@inproceedings{Karvovskaya2013,
  author    = {Karvovskaya, Lena},
  title     = {'Also' in Ishkashimi : additive particle and sentence connector},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-66097},
  year      = {2013},
  abstract  = {The paper discusses the distribution and meaning of the additive particle -m@s in Ishkashimi. -m@s receives different semantic associations while staying in the same syntactic position. Thus, structurally combined with an object, it can semantically associate with the focused object or with the whole focused VP; similarly, combined with the subject it can semantically associate with the focused subject and with the whole focused sentence.},
  language  = {en}
}
@inproceedings{DrużbickaGibasTuszyńska2003,
  author    = {Drużbicka, Aleksandra and Gibas, Marta and Tuszyńska, Joanna},
  title     = {Świadomość językowa młodej inteligencji śląskiej},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-27755},
  year      = {2003},
  language  = {mul}
}
@inproceedings{OPUS4-6414,
  title     = {Zweite Woche des Russischen Rechts, Potsdam, 14.-18.05.2012, mit der Moskauer Staatlichen Juristischen O. E. Kutafin Universit{\"a}t (Akademie)},
  editor    = {Belling, Detlev W. and Fadeev, Vladimir Ivanovič},
  publisher = {Universit{\"a}tsverlag Potsdam},
  address   = {Potsdam},
  isbn      = {978-3-86956-221-6},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-63622},
  pages     = {223},
  year      = {2013},
  abstract  = {Die Moskauer Staatliche Juristische O. E. Kutafin Universit{\"a}t (Akademie) und die Juristische Fakult{\"a}t der Universit{\"a}t Potsdam arbeiten seit 2007 mit hohem wissenschaftlichem Ertrag zusammen. Ihre gemeinsamen Anstrengungen um das Verst{\"a}ndnis und die Entwicklung des Rechts in Russland und in Deutschland finden in den Wochen des Russischen Rechts ihren Ausdruck. In den Beitr{\"a}gen spiegelt sich das wissenschaftliche Denken auf dem Gebiet der Rechtswissenschaft zweier L{\"a}nder wider, deren Rechtsschulen seit jeher ein historisches Band verbindet. Ius est ars aequi et boni - Nach dem Wahren und Guten durch das Recht streben beide Partner. Den thematischen Schwerpunkt der 2. Woche des Russischen Rechts, Potsdam, 2012, bildeten - neben zivilrechtlichen Fragestellungen - das Zusammenwirken und der wechselseitige Einfluss von Staat und Kirche in Russland und Deutschland. Wo harsche Gegens{\"a}tze zwischen Staat und Kirche das Bild pr{\"a}gen, wo die eine Seite die andere gar bek{\"a}mpft, dominieren Unrecht und Willk{\"u}r. Wo aber zwischen Staat und Kirche gegenseitiges Vertrauen und Wohlwollen herrschen, wo Konflikte rechtsstaatlich, mithin friedlich, ausgetragen werden, l{\"a}sst sich das Wahre finden, und das Gute gedeiht. Diese Einsicht zu f{\"o}rdern und zu verbreiten, war ein Ziel der Konferenz.},
  language  = {de}
}
@inproceedings{ItzerottKaden2006,
  author    = {Itzerott, Sibylle and Kaden, Klaus},
  title     = {Zur G{\"u}te der automatisierten Erkennung von Ackerkulturen in Abh{\"a}ngigkeit vom Bodenmuster : Projektergebnisse und weiterf{\"u}hrende Ans{\"a}tze},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-7031},
  year      = {2006},
  abstract  = {Problemstellung • Geo{\"o}kologische Prozessforschung versucht f{\"u}r große Landschaftsausschnitte, die in der Natur ablaufenden und vom Menschen beeinflussten Prozesse mit Hilfe von Modellen nachzuvollziehen • exakte Erfassung der Ausstattung des Untersuchungsraumes ist wesentliche Voraussetzung f{\"u}r eine wirklichkeitsnahe Abbildung • Modelle derzeit weder in der Lage, alle ablaufenden Prozesse in die Betrachtung einzubeziehen, noch pr{\"a}zise Eingangsdaten bei der Beschreibung des Ausgangszustandes zu verarbeiten • h{\"a}ufig liegen Modelleingangsdaten nicht in der notwendigen Pr{\"a}zision vor • In Modellen wird Ausstattung eines Untersuchungsgebietes {\"u}ber den Boden, den Grundwassereinfluss und die Fl{\"a}chennutzung beschrieben • Fl{\"a}chennutzung besitzt weitgehend statische Elemente (Nutzungstypen Wald, Gew{\"a}sser, Siedlung) und hochdynamische Elemente (j{\"a}hrlicher Wechsel der Fruchtart auf jedem Acker) • Bedarf nach detaillierter (lage- und zeitkonkreter) Eingabe der Verteilung der Ackerfr{\"u}chte