TY - JOUR A1 - Torres, D. F. A1 - Romero, G. E. A1 - Eiroa, E. F. A1 - Wambsganß, Joachim A1 - Pessah, M. E. T1 - Gravitational microlensing of gamma-ray blazars N2 - We present a detailed study of the effects of gravitational microlensing on compact and distant gamma-ray blazars. These objects have gamma-ray-emitting regions that are small enough to be affected by microlensing effects produced by stars lying in intermediate galaxies. We compute the gravitational magnification taking into account effects of the lensing and show that, whereas the innermost gamma-ray spheres can be significantly magnified, there is little magnification either for very high gamma-ray energies or for lower (radio) frequencies (because these wavelengths are emitted from larger regions). We analyse the temporal evolution of the gamma-ray magnification for sources moving in a caustic pattern field, where the combined effects of thousands of stars are taken into account using a numerical technique. We propose that some of the unidentified gamma-ray sources (particularly some of those lying at high galactic latitude with gamma-ray statistical properties that are very similar to detected gamma-ray blazars) are indeed the result of gravitational lensing magnification of background undetected active galactic nuclei (AGN). This is partly supported from a statistical point of view: we show herein as well, using the latest information from the third EGRET catalogue, that high-latitude gamma-ray sources have similar averaged properties to already detected gamma-ray AGN. Some differences between both samples, regarding the mean flux level, could also be understood within the lensing model. With an adequate selection of lensing parameters, it is possible to explain a variety of gamma-ray light curves with different time-scales, including non-variable sources. The absence of strong radio counterparts could be naturally explained by differential magnification in the extended source formalism. Y1 - 2003 ER - TY - JOUR A1 - Rodríguez-Quiles y García, José A. A1 - Soria Torres, Carmen M. T1 - Musique et Communautés d’Apprentissage JF - Potsdamer Schriftenreihe zur Musikpädagogik Y1 - 2019 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-433858 IS - 7 SP - 93 EP - 114 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - BOOK A1 - Rodríguez-Quiles y García, José A. A1 - Habib, Michel A1 - Bidal-Loton, Marie-Pierre A1 - Leveau, Nicolas A1 - Tassin, Martine A1 - Verlinden, Dominique A1 - Soria Torres, Carmen M. A1 - Hoonhorst, Ingrid A1 - Vancamp, Marielle A1 - Dormoy, Alice A1 - De Barelli, Tatiana ED - Rodríguez-Quiles y García, José A. T1 - Bienfaits de la musique á l'école T1 - Beneficios de la música en la escuela T1 - Benefits of music at school T1 - Vorzüge der Musik in der Schule BT - une expérience européenne BT - una experiencia europea BT - a European experience BT - eine europäische Erfahrung N2 - A l'heure où l'éducation musicale est remise en cause par les décideurs de certains pays de l'Union européenne, la collaboration internationale et interdisciplinaire est plus que jamais nécessaire pour démontrer l'erreur de ces attitudes. A cette fin, l'ouvrage rassemble les réflexions de différents spécialistes de trois pays européens qui offrent leurs points de vue sous le prisme de l'éducation musicale mais aussi des domaines des neurosciences, de la psychologie, de la logopédie et de la politique. Cette publication combine les résultats de travaux empiriques avec des propositions pratiques, ce qui la rend utile pour les chercheurs, les professeurs de musique et les orthophonistes. N2 - En unos tiempos en los que la educación musical viene siendo