke sollen intellektuelle Werte vermitteln, die einen bedeutenden Beitrag zur Lösung gesellschaftspolitischer Probleme und Konflikte leisten.
VI. Entwicklung der literarischen und gesellschaftspolitischen Vision
Hier wird die Entwicklungslinie der gesellschaftspolitischen Vision in den untersuchten Werken verfolgt.
VII. Zur Rezeption der vier Werke
Durch die Auseinandersetzung mit der negativen Kritik wird angestrebt, ihre Subjektivität darzulegen, damit der gesellschaftspolitische Wert der vier Werke enthüllt wird.
Health effects, attributed to the environmental pollution resulted from using solvents such as benzene, are relatively unexplored among petroleum workers, personal use, and laboratory researchers. Solvents can cause various health problems, such as neurotoxicity, immunotoxicity, and carcinogenicity. As such it can be absorbed via epidermal or respiratory into the human body resulting in interacting with molecules that are responsible for biochemical and physiological processes of the brain.
Owing to the ever-growing demand for finding a solution, an Ionic liquid can use as an alternative solvent. Ionic liquids are salts in a liquid state at low temperature (below 100 C), or even at room temperature. Ionic liquids impart a unique architectural platform, which has been interesting because of their unusual properties that can be tuned by simple ways such as mixing two ionic liquids.
Ionic liquids not only used as reaction solvents but they became a key developing for novel applications based on their thermal stability, electric conductivity with very low vapor pressure in contrast to the conventional solvents.
In this study, ionic liquids were used as a solvent and reactant at the same time for the novel nanomaterials synthesis for different applications including solar cells, gas sensors, and water splitting.
The field of ionic liquids continues to grow, and become one of the most important branches of science. It appears to be at a point where research and industry can work together in a new way of thinking for green chemistry and sustainable production.
Six N-alkylpyridinium salts [CnPy](2)[MCl4] (n = 4 or 12 and M = Co, Cu, Zn) were synthesized, and their structure and thermal properties were studied. The [C4Py](2)[MCl4] compounds are monoclinic and crystallize in the space group P2(1)/n. The crystals of the longer chain analogues [C12Py](2)[MCl4] are triclinic and crystallize in the space group P (1) over bar. Above the melting temperature, all compounds are ionic liquids (ILs). The derivatives with the longer C12 chain exhibit liquid crystallinity and the shorter chain compounds only show a melting transition. Consistent with single-crystal analysis, electron paramagnetic resonance spectroscopy suggests that the [CuCl4](2-) ions in the Cu-based ILs have a distorted tetrahedral geometry.
Six N-alkylpyridinium salts [CnPy](2)[MCl4] (n = 4 or 12 and M = Co, Cu, Zn) were synthesized, and their structure and thermal properties were studied. The [C4Py](2)[MCl4] compounds are monoclinic and crystallize in the space group P2(1)/n. The crystals of the longer chain analogues [C12Py](2)[MCl4] are triclinic and crystallize in the space group P (1) over bar. Above the melting temperature, all compounds are ionic liquids (ILs). The derivatives with the longer C12 chain exhibit liquid crystallinity and the shorter chain compounds only show a melting transition. Consistent with single-crystal analysis, electron paramagnetic resonance spectroscopy suggests that the [CuCl4](2-) ions in the Cu-based ILs have a distorted tetrahedral geometry.
Label-free electrical detection of consecutive deoxyribonucleic acid (DNA) hybridization/denaturation by means of an array of individually addressable field-effect-based nanoplate silicon-on-insulator (SOI) capacitors modified with gold nanoparticles (Au-NP) is investigated. The proposed device detects charge changes on Au-NP/DNA hybrids induced by the hybridization or denaturation event. DNA hybridization was performed in a high ionic-strength solution to provide a high hybridization efficiency. On the other hand, to reduce the screening of the DNA charge by counter ions and to achieve a high sensitivity, the sensor signal induced by the hybridization and denaturation events was measured in a low ionic-strength solution. High sensor signals of about 120, 90, and 80 mV were registered after the DNA hybridization, denaturation, and re-hybridization events, respectively. Fluorescence microscopy has been applied as reference method to verify the DNA immobilization, hybridization, and denaturation processes. An electrostatic charge-plane model for potential changes at the gate surface of a nanoplate field-effect sensor induced by the DNA hybridization has been developed taking into account both the Debye length and the distance of the DNA charge from the gate surface.
Stress inoculation facilitates active avoidance learning of the semi-precocial rodent Octodon degus
(2010)
A growing body of evidence highlights the impact of the early social environment for the adequate development of brain and behavior in animals and humans. Disturbances of this environment were found to be both maladaptive and adaptive to emotional and cognitive function. Using the semi-precocial, biparental rodent Octodon degus, we aimed to examine (i) the impact of age (juvenile/adult), sex (male/female), and (ii) "motivation" to solve the task (by applying increasing foot-shock-intensities) on two-way active avoidance (TWA) learning in socially reared degus, and (iii) whether early life stress inoculation by 1 h daily parental separation during the first three weeks of life has maladaptive or adaptive consequences on cognitive function as measured by TWA learning. Our results showed that (i) juvenile degus, unlike altricial rats of the same age, can successfully learn the TWA task comparable to adults, and (ii) that learning performance improves with increasing "task motivation", irrespective of age and sex. Furthermore, we revealed that (iii) stress inoculation improves avoidance learning, particularly in juvenile males, quantitatively and qualitatively depending on "task motivation". In conclusion, the present study describes for the first time associative learning in O. degus and its modulation by early life stress experience as an animal model to study the underlying mechanisms of learning and memory in the stressed and unstressed brain. Although, stress is commonly viewed as being maladaptive, our data indicate that early life stress inoculation triggers developmental cascades of adaptive functioning, which may improve cognitive and emotional processing of stressors later in life.
Pollination syndromes and their predictive power regarding actual plant-animal interactions have been controversially discussed in the past. We investigate pollination syndromes in Balsaminaceae, utilizing quantitative respectively categorical data sets of flower morphometry, signal and reward traits for 86 species to test for the effect of different types of data on the test patterns retrieved. Cluster Analyses of the floral traits are used in combination with independent pollinator observations. Based on quantitative data we retrieve seven clusters, six of them corresponding to plausible pollination syndromes and one additional, well-supported cluster comprising highly divergent floral architectures. This latter cluster represents a non-syndrome of flowers not segregated by the specific data set here used. Conversely, using categorical data we obtained only a rudimentary resolution of pollination syndromes, in line with several earlier studies. The results underscore that the use of functional, exactly quanitified trait data has the power to retrieve pollination syndromes circumscribed by the specific data used. Data quality can, however, not be replaced by sheer data volume. With this caveat, it is possible to identify pollination syndromes from large datasets and to reliably extrapolate them for taxa for which direct observations are unavailable.
Does a smile open all doors?
(2020)
Online photographs govern an individual’s choices across a variety of contexts. In sharing arrangements, facial appearance has been shown to affect the desire to collaborate, interest to explore a listing, and even willingness to pay for a stay. Because of the ubiquity of online images and their influence on social attitudes, it seems crucial to be able to control these aspects. The present study examines the effect of different photographic self-disclosures on the provider’s perceptions and willingness to accept a potential co-sharer. The findings from our experiment in the accommodation-sharing context suggest social attraction mediates the effect of photographic self-disclosures on willingness to host. Implications of the results for IS research and practitioners are discussed.
Sharing marketplaces emerged as the new Holy Grail of value creation by enabling exchanges between strangers. Identity reveal, encouraged by platforms, cuts both ways: While inducing pre-transaction confidence, it is suspected of backfiring on the information senders with its discriminative potential. This study employs a discrete choice experiment to explore the role of names as signifiers of discriminative peculiarities and the importance of accompanying cues in peer choices of a ridesharing offer. We quantify users' preferences for quality signals in monetary terms and evidence comparative disadvantage of Middle Eastern descent male names for drivers and co-travelers. It translates into a lower willingness to accept and pay for an offer. Market simulations confirm the robustness of the findings. Further, we discover that females are choosier and include more signifiers of involuntary personal attributes in their decision-making. Price discounts and positive information only partly compensate for the initial disadvantage, and identity concealment is perceived negatively.
Sharing marketplaces emerged as the new Holy Grail of value creation by enabling exchanges between strangers. Identity reveal, encouraged by platforms, cuts both ways: While inducing pre-transaction confidence, it is suspected of backfiring on the information senders with its discriminative potential. This study employs a discrete choice experiment to explore the role of names as signifiers of discriminative peculiarities and the importance of accompanying cues in peer choices of a ridesharing offer. We quantify users' preferences for quality signals in monetary terms and evidence comparative disadvantage of Middle Eastern descent male names for drivers and co-travelers. It translates into a lower willingness to accept and pay for an offer. Market simulations confirm the robustness of the findings. Further, we discover that females are choosier and include more signifiers of involuntary personal attributes in their decision-making. Price discounts and positive information only partly compensate for the initial disadvantage, and identity concealment is perceived negatively.