im Modellzeitraum, da Landwirtschaft als eine der bedeutenden Quellen f{\"u}r diffusen N{\"a}hrstoffeintrag ins {\"O}kosystem angesehen wird Stand der Forschung • bei Erfassung von Kulturen der Landwirtschaft aus Fernerkundungsdaten hat sich multitemporale Klassifizierung als sinnvoll erwiesen, weil sich anhand einer Einzelaufnahme die verschiedenen Kulturen nicht sicher trennen lassen • Klassifizierung erfolgt mit {\"u}berwachten Methoden unter Verwendung von Trainingsfl{\"a}chen im Datensatz, von denen die dort angebaute Frucht bekannt ist • in die Klassifizierung werden zus{\"a}tzliche Informationen einbezogen (Fuzzy), die Auskunft {\"u}ber die Wahrscheinlichkeit des Auftretens der Frucht geben (Anbaueignung in Abh{\"a}ngigkeit von Hangneigung, Niederschlag, H{\"o}henlage, Boden) Die Ergebnisse dieser Klassifikationen sind meist nicht auf andere Landschaftsausschnitte und Anbaujahre {\"u}bertragbar, weil die Auspr{\"a}gung der Spektralsignatur einer Kultur durch ver{\"a}nderte Boden- und Witterungsbedingungen variiert. L{\"o}sungsansatz • auf Basis von Satellitendaten und Anbauinformationen aus 15 aufeinander folgenden Jahren (35 Aufnahmetermine) sollten von Witterung und Boden unabh{\"a}ngige Jahreskurven der spektralen Charakteristik wichtiger Ackerkulturen gewonnen werden, die den Wachstumsverlauf der Pflanzen beschreiben • diese Kurven sollen anstelle von Trainingsgebieten zur multitemporalen Klassifizierung von Daten eines Anbaujahres herangezogen werden Schlussfolgerungen und Ausblick • Prinzipiell erscheint Vorgehen erfolgreich, jedoch in Abh{\"a}ngigkeit von der Brauchbarkeit der herangezogenen Szenen schwankt G{\"u}te des Ergebnisses noch • Verfahren stellt wesentlichen Fortschritt zu bisherigem Vorgehen auf Trainingsfl{\"a}chenbasis dar • ist zumindest im Untersuchungsgebiet immer wieder ohne weitere Kenntnis von Anbauinformationen anwendbar, lediglich exakte ph{\"a}nologische Datierung der dann verwendeten Aufnahmen erforderlich • f{\"u}r andere Gebiete (Variation in Niederschlag und Boden) ist Anpassung der ph{\"a}nologischen Datierung der Kurven erforderlich (Form ist weiter verwendbar) • optimale Bildkombination zur Trennung aller Kulturen ist: Anfang/Mitte April - Mitte Mai - Anfang Juli - Mitte August - Mitte September • Kombination sollte bei verbesserter Verf{\"u}gbarkeit von Daten beschaffbar sein • problematisch scheinen Trockensituationen im Mai und Juni zu sein, so dass zu schnell reifende Wintergetreide nicht richtig erkannt werden, Bedarf Bodeninformationen einzubeziehen • Trennung von Hackfr{\"u}chten weiterhin problematisch (wie schon in bisherigen Verfahren), f{\"u}hrt zu {\"u}berm{\"a}ßigen Anteilen im Ergebnis, in Abh{\"a}ngigkeit vom Anbauanteil besser vernachl{\"a}ssigen • Einbeziehung von Fuzzyinformationen erscheint sinnvoll • Zusammenhang von Bodeng{\"u}te und Frucht (Anbaueignung eines Bodens f{\"u}r eine Frucht) • Wasserverf{\"u}gbarkeit am Standort (in Abh{\"a}ngigkeit von Speicherverm{\"o}gen des Bodens, Grundwasseranschluss und Niederschlag) • Summe der Niederschl{\"a}ge bis zum Aufnahmezeitpunkt (Trockenheitsindex) <hr> Dokument 1: Foliensatz | Dokument 2: Abstract <hr> Interdisziplin{\"a}res Zentrum f{\"u}r Musterdynamik und Angewandte Fernerkundung Workshop vom 9. - 10. Februar 2006},
  language  = {de}
}
@inproceedings{Schultze2005,
  author    = {Schultze, Winfried},
  title     = {Zufall - Wunsch - Planung : die Erwerbung von Nachl{\"a}ssen zur Bestandserg{\"a}nzung},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-6098},
  year      = {2005},
  abstract  = {Nachl{\"a}sse sind pers{\"o}nliches Eigentum und unterliegen deshalb keiner Abgabepflicht. Der Wunsch des Nachlassers bez{\"u}glich der weiteren Aufbewahrung seines schriftlichen Erbes ist demzufolge prim{\"a}r gegen{\"u}ber allen unseren W{\"u}nschen. Wir k{\"o}nnen nicht fordern, sondern nur bitten, uns durch eigene Leistungen anbieten und die zuk{\"u}nftigen Nachlassenden oder deren Erben {\"u}berzeugen. Die nicht vorhandene institutionelle Zust{\"a}ndigkeit f{\"u}r die {\"U}bernahme von Nachl{\"a}ssen erzeugt die Reibungspunkte zwischen den Einrichtungen, die sich um den Erwerb von Nachl{\"a}ssen bem{\"u}hen: Archive - Bibliotheken - Museen - Sammlungen. Die W{\"u}nsche zum Erwerb des Nachlasses einer bestimmten Person - egal ob Wissenschaftler, K{\"u}nstler oder Politiker - sind demzufolge immer an verschiedenen Orten gleichzeitig vorhanden. Der Zufall entscheidet dann leider meist dar{\"u}ber, an welcher Stelle der Nachlass zuk{\"u}nftig verwahrt und wissenschaftlich genutzt wird. Es stellt sich die Frage, ob wir auf solche Zuf{\"a}lle hoffen und warten sollen, oder ob wir nicht eher eine engagierte - gemeinsam zwischen den Archiven abgestimmte - Erwerbspolitik betrieben sollten. ------------ Beitr{\"a}ge zum Thema "Nachl{\"a}sse an Universit{\"a}ts- und Hochschularchiven sowie Archiven wissenschaftlicher Institutionen" im Rahmen der Fr{\"u}hjahrstagung der Fachgruppe 8: "Archivare an Hochschularchiven und Archiven wissenschaftlicher Institutionen" am 16./17. Juni an der Universit{\"a}t Potsdam.},
  subject      = {Archiv},
  language  = {de}
}
@inproceedings{GebserHinrichsSchaubetal.2010,
  author    = {Gebser, Martin and Hinrichs, Henrik and Schaub, Torsten H. and Thiele, Sven},
  title     = {xpanda: a (simple) preprocessor for adding multi-valued propositions to ASP},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-41466},
  year      = {2010},
  abstract  = {We introduce a simple approach extending the input language of Answer Set Programming (ASP) systems by multi-valued propositions. Our approach is implemented as a (prototypical) preprocessor translating logic programs with multi-valued propositions into logic programs with Boolean propositions only. Our translation is modular and heavily benefits from the expressive input language of ASP. The resulting approach, along with its implementation, allows for solving interesting constraint satisfaction problems in ASP, showing a good performance.},
  language  = {en}
}
@inproceedings{RaassenHuchtMilleretal.2007,
  author    = {Raassen, A. J. J. and Hucht, K. A. van der and Miller, N. A. and Cassinelli, Joseph P.},
  title     = {XMM-Newton observations of zeta Orionis (O9.7 Ib) : a collisional ionization equilibrium model},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-17747},
  year      = {2007},
  abstract  = {We present the analysis of XMM-Newton observations of ζ Orionis. The analysis is based on fitting to the total spectrum as well as diagnostics of individual line.},
  language  = {en}
}
@inproceedings{OskinovaHamannFeldmeier2007,
  author    = {Oskinova, Lida and Hamann, Wolf-Rainer and Feldmeier, Achim},
  title     = {X-raying clumped stellar winds},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-18133},
  year      = {2007},
  abstract  = {X-ray spectroscopy is a sensitive probe of stellar winds. X-rays originate from optically thin shock-heated plasma deep inside the wind and propagate outwards throughout absorbing cool material. Recent analyses of the line ratios from He-like ions in the X-ray spectra of O-stars highlighted problems with this general paradigm: the measured line ratios of highest ions are consistent with the location of the hottest X-ray emitting plasma very close to the base of the wind, perhaps indicating the presence of a corona, while measurements from lower ions conform with the wind-embedded shock model. Generally, to correctly model the emerging Xray spectra, a detailed knowledge of the cool wind opacities based on stellar atmosphere models is prerequisite. A nearly grey stellar wind opacity for the X-rays is deduced from the analyses of high-resolution X-ray spectra. This indicates that the stellar winds are strongly clumped. Furthermore, the nearly symmetric shape of X-ray emission line profiles can be explained if the wind clumps are radially compressed. In massive binaries the orbital variations of X-ray emission allow to probe the opacity of the stellar wind; results support the picture of strong wind clumping. In high-mass X-ray binaries, the stochastic X-ray variability and the extend of the stellar-wind part photoionized by X-rays provide further strong evidence that stellar winds consist of dense clumps.},
  language  = {en}
}
@inproceedings{CassinelliIgnaceWaldronetal.2007,
  author    = {Cassinelli, Joseph P. and Ignace, R. and Waldron, W. and Cho, J. and Murphy, N. and Lazarian, A.},