cuestionada por los responsables de las políticas educativas de ciertos países de la Unión Europea, se hace más necesaria que nunca una colaboración internacional e interdisciplinar que demuestre lo erróneo de tales actitudes. Con esta finalidad, el libro recoge las reflexiones de diferentes especialistas de tres países europeos quienes ofrecen sus puntos de vista desde el prismade la educación musical pero también, desde los ámbitos de la neurociencia, la psicología, la logopedia y la política. La presente publicación aúna resultados de trabajos empíricos con propuestas de tipo práctico, lo que la hace útil tanto para investigadores, como para docentes, profesores de música y logopedas. N2 - At a time when music education is being questioned by education policy-makers in certain European Union countries, international and interdisciplinary collaboration is needed more than ever to demonstrate the error of such attitudes. To this end, the book gathers the reflections of different specialists from three European countries who offer their points of view from a musical education prism but also from the fields of neuroscience, psychology, speech therapy and politics. This publication combines the results of empirical work with practical proposals, which makes it useful for researchers, music teachers and speech therapists. N2 - In einer Zeit in der die Musikpädagogik von den für die Erziehungsrichtlinien Verantwortlichen in bestimmten Ländern der Europäischen Union in Frage gestellt wird, ist eine interdisziplinäre und internationale Zusammenarbeit, die belegt, dass eine solche Einstellung falsch ist, notwendiger denn je. Zu diesem Zweck sind in diesem Buch die Überlegungen verschiedener Experten aus drei europäischen Ländern zusammengefasst, die ihre Sichtweise aus der Perspektive der Musikpädagogik, aber auch der Neurologie, der Psychologie, der Logopädie und der Politik anbieten. Die vorliegende Veröffentlichung vereint Ergebnisse empirischer Arbeit mit praktischen Vorschlägen, was sie sowohl für Forschung als auch für Musiklehrer und Logopäden nützlich macht. T3 - Potsdamer Schriftenreihe zur Musikpädagogik - 7 KW - education musicale KW - neurosciences et musique KW - communautés d'apprentissage KW - activités musicales KW - déclaration de Marseille KW - educación musical KW - neurociencia y música KW - comunidades de aprendizaje KW - actividades musicales KW - declaración de Marsella KW - musical Education KW - neuroscience and music KW - learning communities KW - musical activities KW - Marseille declaration KW - Musikpädagogik KW - Neurowissenschaft und Musik KW - Lerngemeinschaften KW - musikalische Aktivitäten KW - Deklaration von Marseille Y1 - 2019 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-428627 SN - 978-3-86956-466-1 SN - 1861-8529 SN - 2196-5080 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - JOUR A1 - Pena, M. A1 - Hamann, Wolf-Rainer A1 - Koesterke, Lars A1 - Maza, J. A1 - Mendez, R. H. A1 - Peimbert, M. A1 - Ruiz, M. T. A1 - Torres-Peimbert, S. T1 - HST spectrophotometric data of the central star of the planetary nebula LMC-N66 Y1 - 1997 ER - TY - JOUR A1 - Pena, M. A1 - Hamann, Wolf-Rainer A1 - Koesterke, Lars A1 - Maza, J. A1 - Mendez, R. H. A1 - Peimbert, M. A1 - Ruiz, M. T. A1 - Torres-Peimbert, S. T1 - Spectrophotometric data of the central star of the large magellanic cloud planetary nebula N66. Quantitative analysis of its WN type spectrum Y1 - 1997 ER - TY - JOUR A1 - González-Fortes, Gloria M. A1 - Kolbe, Ben A1 - Fernandes, Daniel A1 - Meleg, Ioana N. A1 - Garcia-Vazquez, Ana A1 - Pinto-Llona, Ana C. A1 - Constantin, Silviu A1 - de Torres, Trino J. A1 - Ortiz, Jose E. A1 - Frischauf, Christine