We used structural topic modeling to analyze over 800,000 German tweets about COVID-19 to answer the questions: What patterns emerge in tweets as a response to a health crisis? And how do topics discussed change over time? The study leans on the goals associated with the health information seeking (GAINS) model, discerning whether a post aims at tackling and eliminating the problem (i.e., problem-focused) or managing the emotions (i.e., emotion-focused); whether it strives to maximize positive outcomes (promotion focus) or to minimize negative outcomes (prevention focus). The findings indicate four clusters salient in public reactions: 1) “Understanding” (problem-promotion); 2) “Action planning” (problem-prevention); 3) “Hope” (emotion-promotion) and 4) “Reassurance” (emotion-prevention). Public communication is volatile over time, and a shift is evidenced from self-centered to community-centered topics within 4.5 weeks. Our study illustrates social media text mining's potential to quickly and efficiently extract public opinions and reactions. Monitoring fears and trending topics enable policymakers to rapidly respond to deviant behavior, like resistive attitudes toward containment measures or deteriorating physical health. Healthcare workers can use the insights to provide mental health services for battling anxiety or extensive loneliness from staying home.
During a crisis event, social media enables two-way communication and many-to-many information broadcasting, browsing others’ posts, publishing own content, and public commenting. These records can deliver valuable insights to approach problematic situations effectively. Our study explores how social media communication can be analyzed to understand the responses to health crises better. Results based on nearly 800 K tweets indicate that the coping and regulation foci framework holds good explanatory power, with four clusters salient in public reactions: 1) “Understanding” (problem-promotion); 2) “Action planning” (problem-prevention); 3) “Hope” (emotion-promotion) and 4) “Reassurance” (emotion-prevention). Second, the inter-temporal analysis shows high volatility of topic proportions and a shift from self-centered to community-centered topics during the course of the event. The insights are beneficial for research on crisis management and practicians who are interested in large-scale monitoring of their audience for well-informed decision-making.
Helping overcome distance, the use of videoconferencing tools has surged during the pandemic. To shed light on the consequences of videoconferencing at work, this study takes a granular look at the implications of the self-view feature for meeting outcomes. Building on self-awareness research and self-regulation theory, we argue that by heightening the state of self-awareness, self-view engagement depletes participants’ mental resources and thereby can undermine online meeting outcomes. Evaluation of our theoretical model on a sample of 179 employees reveals a nuanced picture. Self-view engagement while speaking and while listening is positively associated with self-awareness, which, in turn, is negatively associated with satisfaction with meeting process, perceived productivity, and meeting enjoyment. The criticality of the communication role is put forward: looking at self while listening to other attendees has a negative direct and indirect effect on meeting outcomes; however, looking at self while speaking produces equivocal effects.
With the surging reliance on videoconferencing tools, users may find themselves staring at their reflections for hours a day. We refer to this phenomenon as self-referential information (SRI) consumption and examine its consequences and the mechanism behind them. Building on self-awareness research and the strength model of self-control, we argue that SRI consumption heightens the state of self-awareness and thereby depletes participants’ mental resources, eventually undermining virtual meeting (VM) outcomes. Our findings from a European employee sample revealed contrary effects of SRI consumption across speaker vs listener roles. Engagement with self-view is positively associated with self-awareness, which, in turn, is negatively related to satisfaction with VM process, perceived productivity, and enjoyment. Looking at the self while listening to others exhibits adverse direct and indirect (via self-awareness) effects on VM outcomes. However, looking at the self when speaking exhibits positive direct effects on satisfaction with VM process and enjoyment.
Despite the phenomenal growth of Big Data Analytics in the last few years, little research is done to explicate the relationship between Big Data Analytics Capability (BDAC) and indirect strategic value derived from such digital capabilities. We attempt to address this gap by proposing a conceptual model of the BDAC - Innovation relationship using dynamic capability theory. The work expands on BDAC business value research and extends the nominal research done on BDAC – innovation. We focus on BDAC's relationship with different innovation objects, namely product, business process, and business model innovation, impacting all value chain activities. The insights gained will stimulate academic and practitioner interest in explicating strategic value generated from BDAC and serve as a framework for future research on the subject
One for all, all for one
(2022)
We propose a conceptual model of acceptance of contact tracing apps based on the privacy calculus perspective. Moving beyond the duality of personal benefits and privacy risks, we theorize that users hold social considerations (i.e., social benefits and risks) that underlie their acceptance decisions. To test our propositions, we chose the context of COVID-19 contact tracing apps and conducted a qualitative pre-study and longitudinal quantitative main study with 589 participants from Germany and Switzerland. Our findings confirm the prominence of individual privacy calculus in explaining intention to use and actual behavior. While privacy risks are a significant determinant of intention to use, social risks (operationalized as fear of mass surveillance) have a notably stronger impact. Our mediation analysis suggests that social risks represent the underlying mechanism behind the observed negative link between individual privacy risks and contact tracing apps' acceptance. Furthermore, we find a substantial intention–behavior gap.
One for all, all for one
(2022)
We propose a conceptual model of acceptance of contact tracing apps based on the privacy calculus perspective. Moving beyond the duality of personal benefits and privacy risks, we theorize that users hold social considerations (i.e., social benefits and risks) that underlie their acceptance decisions. To test our propositions, we chose the context of COVID-19 contact tracing apps and conducted a qualitative pre-study and longitudinal quantitative main study with 589 participants from Germany and Switzerland. Our findings confirm the prominence of individual privacy calculus in explaining intention to use and actual behavior. While privacy risks are a significant determinant of intention to use, social risks (operationalized as fear of mass surveillance) have a notably stronger impact. Our mediation analysis suggests that social risks represent the underlying mechanism behind the observed negative link between individual privacy risks and contact tracing apps' acceptance. Furthermore, we find a substantial intention–behavior gap.
Das Jahreskaddisch ist ein Spezifikum der westaschkenasischen Liturgie. Es wird am Abend und am Morgen des Simchat-Tora-Festes vorgetragen und ist aus den wichtigsten musikalischen Motiven des Kaddisch-Gebetes innerhalb des gesamten jüdischen Jahreszyklus zusammengesetzt. Anhand von Tonaufnahmen wurde das Jahreskaddisch der Frankfurter Tradition transkribiert und seine einzelnen melodischen Bestandteile identifiziert. Die vorgestellte Kaddischmelodie wird im heutigen Gottesdienst in Frankfurt a. M. nicht mehr vorgetragen.
Die Zeitschrift möchte die fruchtbare und facettenreiche Kultur des Judentums sowie seine Berührungspunkte zur Umwelt in den unterschiedlichen Bereichen dokumentieren. Daneben dient die Zeitschrift als Forum zur Positionierung der Fächer Jüdische Studien und Judaistik innerhalb des wissenschaftlichen Diskurses sowie zur Diskussion ihrer historischen und gesellschaftlichen Verantwortung.
Aims. We aim for an understanding of the morphological and spectral properties of the supernova remnant RCW 86 and for insights into the production mechanism leading to the RCW 86 very high-energy gamma-ray emission. Methods. We analyzed High Energy Spectroscopic System (H.E.S.S.) data that had increased sensitivity compared to the observations presented in the RCW 86 H.E.S.S. discovery publication. Studies of the morphological correlation between the 0.5-1 keV X-ray band, the 2-5 keV X-ray band, radio, and gamma-ray emissions have been performed as well as broadband modeling of the spectral energy distribution with two different emission models. Results. We present the first conclusive evidence that the TeV gamma-ray emission region is shell-like based on our morphological studies. The comparison with 2-5 keV X-ray data reveals a correlation with the 0.4-50 TeV gamma-ray emission. The spectrum of RCW 86 is best described by a power law with an exponential cutoff at E-cut = (3.5 +/- 1.2(stat)) TeV and a spectral index of Gamma approximate to 1.6 +/- 0.2. A static leptonic one-zone model adequately describes the measured spectral energy distribution of RCW 86, with the resultant total kinetic energy of the electrons above 1 GeV being equivalent to similar to 0.1% of the initial kinetic energy of a Type Ia supernova explosion (10(51) erg). When using a hadronic model, a magnetic field of B approximate to 100 mu G is needed to represent the measured data. Although this is comparable to formerly published estimates, a standard E-2 spectrum for the proton distribution cannot describe the gamma-ray data. Instead, a spectral index of Gamma(p) approximate to 1.7 would be required, which implies that similar to 7 x 10(49)/n(cm-3) erg has been transferred into high-energy protons with the effective density n(cm-3) = n/1 cm(-3). This is about 10% of the kinetic energy of a typical Type Ia supernova under the assumption of a density of 1 cm(-3).