  title     = {X-ray line emission produced in clump bow shocks},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-18057},
  year      = {2007},
  abstract  = {We summarize Chandra observations of the emission line profiles from 17 OB stars. The lines tend to be broad and unshifted. The forbidden/intercombination line ratios arising from Helium-like ions provide radial distance information for the X-ray emission sources, while the H-like to He-like line ratios provide X-ray temperatures, and thus also source temperature versus radius distributions. OB stars usually show power law differential emission measure distributions versus temperature. In models of bow shocks, we find a power law differential emission measure, a wide range of ion stages, and the bow shock flow around the clumps provides transverse velocities comparable to HWHM values. We find that the bow shock results for the line profile properties, consistent with the observations of X-ray line emission for a broad range of OB star properties.},
  language  = {en}
}
@inproceedings{Fiedlerowa2003,
  author    = {Fiedlerowa, Alicja},
  title     = {Wulgaryzmu wpływ na urodę języka},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-27779},
  year      = {2003},
  language  = {mul}
}
@inproceedings{OPUS4-8426,
  title     = {Wolf-Rayet Stars},
  editor    = {Hamann, Wolf-Rainer and Sander, Andreas Alexander Christoph and Todt, Helge Tobias},
  publisher = {Universit{\"a}tsverlag Potsdam},
  address   = {Potsdam},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-84268},
  year      = {2015},
  abstract  = {Nearly 150 years ago, the French astronomers Charles Wolf and Georges Rayet described stars with very conspicuous spectra that are dominated by bright and broad emission lines. Meanwhile termed Wolf-Rayet Stars after their discoverers, those objects turned out to represent important stages in the life of massive stars. As the first conference in a long time that was specifically dedicated to Wolf-Rayet stars, an international workshop was held in Potsdam, Germany, from 1.-5. June 2015. About 100 participants, comprising most of the leading experts in the field as well as as many young scientists, gathered for one week of extensive scientific exchange and discussions. Considerable progress has been reported throughout, e.g. on finding such stars, modeling and analyzing their spectra, understanding their evolutionary context, and studying their circumstellar nebulae. While some major questions regarding Wolf-Rayet stars still remain open 150 years after their discovery, it is clear today that these objects are not just interesting stars as such, but also keystones in the evolution of galaxies. These proceedings summarize the talks and posters presented at the Potsdam Wolf-Rayet workshop. Moreover, they also include the questions, comments, and discussions emerging after each talk, thereby giving a rare overview not only about the research, but also about the current debates and unknowns in the field. The Scientific Organizing Committee (SOC) included Alceste Bonanos (Athens), Paul Crowther (Sheffield), John Eldridge (Auckland), Wolf-Rainer Hamann (Potsdam, Chair), John Hillier (Pittsburgh), Claus Leitherer (Baltimore), Philip Massey (Flagstaff), George Meynet (Geneva), Tony Moffat (Montreal), Nicole St-Louis (Montreal), and Dany Vanbeveren (Brussels).},
  language  = {en}
}
@inproceedings{Szeifert2007,
  author    = {Szeifert, T.},
  title     = {Wind variabilities and asymmetries in Luminous Blue Variables},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-18146},
  year      = {2007},