A deep observation campaign carried out by the High Energy Stereoscopic System (HESS) on Centaurus A enabled the discovery of gamma-rays from the blazar 1ES 1312-423, 2 degrees away from the radio galaxy. With a differential flux at 1 TeV of phi(1 TeV) = (1.9 +/- 0.6(stat) +/- 0.4(sys)) x 10(-13) cm(-2) s(-1) TeV-1 corresponding to 0.5 per cent of the Crab nebula differential flux and a spectral index Gamma = 2.9 +/- 0.5(stat) +/- 0.2(sys), 1ES 1312-423 is one of the faintest sources ever detected in the very high energy (E > 100 GeV) extragalactic sky. A careful analysis using three and a half years of Fermi Large Area Telescope (Fermi-LAT) data allows the discovery at high energies (E > 100 MeV) of a hard spectrum (Gamma = 1.4 +/- 0.4(stat) +/- 0.2(sys)) source coincident with 1ES 1312-423. Radio, optical, UV and X-ray observations complete the spectral energy distribution of this blazar, now covering 16 decades in energy. The emission is successfully fitted with a synchrotron self-Compton model for the non-thermal component, combined with a blackbody spectrum for the optical emission from the host galaxy.
Discovery of high and very high-energy emission from the BL Lacertae object SHBL J001355.9-185406
(2013)
The detection of the high-frequency peaked BL Lac object (HBL) SHBL J001355.9-185406 (z = 0.095) at high (HE; 100 MeV < E < 300 GeV) and very high-energy (VHE; E > 100 GeV) with the Fermi Large Area Telescope (LAT) and the High Energy Stereoscopic System (H.E.S.S.) is reported. Dedicated observations were performed with the H. E. S. S. telescopes, leading to a detection at the 5.5 sigma significance level. The measured flux above 310 GeV is (8.3 +/- 1.7(stat) +/- 1.7(sys)) x 10(-13) photons cm(-2) s(-1) (about 0.6% of that of the Crab Nebula), and the power-law spectrum has a photon index of Gamma = 3.4 +/- 0.5(stat) +/- 0.2(sys). Using 3.5 years of publicly available Fermi-LAT data, a faint counterpart has been detected in the LAT data at the 5.5 sigma significance level, with an integrated flux above 300 MeV of (9.3 +/- 3.4(stat) +/- 0.8(sys)) x 10(-10) photons cm(-2) s(-1) and a photon index of Gamma = 1.96 +/- 0.20(stat) +/- 0.08(sys). X-ray observations with Swift-XRT allow the synchrotron peak energy in vF(v) representation to be located at similar to 1.0 keV. The broadband spectral energy distribution is modelled with a one-zone synchrotron self-Compton (SSC) model and the optical data by a black-body emission describing the thermal emission of the host galaxy. The derived parameters are typical of HBLs detected at VHE, with a particle-dominated jet.
The quasar PKS 1510-089 (z = 0.361) was observed with the H.E.S.S. array of imaging atmospheric Cherenkov telescopes during high states in the optical and GeV bands, to search for very high energy (VHE, defined as E >= 0.1 TeV) emission. VHE gamma-rays were detected with a statistical significance of 9.2 standard deviations in 15.8 h of H. E. S. S. data taken during March and April 2009. A VHE integral flux of I(0.15 TeV < E < 1.0TeV) = (1.0 +/- 0.2(stat) +/- 0.2(sys)) x 10(-11) cm(-2) s(-1) is measured. The best-fit power law to the VHE data has a photon index of G = 5.4 +/- 0.7(stat) +/- 0.3(sys). The GeV and optical light curves show pronounced variability during the period of H.E.S.S. observations. However, there is insufficient evidence to claim statistically significant variability in the VHE data. Because of its relatively high redshift, the VHE flux from PKS 1510-089 should suffer considerable attenuation in the intergalactic space due to the extragalactic background light (EBL). Hence, the measured gamma-ray spectrum is used to derive upper limits on the opacity due to EBL, which are found to be comparable with the previously derived limits from relatively-nearby BL Lac objects. Unlike typical VHE-detected blazars where the broadband spectrum is dominated by nonthermal radiation at all wavelengths, the quasar PKS 1510-089 has a bright thermal component in the optical to UV frequency band. Among all VHE detected blazars, PKS 1510-089 has the most luminous broad line region. The detection of VHE emission from this quasar indicates a low level of gamma - gamma absorption on the internal optical to UV photon field.
Context. Globular clusters (GCs) are established emitters of high-energy (HE, 100 MeV < E < 100 GeV) gamma-ray radiation which could originate from the cumulative emission of the numerous millisecond pulsars (msPSRs) in the clusters’ cores or from inverse Compton (IC) scattering of relativistic leptons accelerated in the GC environment. These stellar clusters could also constitute a new class of sources in the very-high-energy (VHE, E > 100 GeV) gamma-ray regime, judging from the recent detection of a signal from the direction of Terzan 5 with the H.E.S.S. telescope array. Aims. To search for VHE gamma-ray sources associated with other GCs, and to put constraints on leptonic emission models, we systematically analyzed the observations towards 15 GCs taken with the H. E. S. S. array of imaging atmospheric Cherenkov telescopes. Methods. We searched for point-like and extended VHE gamma-ray emission from each GC in our sample and also performed a stacking analysis combining the data from all GCs to investigate the hypothesis of a population of faint emitters. Assuming IC emission as the origin of the VHE gamma-ray signal from the direction of Terzan 5, we calculated the expected gamma-ray flux from each of the 15 GCs, based on their number of millisecond pulsars, their optical brightness and the energy density of background photon fields. Results. We did not detect significant VHE gamma-ray emission from any of the 15 GCs in either of the two analyses. Given the uncertainties related to the parameter determinations, the obtained flux upper limits allow to rule out the simple IC/msPSR scaling model for NGC6388 and NGC7078. The upper limits derived from the stacking analyses are factors between 2 and 50 below the flux predicted by the simple leptonic scaling model, depending on the assumed source extent and the dominant target photon fields. Therefore, Terzan 5 still remains exceptional among all GCs, as the VHE gamma-ray emission either arises from extra-ordinarily efficient leptonic processes, or from a recent catastrophic event, or is even unrelated to the GC itself.
Gamma-ray line signatures can be expected in the very-high-energy (E-gamma > 100 GeV) domain due to self-annihilation or decay of dark matter (DM) particles in space. Such a signal would be readily distinguishable from astrophysical gamma-ray sources that in most cases produce continuous spectra that span over several orders of magnitude in energy. Using data collected with the H. E. S. S. gamma-ray instrument, upper limits on linelike emission are obtained in the energy range between similar to 500 GeV and similar to 25 TeV for the central part of the Milky Way halo and for extragalactic observations, complementing recent limits obtained with the Fermi-LAT instrument at lower energies. No statistically significant signal could be found. For monochromatic gamma-ray line emission, flux limits of (2 x 10(-7)-2 x 10(-5)) m(-2)s(-1)sr(-1) and (1 x 10(-8)- 2 x 10(-6)) m(-2)s(-1)sr(-1) are obtained for the central part of the Milky Way halo and extragalactic observations, respectively. For a DM particle mass of 1 TeV, limits on the velocity- averaged DM annihilation cross section <sigma upsilon >(chi chi ->gamma gamma) reach similar to 10(-27)cm(3)s(-1), based on the Einasto parametrization of the Galactic DM halo density profile. DOI: 10.1103/PhysRevLett.110.041301
HESS observations of the binary system PSR B1259-63/LS 2883 around the 2010/2011 periastron passage
(2013)
Aims. We present very high energy (VHE; E > 100 GeV) data from the gamma-ray binary system PSR B1259-63/LS 2883 taken around its periastron passage on 15th of December 2010 with the High Energy Stereoscopic System (H. E. S. S.) of Cherenkov Telescopes. We aim to search for a possible TeV counterpart of the GeV flare detected by the Fermi LAT. In addition, we aim to study the current periastron passage in the context of previous observations taken at similar orbital phases, testing the repetitive behaviour of the source.
Methods. Observations at VHEs were conducted with H.E.S.S. from 9th to 16th of January 2011. The total dataset amounts to similar to 6 h of observing time. The data taken around the 2004 periastron passage were also re-analysed with the current analysis techniques in order to extend the energy spectrum above 3 TeV to fully compare observation results from 2004 and 2011.
Results. The source is detected in the 2011 data at a significance level of 11.5 sigma revealing an averaged integral flux above 1 TeV of (1.01 +/- 0.18(stat) +/- 0.20(sys)) x 10(-12) cm(-2) s(-1). The differential energy spectrum follows a power-law shape with a spectral index Gamma = 2.92 +/- 0.30(stat) +/- 0.20(sys) and a flux normalisation at 1 TeV of N-0 = (1.95 +/- 0.32(stat) +/- 0.39(sys)) x 10(-12) TeV-1 cm(-2) s(-1). The measured light curve does not show any evidence for variability of the source on the daily scale. The re-analysis of the 2004 data yields results compatible with the published ones. The differential energy spectrum measured up to similar to 10 TeV is consistent with a power law with a spectral index Gamma = 2.81 +/- 0.10(stat) +/- 0.20(sys) and a flux normalisation at 1 TeV of N-0 = (1.29 +/- 0.08(stat) +/- 0.26(sys)) x 10(-12) TeV-1 cm(-2) s(-1).
Conclusions. The measured integral flux and the spectral shape of the 2011 data are compatible with the results obtained around previous periastron passages. The absence of variability in the H.E.S.S. data indicates that the GeV flare observed by Fermi LAT in the time period covered also by H.E.S.S. observations originates in a different physical scenario than the TeV emission. Moreover, the comparison of the new results to the results from the 2004 observations made at a similar orbital phase provides a stronger evidence of the repetitive behaviour of the source.
The 2010 very high energy gamma-ray flare and 10 years ofmulti-wavelength oservations of M 87
(2012)
The giant radio galaxy M 87 with its proximity (16 Mpc), famous jet, and very massive black hole ((3-6) x 10(9) M-circle dot) provides a unique opportunity to investigate the origin of very high energy (VHE; E > 100 GeV) gamma-ray emission generated in relativistic outflows and the surroundings of supermassive black holes. M 87 has been established as a VHE gamma-ray emitter since 2006. The VHE gamma-ray emission displays strong variability on timescales as short as a day. In this paper, results from a joint VHE monitoring campaign on M 87 by the MAGIC and VERITAS instruments in 2010 are reported. During the campaign, a flare at VHE was detected triggering further observations at VHE (H.E.S.S.), X-rays (Chandra), and radio (43 GHz Very Long Baseline Array, VLBA). The excellent sampling of the VHE gamma-ray light curve enables one to derive a precise temporal characterization of the flare: the single, isolated flare is well described by a two-sided exponential function with significantly different flux rise and decay times of tau(rise)(d) = (1.69 +/- 0.30) days and tau(decay)(d) = (0.611 +/- 0.080) days, respectively. While the overall variability pattern of the 2010 flare appears somewhat different from that of previous VHE flares in 2005 and 2008, they share very similar timescales (similar to day), peak fluxes (Phi(>0.35 TeV) similar or equal to (1-3) x 10(-11) photons cm(-2) s(-1)), and VHE spectra. VLBA radio observations of 43 GHz of the inner jet regions indicate no enhanced flux in 2010 in contrast to observations in 2008, where an increase of the radio flux of the innermost core regions coincided with a VHE flare. On the other hand, Chandra X-ray observations taken similar to 3 days after the peak of the VHE gamma-ray emission reveal an enhanced flux from the core (flux increased by factor similar to 2; variability timescale <2 days). The long-term (2001-2010) multi-wavelength (MWL) light curve of M 87, spanning from radio to VHE and including data from Hubble Space Telescope, Liverpool Telescope, Very Large Array, and European VLBI Network, is used to further investigate the origin of the VHE gamma-ray emission. No unique, common MWL signature of the three VHE flares has been identified. In the outer kiloparsec jet region, in particular in HST-1, no enhanced MWL activity was detected in 2008 and 2010, disfavoring it as the origin of the VHE flares during these years. Shortly after two of the three flares (2008 and 2010), the X-ray core was observed to be at a higher flux level than its characteristic range (determined from more than 60 monitoring observations: 2002-2009). In 2005, the strong flux dominance of HST-1 could have suppressed the detection of such a feature. Published models for VHE gamma-ray emission from M 87 are reviewed in the light of the new data.
Discovery of very high energy gamma-ray emission from the BL Lacertae
object PKS0301-243 with HESS
(2013)
The active galactic nucleus PKS 0301-243 (z = 0.266) is a high-synchrotron-peaked BL Lac object that is detected at high energies (HE, 100 MeV < E < 100 GeV) by Fermi/LAT. This paper reports on the discovery of PKS 0301-243 at very high energies (E > 100 GeV) by the High Energy Stereoscopic System (H.E.S.S.) from observations between September 2009 and December 2011 for a total live time of 34.9 h. Gamma rays above 200 GeV are detected at a significance of 9.4 sigma. A hint of variability at the 2.5 sigma level is found. An integral flux I(E > 200GeV) = (3.3 +/- 1.1(stat) +/- 0.7(syst)) x 10(-12) ph cm(-2) s(-1) and a photon index Gamma = 4.6 +/- 0.7(stat) +/- 0.2(syst) are measured. Multi-wavelength light curves in HE, X-ray and optical bands show strong variability, and a minimal variability timescale of eight days is estimated from the optical light curve. A single-zone leptonic synchrotron self-Compton scenario satisfactorily reproduces the multi-wavelength data. In this model, the emitting region is out of equipartition and the jet is particle dominated. Because of its high redshift compared to other sources observed at TeV energies, the very high energy emission from PKS 0301-243 is attenuated by the extragalactic background light (EBL) and the measured spectrum is used to derive an upper limit on the opacity of the EBL.
Axionlike particles (ALPs) are hypothetical light (sub-eV) bosons predicted in some extensions of the Standard Model of particle physics. In astrophysical environments comprising high-energy gamma rays and turbulent magnetic fields, the existence of ALPs can modify the energy spectrum of the gamma rays for a sufficiently large coupling between ALPs and photons. This modification would take the form of an irregular behavior of the energy spectrum in a limited energy range. Data from the H. E. S. S. observations of the distant BL Lac object PKS 2155 - 304 (z = 0.116) are used to derive upper limits at the 95% C. L. on the strength of the ALP coupling to photons, g(gamma a) < 2.1 x 10(-11) GeV-1 for an ALP mass between 15 and 60 neV. The results depend on assumptions on the magnetic field around the source, which are chosen conservatively. The derived constraints apply to both light pseudoscalar and scalar bosons that couple to the electromagnetic field.
Very high-energy gamma-ray emission from PKS 0447-439 was detected with the H. E. S. S. Cherenkov telescope array in December 2009. This blazar is one of the brightest extragalactic objects in the Fermi bright source list and has a hard spectrum in the MeV to GeV range. In the TeV range, a photon index of 3.89 +/- 0.37 (stat) +/- 0.22 (sys) and a flux normalisation at 1 TeV, phi(1) (TeV) = (3.5 +/- 1.1(stat) +/- 0.9(sys)) x 10(-13) cm(-2) s(-1) TeV-1 were found. The detection with H. E. S. S. triggered observations in the X-ray band with the Swift and RXTE telescopes. Simultaneous UV and optical data from Swift UVOT and data from the optical telescopes ATOM and ROTSE are also available. The spectrum and light curve measured with H. E. S. S. are presented and compared to the multi-wavelength data at lower energies. A rapid flare is seen in the Swift XRT and RXTE data, together with a flux variation in the UV band, at a time scale of the order of one day. A firm upper limit of z < 0.59 on the redshift of PKS 0447-439 is derived from the combined Fermi-LAT and H. E. S. S. data, given the assumptions that there is no upturn in the intrinsic spectrum above the Fermi-LAT energy range and that absorption on the extragalactic background light (EBL) is not weaker than the lower limit provided by current models. The spectral energy distribution is well described by a simple one-zone synchrotron self-Compton scenario, if the redshift of the source is less than z less than or similar to 0.4.
The gamma-ray spectrum of the low-frequency-peaked BL Lac (LBL) object AP Librae is studied, following the discovery of very-high-energy (VHE; E > 100 GeV) gamma-ray emission up to the TeV range by the H.E.S.S. experiment. Thismakes AP Librae one of the few VHE emitters of the LBL type. The measured spectrum yields a flux of (8.8 +/- 1.5(stat) +/- 1.8(sys)) x 10(-12) cm(-2) s(-1) above 130 GeV and a spectral index of Gamma = 2.65 +/- 0.19(stat) +/- 0.20(sys). This study also makes use of Fermi-LAT observations in the high energy (HE, E > 100 MeV) range, providing the longest continuous light curve (5 years) ever published on this source. The source underwent a flaring event between MJD 56 306-56 376 in the HE range, with a flux increase of a factor of 3.5 in the 14 day bin light curve and no significant variation in spectral shape with respect to the low-flux state. While the H.E.S.S. and (low state) Fermi-LAT fluxes are in good agreement where they overlap, a spectral curvature between the steep VHE spectrum and the Fermi-LAT spectrum is observed. The maximum of the gamma-ray emission in the spectral energy distribution is located below the GeV energy range.
Aims. Previous observations with the High Energy Stereoscopic System (H.E.S.S.) have revealed an extended very-high-energy (VHE; E > 100 GeV) gamma-ray source, HESS J1834-087, coincident with the supernova remnant (SNR) W41. The origin of the gamma-ray emission was investigated in more detail with the H.E.S.S. array and the Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope.