  abstract  = {Luminous Blue Variables show strong changes in their stellar wind on time scales of typically years to decades when they expand and contract radially at approximately constant luminosity. Micro-variability on shorter time scales and amplitudes can be observed superimposed to the larger scale radial changes. I will show long-term time series of high resolution spectra which we have collected in the past 20 years for many of the well known LBVs together with a few time series of weekly sampling (HR Car, R40, R71, R110, R127, S Dor) covering a time windows of up to a few months. Wind variability is seen on short and intermediate time scales with the line profiles changing from P Cygni to inverse P Cygni and double peeked profiles sometimes for the same star and spectral line. On longer time scales the ionisation levels for all chemical elements change drastically due to the strong change of the temperature on the stellar surface. While on the long term the characteristic radial changes may have impact on the over all mass loss rates, the variabilities and asymmetries on short and intermediate time scales may cause false estimates of the mass loss rates when confronting models with the observed line profiles},
  language  = {en}
}
@inproceedings{Weis2007,
  author    = {Weis, K.},
  title     = {Wind relics : clumps, inhomogeneities and outflows in LBV nebulae},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-18235},
  year      = {2007},
  abstract  = {The most massive stars are those with the shortest but most active life. One group of massive stars, the Luminous Blue Variables (LBVs), of which only a few objects are known, are in particular of interest concerning the stability of stars. They have a high mass loss rate and are close to being instable. This is even more likely as rotation becomes an important factor in stellar evolution of these stars. Through massive stellar winds and sometimes giant eruptions, LBV nebulae are formed. Various aspects in the evolution in the LBV phase lead, beside the large scale morphological and kinematical differences, to a diversity of small structures like clumps, rims, and outflows in these nebulae.},
  language  = {en}
}
@inproceedings{Marchenko2007,
  author    = {Marchenko, S. V.},
  title     = {Wind inhomogeneities in low-Z environment : observations},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-17769},
  year      = {2007},
  abstract  = {We discuss the results of time-resolved spectroscopy of three presumably single Population I Wolf-Rayet stars in the Small Magellanic Cloud, where the ambient metallicity is \$\sim 1/5 Z_\odot\$. We were able to detect and follow numerous small-scale wind-embedded inhomogeneities in all observed stars. The general properties of the moving features, such as their velocity dispersions, emissivities and average accelerations, closely match the corresponding characteristics of small-scale inhomogeneities in the winds of Galactic Wolf-Rayet stars.},
  language  = {en}
}
@inproceedings{KrausKubatKrtička2007,
  author    = {Kraus, M. and Kub{\´a}t, Jiř{\´i} and Krtička, Jiri},
  title     = {Wind emission of OB supergiants and the influence of clumping},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-17757},
  year      = {2007},
  abstract  = {The influence of the wind to the total continuum of OB supergiants is discussed. For wind velocity distributions with β > 1.0, the wind can have strong influence to the total continuum emission, even at optical wavelengths. Comparing the continuum emission of clumped and unclumped winds, especially for stars with high β values, delivers flux differences of up to 30\% with maximum in the near-IR. Continuum observations at these wavelengths are therefore an ideal tool to discriminate between clumped and unclumped winds of OB supergiants.},
  language  = {en}
}
@inproceedings{Bartle2008,
  author    = {Bartle, Richard},
  title     = {When openness closes : the line between play and design},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-24536},
  year      = {2008},
  abstract  = {One of the informal properties often used to describe a new virtual world is its degree of openness. Yet what is an "open" virtual world? Does the phrase mean generally the same thing to different people? What distinguishes an open world from a less open world? Why does openness matter anyway? The answers to these questions cast light on an important, but shadowy, and uneasy, topic for virtual worlds: the relationship between those who construct the virtual, and those who use these constructions.},
  language  = {en}
}
@inproceedings{Rapp2015,
  author    = {Rapp, Michael Armin},
  title     = {When Local Poverty is More Important Than Your Income: Migrant Mental Health in Inner Cities},