Methods. The gamma-ray data provided by 61 h of observations with H.E.S.S., and four years with the Fermi LAT were analyzed, covering over five decades in energy from 1.8 GeV up to 30 TeV. The morphology and spectrum of the TeV and GeV sources were studied and multiwavelength data were used to investigate the origin of the gamma-ray emission toward W41.
Results. The TeV source can be modeled with a sum of two components: one point-like and one significantly extended (sigma(TeV) = 0.17 degrees +/- 0.01 degrees), both centered on SNR W41 and exhibiting spectra described by a power law with index Gamma(TeV) similar or equal to 2.6. The GeV source detected with Fermi LAT is extended (sigma(GeV) = 0.15 degrees +/- 0.03 degrees) and morphologically matches the VHE emission. Its spectrum can be described by a power-law model with an index Gamma(GeV) = 2.15 +/- 0.12 and smoothly joins the spectrum of the whole TeV source. A break appears in the gamma-ray spectra around 100 GeV. No pulsations were found in the GeV range.
Conclusions. Two main scenarios are proposed to explain the observed emission: a pulsar wind nebula (PWN) or the interaction of SNR W41 with an associated molecular cloud. X-ray observations suggest the presence of a point-like source (a pulsar candidate) near the center of the remnant and nonthermal X-ray diffuse emission that could arise from the possibly associated PWN. The PWN scenario is supported by the compatible positions of the TeV and GeV sources with the putative pulsar. However, the spectral energy distribution from radio to gamma-rays is reproduced by a one-zone leptonic model only if an excess of low-energy electrons is injected following a Maxwellian distribution by a pulsar with a high spin-down power (> 10(37) erg s(-1)). This additional low-energy component is not needed if we consider that the point-like TeV source is unrelated to the extended GeV and TeV sources. The interacting SNR scenario is supported by the spatial coincidence between the gamma-ray sources, the detection of OH (1720 MHz) maser lines, and the hadronic modeling.
Context. Very-high-energy (VHE; E > 100 GeV) gamma-ray emission from blazars inevitably gives rise to electron-positron pair production through the interaction of these gamma-rays with the extragalactic background light (EBL). Depending on the magnetic fields in the proximity of the source, the cascade initiated from pair production can result in either an isotropic halo around an initially- beamed source or a magnetically- broadened cascade :aux.
Aims. Both extended pair-halo (PH) and magnetically broadened cascade (MBC) emission from regions surrounding the blazars 1ES 1101-232, IRS 0229+200, and PKS 2155-304 were searched for using VHE y-ray data taken with the High Energy Stereoscopic System (HESS.) and high-energy (HE; 100 MeV < E < 100 GeV) gamma-ray data with the Fermi Large Area Telescope (LAT).
Methods. By comparing the angular distributions of the reconstructed gamma-ray events to the angular profiles calculated from detailed theoretical models, the presence of PH and MBC was investigated.
Results. Upper limits on the extended emission around lES 1101-232, lES 0229+200, and PKS 2155-304 are found to be at a level of a few per cent of the Crab nebula flux above 1 TeV, depending on the assumed photon index of the cascade emission. Assuming strong extra-Galactic magnetic field (EGME) values, >10(-12) G, this limits the production of pair haloes developing from electromagnetic cascades. For weaker magnetic fields, in which electromagnetic cascades would result in MBCs. EGMF strengths in the range (0.3-3) x 10(-15) G were excluded for PKS 2155-304 at the 99% confidence level, under the assumption of a 1 Mpc coherence length.
Composite supernova remnants (SNRs) constitute a small subclass of the remnants of massive stellar explosions where non-thermal radiation is observed from both the expanding shell-like shock front and from a pulsar wind nebula (PWN) located inside of the SNR. These systems represent a unique evolutionary phase of SNRs where observations in the radio, X-ray, and gamma-ray regimes allow the study of the co-evolution of both these energetic phenomena. In this article, we report results from observations of the shell-type SNR G15.4+0.1 performed with the High Energy Stereoscopic System (H. E. S. S.) and XMM-Newton. A compact TeV gamma-ray source, HESS J1818-154, located in the center and contained within the shell of G15.4+0.1 is detected by H. E. S. S. and featurs a spectrum best represented by a power-law model with a spectral index of -2.3 +/- 0.3(stat) +/- 0.2(sys) and an integral flux of F(>0.42 TeV) = (0.9 +/- 0.3(stat) +/- 0.2(sys)) x 10(-12) cm(-2) s(-1). Furthermore, a recent observation with XMM-Newton reveals extended X-ray emission strongly peaked in the center of G15.4+0.1. The X-ray source shows indications of an energy-dependent morphology featuring a compact core at energies above 4 keV and more extended emission that fills the entire region within the SNR at lower energies. Together, the X-ray and VHE gamma-ray emission provide strong evidence of a PWN located inside the shell of G15.4+0.1 and this SNR can therefore be classified as a composite based on these observations. The radio, X-ray, and gamma-ray emission from the PWN is compatible with a one-zone leptonic model that requires a low average magnetic field inside the emission region. An unambiguous counterpart to the putative pulsar, which is thought to power the PWN, has been detected neither in radio nor in X-ray observations of G15.4+0.1.
HESS J1640-465 - an exceptionally luminous TeV gamma-ray supernova remnant (vol 439, pg 2828, 2014)
(2014)
TeV gamma-ray observations of the young synchrotron-dominated SNRs G1.9+0.3 and G330.2+1.0 with HESS
(2014)
The non-thermal nature of the X-ray emission from the shell-type supernova remnants (SNRs) G1.9+0.3 and G330.2+1.0 is an indication of intense particle acceleration in the shock fronts of both objects. This suggests that the SNRs are prime candidates for very-high-energy (VHE; E > 0.1 TeV) gamma-ray observations. G1.9+0.3, recently established as the youngest known SNR in the Galaxy, also offers a unique opportunity to study the earliest stages of SNR evolution in the VHE domain. The purpose of this work is to probe the level of VHE gamma-ray emission from both SNRs and use this to constrain their physical properties. Observations were conducted with the H. E. S. S. (High Energy Stereoscopic System) Cherenkov Telescope Array over a more than six-year period spanning 2004-2010. The obtained data have effective livetimes of 67 h for G1.9+0.3 and 16 h for G330.2+1.0. The data are analysed in the context of the multiwavelength observations currently available and in the framework of both leptonic and hadronic particle acceleration scenarios. No significant gamma-ray signal from G1.9+0.3 or G330.2+1.0 was detected. Upper limits (99 per cent confidence level) to the TeV flux from G1.9+0.3 and G330.2+1.0 for the assumed spectral index Gamma = 2.5 were set at 5.6 x 10(-1)3 cm(-2) s(-1) above 0.26 TeV and 3.2 x 10(-12) cm(-2) s(-1) above 0.38 TeV, respectively. In a one-zone leptonic scenario, these upper limits imply lower limits on the interior magnetic field to B-G1.9 greater than or similar to 12 mu G for G1.9+0.3 and to B-G330 greater than or similar to 8 mu G for G330.2+1.0. In a hadronic scenario, the low ambient densities and the large distances to the SNRs result in very low predicted fluxes, for which the H.E.S.S. upper limits are not constraining.
Context. About 40% of the observation time of the High Energy Stereoscopic System (H.E.S.S.) is dedicated to studying active galactic nuclei (AGN), with the aim of increasing the sample of known extragalactic very-high-energy (VHE, E > 100 GeV) sources and constraining the physical processes at play in potential emitters.
Aims. H.E.S.S. observations of AGN, spanning a period from April 2004 to December 2011, are investigated to constrain their gamma-ray fluxes. Only the 47 sources without significant excess detected at the position of the targets are presented.
Methods. Upper limits on VHE fluxes of the targets were computed and a search for variability was performed on the nightly time scale.
Results. For 41 objects, the flux upper limits we derived are the most constraining reported to date. These constraints at VHE are compared with the flux level expected from extrapolations of Fermi-LAT measurements in the two-year catalog of AGN. The H.E.S.S. upper limits are at least a factor of two lower than the extrapolated Fermi-LAT fluxes for 11 objects Taking into account the attenuation by the extragalactic background light reduces the tension for all but two of them, suggesting intrinsic curvature in the high-energy spectra of these two AGN.
Conclusions. Compilation efforts led by current VHE instruments are of critical importance for target-selection strategies before the advent of the Cherenkov Telescope Array (CTA).
The results of follow-up observations of the TeV gamma-ray source HESS J1640-465 from 2004 to 2011 with the High Energy Stereoscopic System (HESS) are reported in this work. The spectrum is well described by an exponential cut-off power law with photon index Gamma = 2.11 +/- 0.09(stat) +/- 0.10(sys), and a cut-off energy of E-2 = 6.0(-1.2)(+2.0) TeV. The TeV emission is significantly extended and overlaps with the northwestern part of the shell of the SNR G338.3-0.0. The new HESS results, a re-analysis of archival XMM-Newton data and multiwavelength observations suggest that a significant part of the gamma-ray emission from HESS J1640-465 originates in the supernova remnant shell. In a hadronic scenario, as suggested by the smooth connection of the GeV and TeV spectra, the product of total proton energy and mean target density could be as high as W(p)n(H) similar to 4 x 10(52)(d/10kpc)(2) erg cm(-3).
Search for TeV Gamma-ray emission from GRB 100621A, an extremely bright GRB in X-rays, with HESS
(2014)
The long gamma-ray burst (GRB) 100621A, at the time the brightest X-ray transient ever detected by Swift-XRT in the 0.3-10 keV range, has been observed with the H.E.S.S. imaging air Cherenkov telescope array, sensitive to gamma radiation in the very-high-energy (VHE, >100 GeV) regime. Due to its relatively small redshift of z similar to 0.5, the favourable position in the southern sky and the relatively short follow-up time (<700 s after the satellite trigger) of the H.E.S.S. observations, this GRB could be within the sensitivity reach of the HESS. instrument. The analysis of the HESS. data shows no indication of emission and yields an integral flux upper limit above similar to 380 GeV of 4.2 x 10(-12) cm(-2) s(-1) s (95% confidence level), assuming a simple Band function extension model. A comparison to a spectral-temporal model, normalised to the prompt flux at sub-MeV energies, constraints the existence of a temporally extended and strong additional hard power law, as has been observed in the other bright X-ray GRB 130427A. A comparison between the HESS. upper limit and the contemporaneous energy output in X-rays constrains the ratio between the X-ray and VHE gamma-ray fluxes to be greater than 0.4. This value is an important quantity for modelling the afterglow and can constrain leptonic emission scenarios, where leptons are responsible for the X-ray emission and might produce VHE gamma rays.
The Large Magellanic Cloud, a satellite galaxy of the Milky Way, has been observed with the High Energy Stereoscopic System (H.E.S.S.) above an energy of 100 billion electron volts for a deep exposure of 210 hours. Three sources of different types were detected: the pulsar wind nebula of the most energetic pulsar known, N 157B; the radio-loud supernova remnant N 132D; and the largest nonthermal x-ray shell, the superbubble 30 Dor C. The unique object SN 1987A is, unexpectedly, not detected, which constrains the theoretical framework of particle acceleration in very young supernova remnants. These detections reveal the most energetic tip of a g-ray source population in an external galaxy and provide via 30 Dor C the unambiguous detection of g-ray emission from a superbubble.
Very high energy (VHE, E > 100 GeV)gamma-ray flaring activity of the high-frequency peaked BL Lac object PG 1553 + 113 has been detected by the H.E.S.S. telescopes. The flux of the source increased by a factor of 3 during the nights of 2012 April 26 and 27 with respect to the archival measurements with a hint of intra-night variability. No counterpart of this event has been detected in the Fermi-Large Area Telescope data. This pattern is consistent with VHE gamma(-)ray flaring being caused by the injection of ultrarelativistic particles, emitting.-rays at the highest energies. The dataset offers a unique opportunity to constrain the redshift of this source at z = 0.49 +/- 0.04 using a novel method based on Bayesian statistics. The indication of intra-night variability is used to introduce a novel method to probe for a possible Lorentz invariance violation (LIV), and to set limits on the energy scale at which Quantum Gravity (QG) effects causing LIV may arise. For the subluminal case, the derived limits are E-QG,E- 1 > 4.10 x 10(17) GeV and E-QG,E- 2 > 2.10 x 10(10) GeV for linear and quadratic LIV effects, respectively.
Search for dark matter annihilation signatures in HESS observations of
dwarf spheroidal galaxies
(2014)
Dwarf spheroidal galaxies of the Local Group are close satellites of the Milky Way characterized by a large mass-to-light ratio and are not expected to be the site of nonthermal high-energy gamma-ray emission or intense star formation. Therefore they are among the most promising candidates for indirect dark matter searches. During the last years the High Energy Stereoscopic System (H.E.S.S.) of imaging atmospheric Cherenkov telescopes observed five of these dwarf galaxies for more than 140 hours in total, searching for TeV gamma-ray emission from annihilation of dark matter particles. The new results of the deep exposure of the Sagittarius dwarf spheroidal galaxy, the first observations of the Coma Berenices and Fornax dwarves and the reanalysis of two more dwarf spheroidal galaxies already published by the H.E.S.S. Collaboration, Carina and Sculptor, are presented. In the absence of a significant signal new constraints on the annihilation cross section applicable to weakly interacting massive particles (WIMPs) are derived by combining the observations of the five dwarf galaxies. The combined exclusion limit depends on the WIMP mass and the best constraint is reached at 1-2 TeV masses with a cross-section upper bound of similar to 3.9 x 10(-24) cm(3) s(-1) at a 95% confidence level.
Diffuse gamma-ray emission is the most prominent observable signature of celestial cosmic-ray interactions at high energies. While already being investigated at GeVenergies over several decades, assessments of diffuse gamma-ray emission at TeVenergies remain sparse. After completion of the systematic survey of the inner Galaxy, the H.E.S.S. experiment is in a prime position to observe large-scale diffuse emission at TeVenergies. Data of the H.E.S.S. Galactic Plane Survey are investigated in regions off known gamma-ray sources. Corresponding gamma-ray flux measurements were made over an extensive grid of celestial locations. Longitudinal and latitudinal profiles of the observed gamma-ray fluxes show characteristic excess emission not attributable to known gamma-ray sources. For the first time large-scale gamma-ray emission along the Galactic plane using imaging atmospheric Cherenkov telescopes has been observed. While the background subtraction technique limits the ability to recover modest variation on the scale of the H.E.S.S. field of view or larger, which is characteristic of the inverse Compton scatter-induced Galactic diffuse emission, contributions of neutral pion decay as well as emission from unresolved gamma-ray sources can be recovered in the observed signal to a large fraction. Calculations show that the minimum gamma-ray emission from pi(0) decay represents a significant contribution to the total signal. This detection is interpreted as a mix of diffuse Galactic gamma-ray emission and unresolved sources.
An annihilation signal of dark matter is searched for from the central region of the Milky Way. Data acquired in dedicated on-off observations of the Galactic center region with H.E.S.S. are analyzed for this purpose. No significant signal is found in a total of similar to 9 h of on-off observations. Upper limits on the velocity averaged cross section, <sigma upsilon >, for the annihilation of dark matter particles with masses in the range of similar to 300 GeV to similar to 10 TeV are derived. In contrast to previous constraints derived from observations of the Galactic center region, the constraints that are derived here apply also under the assumption of a central core of constant dark matter density around the center of the Galaxy. Values of <sigma upsilon > that are larger than 3 x 10(-24) cm(3)/s are excluded for dark matter particles with masses between similar to 1 and similar to 4 TeV at 95% C.L. if the radius of the central dark matter density core does not exceed 500 pc. This is the strongest constraint that is derived on <sigma upsilon > for annihilating TeV mass dark matter without the assumption of a centrally cusped dark matter density distribution in the search region.
Context. Puppis A is an interesting similar to 4 kyr-old supernova remnant (SNR) that shows strong evidence of interaction between the forward shock and a molecular cloud. It has been studied in detail from radio frequencies to high-energy (HE, 0.1-100 GeV) gamma-rays. An analysis of the Fermi-LAT data has shown extended HE gamma-ray emission with a 0.2-100 GeV spectrum exhibiting no significant deviation from a power law, unlike most of the GeV-emitting SNRs known to be interacting with molecular clouds. This makes it a promising target for imaging atmospheric Cherenkov telescopes (IACTs) to probe the gamma-ray emission above 100 GeV.
Aims. Very-high-energy (VHE, E >= 0.1 TeV) gamma-ray emission from Puppis A has been, for the first time, searched for with the High Energy Stereoscopic System (HESS.).
Methods. Stereoscopic imaging of Cherenkov radiation from extensive air showers is used to reconstruct the direction and energy of the incident gamma-rays in order to produce sky images and source spectra. The profile likelihood method is applied to find constraints on the existence of a potential break or cutoff in the photon spectrum.