  series = {European psychiatry : the journal of the Association of European Psychiatrists},
  volume    = {30},
  booktitle = {European psychiatry : the journal of the Association of European Psychiatrists},
  publisher = {Elsevier},
  address   = {Paris},
  issn      = {0924-9338},
  pages     = {1},
  year      = {2015},
  language  = {en}
}
@inproceedings{Apelojg2019,
  author    = {Apelojg, Benjamin},
  title     = {What´s going on?! Needs and emotions during classes},
  series = {9th International Conference on Society and Information Technologies (ICSIT 2018)},
  booktitle = {9th International Conference on Society and Information Technologies (ICSIT 2018)},
  number    = {1},
  publisher = {Curran Associates},
  address   = {Red Hook},
  isbn      = {978-1-5108-9702-1},
  pages     = {85 -- 88},
  year      = {2019},
  abstract  = {The "output-orientation" is omnipresent in teacher education. In order to evaluate teachers' and students' performances, a wide range of different quantitative questionnaires exist worldwide. One important goal of teaching evaluation is to increase the quality of teaching and learning. The author argues, that standard evaluations which are typically made at the end of the semester are problematic due to two reasons. The first one is that some of the questions are too general and don`t offer concrete ideas as to what kind of actions can be taken to make the courses better. The second problem is that the evaluation is mostly made when the course is already over. Because of this criticism, Apelojg invented the Felix-App which offers the possibility to give feedback in real-time by asking for the emotions and needs that occur during different learning situations. The idea is very simple: positive emotions and satisfied needs are helpful for the learning process. Negative emotions and unsatisfied needs have negative effects on the learning process. First descriptive results show, that "managing emotions" during classes can have positive effects on both motivation and emotions.},
  language  = {en}
}
@inproceedings{Zhou2010,
  author    = {Zhou, Neng-Fa},
  title     = {What I have learned from all these solver competitions},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-41431},
  year      = {2010},
  abstract  = {In this talk, I would like to share my experiences gained from participating in four CSP solver competitions and the second ASP solver competition. In particular, I'll talk about how various programming techniques can make huge differences in solving some of the benchmark problems used in the competitions. These techniques include global constraints, table constraints, and problem-specific propagators and labeling strategies for selecting variables and values. I'll present these techniques with experimental results from B-Prolog and other CLP(FD) systems.},
  language  = {en}
}
@inproceedings{ErmakovaFabianBenderetal.2018,
  author    = {Ermakova, Tatiana and Fabian, Benjamin and Bender, Benedict and Klimek, Kerstin},
  title     = {Web Tracking},
  series = {Proceedings of the Annual Hawaii International Conference on System Sciences (HICSS 51)},
  booktitle = {Proceedings of the Annual Hawaii International Conference on System Sciences (HICSS 51)},
  publisher = {HICSS Conference Office University of Hawaii at Manoa},
  address   = {Maile Way},
  issn      = {2572-6862},
  doi       = {10.24251/HICSS.2018.596},
  pages     = {4732 -- 4741},
  year      = {2018},
  abstract  = {Web tracking seems to become ubiquitous in online business and leads to increased privacy concerns of users. This paper provides an overview over the current state of the art of web-tracking research, aiming to reveal the relevance and methodologies of this research area and creates a foundation for future work. In particular, this study addresses the following research questions: What methods are followed? What results have been achieved so far? What are potential future research areas? For these goals, a structured literature review based upon an established methodological framework is conducted. The identified articles are investigated with respect to the applied research methodologies and the aspects of web tracking they emphasize.},
  language  = {en}
}