Results. The analysis of the HESS. data does not reveal any significant emission towards Puppis A. The derived upper limits on the differential photon flux imply that its broadband gamma-ray spectrum must exhibit a spectral break or cutoff. By combining Fermi-LAT and HESS. measurements, the 99% confidence-level upper limits on such a cutoff are found to be 450 and 280 GeV, assuming a power law with a simple exponential and a sub-exponential cutoff, respectively. It is concluded that none of the standard limitations (age, size, radiative losses) on the particle acceleration mechanism, assumed to be continuing at present, can explain the lack of VHE signal. The scenario in which particle acceleration has ceased some time ago is considered as an alternative explanation. The HE/VHE spectrum of Puppis A could then exhibit a break of non-radiative origin (as observed in several other interacting SNRs, albeit at somewhat higher energies), owing to the interaction with dense and neutral material, in particular towards the NE region.
G349.7+0.2 is a young Galactic supernova remnant (SNR) located at the distance of 11.5 kpc and observed across the entire electromagnetic spectrum from radio to high energy (HE; 0.1 GeV < E < 100 GeV) gamma-rays. Radio and infrared observations indicate that the remnant is interacting with a molecular cloud. In this paper, the detection of very high energy (VHE, E > 100 GeV) gamma-ray emission coincident with this SNR with the High Energy Stereoscopic System (HESS.) is reported. This makes it one of the farthest Galactic SNR ever detected in this domain. An integral flux F(E > 400 GeV) = (6.5 +/- 1.1(stat) +/- 1.3(syst)) x 10-11 ph cm(-2) s(-1) corresponding to similar to 0.7% of that of the Crab Nebula and to a luminosity of similar to 10(34) erg s(-1) above the same energy threshold, and a steep photon index Gamma(VHE) = 2.8 +/- 0.27(stat) +/- 0.20(syst) are measured. The analysis of more than 5 yr of Fermi-LAT data towards this source shows a power-law like spectrum with a best-fit photon index Gamma(HE) = 2.2 +/- 0.04.2(stat-0.31sys)(+0.13), The combined gamma-ray spectrum of 0349.7+0.2 can be described by either a broken power law (I3PL) or a power law with exponential (or sub exponential) cutoff (PLC). In the former case, the photon break energy is found at E-br,E-gamma = 551(-30)(+70) GeV, slightly higher than what is usually observed in the HE/VHE gamma-ray emitting middle-aged SNRs known to be interacting with molecular clouds. In the latter case. the exponential (respectively sub-exponential) cutoff energy is measured at E-cat,E-gamma = 1.4(-0.55)(+1.6) (respectively 0.35(-0.21)(+0.75)) TeV. A pion decay process resulting from the interaction of the accelerated protons and nuclei with the dense surrounding medium is clearly the preferred scenario to explain the gamma-ray emission. The BPL with a spectral steepening of 0.5-1 and the PLC provide equally good fits to the data. The product or the average gas density and the total energy content of accelerated protons and nuclei amounts to nu W-p similar to 5 x 10(51) erg cm(-3)
In this paper we report on the analysis of all the available optical and very high-energy gamma-ray (> 200 GeV) data for the BL Lac object PKS 2155-304, collected simultaneously with the ATOM and H.E.S.S. telescopes from 2007 until 2009. This study also includes X-ray (RXTE, Swift) and high-energy gamma-ray (Fermi-LAT) data. During the period analysed, the source was transitioning from its flaring to quiescent optical states, and was characterized by only moderate flux changes at different wavelengths on the timescales of days and months. A flattening of the optical continuum with an increasing optical flux can be noted in the collected dataset, but only occasionally and only at higher flux levels. We did not find any universal relation between the very high-energy gamma-ray and optical flux changes on the timescales from days and weeks up to several years. On the other hand, we noted that at higher flux levels the source can follow two distinct tracks in the optical flux-colour diagrams, which seem to be related to distinct gamma-ray states of the blazar. The obtained results therefore indicate a complex scaling between the optical and gamma-ray emission of PKS 2155 304, with different correlation patterns holding at different epochs, and a gamma-ray flux depending on the combination of an optical flux and colour rather than a flux alone.
Galactic cosmic rays reach energies of at least a few petaelectronvolts (of the order of 1015 electronvolts). This implies that our Galaxy contains petaelectronvolt accelerators (‘PeVatrons’), but all proposed models of Galactic cosmic-ray accelerators encounter difficulties at exactly these energies. Dozens of Galactic accelerators capable of accelerating particles to energies of tens of teraelectronvolts (of the order of 1013 electronvolts) were inferred from recent γ-ray observations3. However, none of the currently known accelerators—not even the handful of shell-type supernova remnants commonly believed to supply most Galactic cosmic rays—has shown the characteristic tracers of petaelectronvolt particles, namely, power-law spectra of γ-rays extending without a cut-off or a spectral break to tens of teraelectronvolts4. Here we report deep γ-ray observations with arcminute angular resolution of the region surrounding the Galactic Centre, which show the expected tracer of the presence of petaelectronvolt protons within the central 10 parsecs of the Galaxy. We propose that the supermassive black hole Sagittarius A* is linked to this PeVatron. Sagittarius A* went through active phases in the past, as demonstrated by X-ray outbursts5and an outflow from the Galactic Centre6. Although its current rate of particle acceleration is not sufficient to provide a substantial contribution to Galactic cosmic rays, Sagittarius A* could have plausibly been more active over the last 106–107 years, and therefore should be considered as a viable alternative to supernova remnants as a source of petaelectronvolt Galactic cosmic rays.
Re-observations with the HESS telescope array of the very high-energy (VHE) source HESS J1018-589A that is coincident with the Fermi-LAT gamma-ray binary 1FGL J1018.6-5856 have resulted in a source detection significance of more than 9 sigma and the detection of variability (chi(2)/nu of 238.3/155) in the emitted gamma-ray flux. This variability confirms the association of HESS J1018-589A with the high-energy gamma-ray binary detected Fermi-LAT and also confirms the point-like source as a new VHE binary system. The spectrum of HESS J1018-589A is best fit with a power-law function with photon index Gamma = 2.20 +/- 0.14(stat) +/- 0.2(sys). Emission is detected up to similar to 20 TeV. The mean differential flux level is (2.9 +/- 0.4) x 10(-13) TeV-1 cm(-2) s(-1) at 1 TeV, equivalent to similar to 1% of the flux from the Crab Nebula at the same energy. Variability is clearly detected the night-by-night light curve. When folded on the orbital period of 16.58 days, the rebinned light curve peaks in phase with the observed X-ray high-energy phaseograms. The fit of the HESS phaseogram to a constant flux provides evidence of periodicity at the level of N-sigma > 3 sigma. The of the VHE phaseogram and measured spectrum suggest a low-inclination, low-eccentricity system with a modest impact from VHE gamma-ray due to pair production (tau less than or similar to 1 at 300 GeV).
This Letter reports the discovery of a remarkably hard spectrum source, HESS J1641-463, by the High Energy Stereoscopic System (H.E.S.S.) in the very high energy (VHE) domain. HESS J1641-463 remained unnoticed by the usual analysis techniques due to confusion with the bright nearby source HESS J1640-465. It emerged at a significance level of 8.5 standard deviations after restricting the analysis to events with energies above 4 TeV. It shows a moderate flux level of phi(E > 1TeV) = (3.64 +/- 0.44(stat)+/- 0.73(sys)) x 10(-13) cm(-2) s(-1), corresponding to 1.8% of the Crab Nebula flux above the same energy, and a hard spectrum with a photon index of Gamma = 2.07 +/- 0.11(stat)+/- 0.20(sys). It is a point-like source, although an extension up to a Gaussian width of sigma = 3 arcmin cannot be discounted due to uncertainties in the H.E.S.S. point-spread function. The VHE gamma-ray flux of HESS J1641-463 is found to be constant over the observed period when checking time binnings from the year-by-year to the 28 minute exposure timescales. HESS J1641-463 is positionally coincident with the radio supernova remnant SNR G338.5+0.1. No X-ray candidate stands out as a clear association; however, Chandra and XMM-Newton data reveal some potential weak counterparts. Various VHE gamma-ray production scenarios are discussed. If the emission from HESS J1641-463 is produced by cosmic ray protons colliding with the ambient gas, then their spectrum must extend close to 1 PeV. This object may represent a source population contributing significantly to the galactic cosmic ray flux around the knee.
Vertragsgestaltung ist ein praktisch sehr relevantes Thema, das wegen der Justizorientierung in der Wissenschaft noch weitgehend stiefmütterlich behandelt wird. In dieser Untersuchung wird, zumindest für die besonders delikate Konstellation bei komplexen Kooperationen des Staats mit Privaten (ÖPP/PPP), Abhilfe geschaffen. Dabei gründet die Analyse auf einer fundierten Typisierung und Charakterisierung der Probleme solcher Projekte. Den theoretischen Rahmen liefert eine effizienzorientierte Studie institutionenökonomischer Ansätze, namentlich der Transaktionskostentheorie und der Prinzipal-Agenten-Theorie, rückversichert über die praxisorientierten Grundregeln der vertraglichen Risikoverteilung. So gelingt es praktische Formulierungsvorschläge für Standardprobleme der Vertragsgestaltung, wie Leistungsbestimmungen, Anpassungsmechanismen, Konfliktbeilegungsregeln, Informationsmechanismen und Kündigungsregeln zu finden. Diese werden auch aus den Erfolgsbedingungen erläutert.
Verwaltungsmodernisierung
(2020)
Die Modernisierung der öffentlichen Verwaltung hat sich längst zu einer Daueraufgabe entwickelt. In den Modernisierungsprozessen stehen derzeit zwei Segmente besonders im Fokus: Digitalisierung und Partizipation. Digitalisierung geht heute weit über die ursprünglich mit diesem Stichwort angesprochene Umwandlung analoger Daten in elektronische Datenformate hinaus. Die Programmatik der Digitalisierung zielt auf den möglichst umfassenden Einsatz elektronischer Informations- und Kommunikationstechniken zur Unterstützung, Beschleunigung, Rationalisierung und in Teilen auch Ersetzung von herkömmlichen Verwaltungsabläufen mit der Perspektive auf eine Transformation und Durchdringung sowohl des gesamten Verwaltungshandelns als auch der gesamten Verwaltungsorganisation. Demgegenüber meint Partizipation nach gängigem Verständnis die Beteiligung von Bürgern und anderen gesellschaftlichen Akteuren an politischen Willensbildungs- und Entscheidungsprozessen. In spezifisch administrativem Zusammenhang geht es vor allem um die Einbindung von Bürgern in Entscheidungsprozesse der Verwaltung und um die Aktivierung der Zivilgesellschaft, die Erschließung bürgerschaftlichen Engagements sowie gesellschaftlicher Ressourcen für die Erfüllung von Verwaltungsaufgaben – und dies alles mit dem Ziel einer Verbesserung der Legitimität und Qualität öffentlicher Verwaltung. Die beiden Modernisierungsansätze stehen nicht unverbunden nebeneinander. Vielmehr gehen sie nicht selten ineinander über. Beispiele dafür sind die Bereitstellung von Optionen zu elektronischer Stellung und Bearbeitung von Anträgen sowie von elektronischen Plattformen für die Bürgerpartizipation.
An diesen Themenfeldern der Verwaltungsmodernisierung setzt der Tagungsband an. Er dokumentiert den Gedankenaustausch über Digitalisierungs- und Partizipationsprozesse zwischen polnischen und deutschen Verwaltungsrechtswissenschaftlern auf einer Tagung, die im Dezember 2019 an der Universität Potsdam stattgefunden hat.
Answer Set Programming (ASP) is a powerful declarative programming paradigm that has been successfully applied to many different domains. Recently, ASP has also proved successful for hard optimization problems like course timetabling and travel allotment. In this paper, we approach another important task, namely, the shift design problem, aiming at an alignment of a minimum number of shifts in order to meet required numbers of employees (which typically vary for different time periods) in such a way that over- and understaffing is minimized. We provide an ASP encoding of the shift design problem, which, to the best of our knowledge, has not been addressed by ASP yet. Our experimental results demonstrate that ASP is capable of improving the best known solutions to some benchmark problems. Other instances remain challenging and make the shift design problem an interesting benchmark for ASP-based optimization methods.
Digital inclusion
(2021)
In this thesis, we tackle two social disruptions: recent refugee waves in Germany and the COVID-19 pandemic. We focus on the use of information and communication technology (ICT) as a key means of alleviating these disruptions and promoting social inclusion. As social disruptions typically lead to frustration and fragmentation, it is essential to ensure the social inclusion of individuals and societies during such times.
In the context of the social inclusion of refugees, we focus on the Syrian refugees who arrived in Germany as of 2015, as they form a large and coherent refugee community. In particular, we address the role of ICTs in refugees’ social inclusion and investigate how different ICTs (especially smartphones and social networks) can foster refugees’ integration and social inclusion. In the context of the COVID-19 pandemic, we focus on the widespread unconventional working model of work from home (WFH). Our research here centers on the main constructs of WFH and the key differences in WFH experiences based on personal characteristics such as gender and parental status.
We reveal novel insights through four well-established research methods: literature review, mixed methods, qualitative method, and quantitative method. The results of our research have been published in the form of eight articles in major information systems venues and journals. Key results from the refugee research stream include the following: Smartphones represent a central component of refugee ICT use; refugees view ICT as a source of information and power; the social connectedness of refugees is strongly correlated with their Internet use; refugees are not relying solely on traditional methods to learn the German language or pursue further education; the ability to use smartphones anytime and anywhere gives refugees an empowering feeling of global connectedness; and ICTs empower refugees on three levels (community participation, sense of control, and self-efficacy).
Key insights from the COVID-19 WFH stream include: Gender and the presence of children under the age of 18 affect workers’ control over their time, technology usefulness, and WFH conflicts, while not affecting their WFH attitudes; and both personal and technology-related factors affect an individual’s attitude toward WFH and their productivity. Further insights are being gathered at the time of submitting this thesis.
This thesis contributes to the discussion within the information systems community regarding how to use different ICT solutions to promote the social inclusion of refugees in their new communities and foster an inclusive society. It also adds to the growing body of research on COVID-19, in particular on the sudden workplace transformation to WFH. The insights gathered in this thesis reveal theoretical implications and future opportunities for research in the field of information systems, practical implications for relevant stakeholders, and social implications related to the refugee crisis and the COVID-19 pandemic that must be addressed.
Immigrant integration has become a primary political concern for leaders in Germany and the United States. The information systems (IS) community has begun to research how information and communications technologies can assist immigrants and refugees, such as by examining how countries can facilitate social-inclusion processes. Migrants face the challenge of joining closed communities that cannot integrate or fear doing so. We conducted a panel discussion at the 2019 Americas Conference on Information Systems (AMCIS) in Cancun, Mexico, to introduce multiple viewpoints on immigration. In particular, the panel discussed how technology can both support and prevent immigrants from succeeding in their quest. We conducted the panel to stimulate a thoughtful and dynamic discussion on best practices and recommendations to enhance the discipline's impact on alleviating the challenges that occur for immigrants in their host countries. In this panel report, we introduce the topic of using ICT to help immigrants integrate and identify differences between North/Central America and Europe. We also discuss how immigrants (particularly refugees) use ICT to connect with others, feel that they belong, and maintain their identity. We also uncover the dark and bright sides of how governments use ICT to deter illegal immigration. Finally, we present recommendations for researchers and practitioners on how to best use ICT to assist with immigration.
The coronavirus disease of 2019 (COVID-19) pandemic has forced most academics to work from home. This sudden venue change can affect academics' productivity and exacerbate the challenges that confront universities as they face an uncertain future. In this paper, we identify factors that influence academics' productivity while working from home during the mandate to self-isolate. From analyzing results from a global survey we conducted, we found that both personal and technology-related factors affect an individual's attitude toward working from home and productivity. Our results should prove valuable to university administrators to better address the work-life challenges that academics face.
Since the beginning of the recent global refugee crisis, researchers have been tackling many of its associated aspects, investigating how we can help to alleviate this crisis, in particular, using ICTs capabilities. In our research, we investigated the use of ICT solutions by refugees to foster the social inclusion process in the host community. To tackle this topic, we conducted thirteen interviews with Syrian refugees in Germany. Our findings reveal different ICT usages by refugees and how these contribute to feeling empowered. Moreover, we show the sources of empowerment for refugees that are gained by ICT use. Finally, we identified the two types of social inclusion benefits that were derived from empowerment sources. Our results provide practical implications to different stakeholders and decision-makers on how ICT usage can empower refugees, which can foster the social inclusion of refugees, and what should be considered to support them in their integration effort.
Since the beginning of the recent global refugee crisis, researchers have been tackling many of its associated aspects, investigating how we can help to alleviate this crisis, in particular, using ICTs capabilities. In our research, we investigated the use of ICT solutions by refugees to foster the social inclusion process in the host community. To tackle this topic, we conducted thirteen interviews with Syrian refugees in Germany. Our findings reveal different ICT usages by refugees and how these contribute to feeling empowered. Moreover, we show the sources of empowerment for refugees that are gained by ICT use. Finally, we identified the two types of social inclusion benefits that were derived from empowerment sources. Our results provide practical implications to different stakeholders and decision-makers on how ICT usage can empower refugees, which can foster the social inclusion of refugees, and what should be considered to support them in their integration effort.
Weltweit brodelt es, Bürger gehen auf die Straße. In Chile will man sich die Ungerechtigkeiten des Bildungssystems nicht länger gefallen lassen. Nur wer zahlt, darf lernen – dagegen wehrt sich vor allem die Jugend mit aller Macht, auch mit der Macht der Neuen Medien. Öffentlichkeitswirksam werden die Proteste inszeniert. Wird die chilenische Regierung weiterhin mit Knüppeln auf Demonstranten einschlagen oder einlenken?