A1 - Rabeder, Gernot A1 - Hofreiter, Michael A1 - Barlow, Axel T1 - Ancient DNA reveals differences in behaviour and sociality between brown bears and extinct cave bears JF - Molecular ecology N2 - Ancient DNA studies have revolutionized the study of extinct species and populations, providing insights on phylogeny, phylogeography, admixture and demographic history. However, inferences on behaviour and sociality have been far less frequent. Here, we investigate the complete mitochondrial genomes of extinct Late Pleistocene cave bears and middle Holocene brown bears that each inhabited multiple geographically proximate caves in northern Spain. In cave bears, we find that, although most caves were occupied simultaneously, each cave almost exclusively contains a unique lineage of closely related haplotypes. This remarkable pattern suggests extreme fidelity to their birth site in cave bears, best described as homing behaviour, and that cave bears formed stable maternal social groups at least for hibernation. In contrast, brown bears do not show any strong association of mitochondrial lineage and cave, suggesting that these two closely related species differed in aspects of their behaviour and sociality. This difference is likely to have contributed to cave bear extinction, which occurred at a time in which competition for caves between bears and humans was likely intense and the ability to rapidly colonize new hibernation sites would have been crucial for the survival of a species so dependent on caves for hibernation as cave bears. Our study demonstrates the potential of ancient DNA to uncover patterns of behaviour and sociality in ancient species and populations, even those that went extinct many tens of thousands of years ago. KW - ancient DNA KW - extinction KW - homing KW - sociality KW - Ursus arctos KW - Ursus spelaeus Y1 - 2016 U6 - https://doi.org/10.1111/mec.13800 SN - 0962-1083 SN - 1365-294X VL - 25 SP - 4907 EP - 4918 PB - Wiley-Blackwell CY - Hoboken ER - TY - JOUR A1 - Furniss, A. A1 - Noda, K. A1 - Boggs, S. A1 - Chiang, J. A1 - Christensen, F. A1 - Craig, W. A1 - Giommi, P. A1 - Hailey, C. A1 - Harisson, F. A1 - Madejski, G. A1 - Nalewajko, K. A1 - Perri, M. A1 - Stern, D. A1 - Urry, M. A1 - Verrecchia, F. A1 - Zhang, W. A1 - Ahnen, M. L. A1 - Ansoldi, S. A1 - Antonelli, L. A. A1 - Antoranz, P. A1 - Babic, A. A1 - Banerjee, B. A1 - Bangale, P. A1 - de Almeida, U. Barres A1 - Barrio, J. A. A1 - Becerra Gonzalez, J. A1 - Bednarek, W. A1 - Bernardini, E. A1 - Biasuzzi, B. A1 - Biland, A. A1 - Blanch Bigas, O. A1 - Bonnefoy, S. A1 - Bonnoli, G. A1 - Borracci, F. A1 - Bretz, T. A1 - Carmona, E. A1 - Carosi, A. A1 - Chatterjee, A. A1 - Clavero, R. A1 - Colin, P. A1 - Colombo, E. A1 - Contreras, J. L. A1 - Cortina, J. A1 - Covino, S. A1 - Da Vela, P. A1 - Dazzi, F. A1 - De Angelis, A. A1 - De Caneva, G. A1 - De Lotto, B. A1 - de Ona Wilhelmi, E. A1 - Delgado Mendez, C. A1 - Di Pierro, F. A1 - Prester, Dijana Dominis A1 - Dorner, D. A1 - Doro, M. A1 - Einecke, S. A1 - Eisenacher Glawion, D. A1 - Elsaesser, D. A1 - Fernandez-Barral, A. A1 - Fidalgo, D. A1 - Fonseca, M. V. A1 - Font, L. A1 - Frantzen, K. A1 - Fruck, C. A1 - Galindo, D. A1 - Garcia Lopez, R. J. A1 - Garczarczyk, M. A1 - Garrido Terrats, D. A1 - Gaug, M. A1 - Giammaria, P. A1 - Godinovic, N. A1 - Gonzalez Munoz, A. A1 - Guberman, D. A1 - Hanabata, Y. A1 - Hayashida, M. A1 - Herrera, J. A1 - Hose, J. A1 - Hrupec, D. A1 - Hughes, G. A1 - Idec, W. A1 - Kellermann, H. A1 - Kodani, K. A1 - Konno, Y. A1 - Kubo, H. A1 - Kushida, J. A1 - La Barbera, A. A1 - Lelas, D. A1 - Lewandowska, N. A1 - Lindfors, E. A1 - Lombardi, S. A1 - Longo, F. A1 - Lopez, M. A1 - Lopez-Coto, R. A1 - Lopez-Oramas, A. A1 - Lorenz, E. A1 - Majumdar, P. A1 - Makariev, M. A1 - Mallot, K. A1 - Maneva, G. A1 - Manganaro, M. A1 - Mannheim, K. A1 - Maraschi, L. A1 - Marcote, B. A1 - Mariotti, M. A1 - Martinez, M. A1 - Mazin, D. A1 - Menzel, U. A1 - Miranda, J. M. A1 - Mirzoyan, R. A1 - Moralejo, A. A1 - Nakajima, D. A1 - Neustroev, V. A1 - Niedzwiecki, A. A1 - Nievas Rosillo, M. A1 - Nilsson, K. A1 - Nishijima, K. A1 - Orito, R. A1 - Overkemping, A. A1 - Paiano, S. A1 - Palacio, J. A1 - Palatiello, M. A1 - Paneque, D. A1 - Paoletti, R. A1 - Paredes, J. M. A1 - Paredes-Fortuny, X. A1 - Persic, M. A1 - Poutanen, J. A1 - Moroni, P. G. Prada A1 - Prandini, E. A1 - Puljak, I. A1 - Reinthal, R. A1 - Rhode, W. A1 - Ribo, M. A1 - Rico, J. A1 - Garcia, J. Rodriguez A1 - Saito, T. A1 - Saito, K. A1 - Satalecka, K. A1 - Scapin, V. A1 - Schultz, C. A1 - Schweizer, T. A1 - Shore, S. N. A1 - Sillanpaa, A. A1 - Sitarek, J. A1 - Snidaric, I. A1 - Sobczynska, D. A1 - Stamerra, A. A1 - Steinbring, T. A1 - Strzys, M. A1 - Takalo, L. A1 - Takami, H. A1 - Tavecchio, F. A1 - Temnikov, P. A1 - Terzic, T. A1 - Tescaro, D. A1 - Teshima, M. A1 - Thaele, J. A1 - Torres, D. F. A1 - Toyama, T. A1 - Treves, A. A1 - Verguilov, V. A1 - Vovk, I. A1 - Will, M. A1 - Zanin, R. A1 - Archer, A. A1 - Benbow, W. A1 - Bird, R. A1 - Biteau, Jonathan A1 - Bugaev, V. A1 - Cardenzana, J. V. A1 - Cerruti, M. A1 - Chen, Xuhui A1 - Ciupik, L. A1 - Connolly, M. P. A1 - Cui, W. A1 - Dickinson, H. J. A1 - Dumm, J. A1 - Eisch, J. D. A1 - Falcone, A. A1 - Feng, Q. A1 - Finley, J. P. A1 - Fleischhack, H. A1 - Fortin, P. A1 - Fortson, L. A1 - Gerard, L. A1 - Gillanders, G. H. A1 - Griffin, S. A1 - Griffiths, S. T. A1 - Grube, J. A1 - Gyuk, G. A1 - Hakansson, Nils A1 - Holder, J. A1 - Humensky, T. B. A1 - Johnson, C. A. A1 - Kaaret, P. A1 - Kertzman, M. A1 - Kieda, D. A1 - Krause, M. A1 - Krennrich, F. A1 - Lang, M. J. A1 - Lin, T. T. Y. A1 - Maier, G. A1 - McArthur, S. A1 - McCann, A. A1 - Meagher, K. A1 - Moriarty, P. A1 - Mukherjee, R. A1 - Nieto, D. A1 - Ong, R. A. A1 - Park, N. A1 - Petry, D. A1 - Pohl, Martin A1 - Popkow, A. A1 - Ragan, K. A1 - Ratliff, G. A1 - Reyes, L. C. A1 - Reynolds, P. T. A1 - Richards, G. T. A1 - Roache, E. A1 - Santander, M. A1 - Sembroski, G. H. A1 - Shahinyan, K. A1 - Staszak, D. A1 - Telezhinsky, Igor O. A1 - Tucci, J. V. A1 - Tyler, J. A1 - Vassiliev, V. V. A1 - Wakely, S. P. A1 - Weiner, O. M. A1 - Weinstein, A. A1 - Wilhelm, Alina A1 - Williams, D. A. A1 - Zitzer, B. A1 - Vince, O. A1 - Fuhrmann, L. A1 - Angelakis, E. A1 - Karamanavis, V. A1 - Myserlis, I. A1 - Krichbaum, T. P. A1 - Zensus, J. A. A1 - Ungerechts, H. A1 - Sievers, A. A1 - Bachev, R. A1 - Boettcher, Markus A1 - Chen, W. P. A1 - Damljanovic, G. A1 - Eswaraiah, C. A1 - Guver, T. A1 - Hovatta, T. A1 - Hughes, Z. A1 - Ibryamov, S. I. A1 - Joner, M. D. A1 - Jordan, B. A1 - Jorstad, S. G. A1 - Joshi, M. A1 - Kataoka, J. A1 - Kurtanidze, O. M. A1 - Kurtanidze, S. O. A1 - Lahteenmaki, A. A1 - Latev, G. A1 - Lin, H. C. A1 - Larionov, V. M. A1 - Mokrushina, A. A. A1 - Morozova, D. A. A1 - Nikolashvili, M. G. A1 - Raiteri, C. M. A1 - Ramakrishnan, V. A1 - Readhead, A. C. R. A1 - Sadun, A. C. A1 - Sigua, L. A. A1 - Semkov, E. H. A1 - Strigachev, A. A1 - Tammi, J. A1 - Tornikoski, M. A1 - Troitskaya, Y. V. A1 - Troitsky, I. S. A1 - Villata, M. T1 - First NuSTAR observations of MRK 501 within a radio to TeV multi-instrument campaign JF - The astrophysical journal : an international review of spectroscopy and astronomical physics N2 - We report on simultaneous broadband observations of the TeV-emitting blazar Markarian 501 between 2013 April 1 and August 10, including the first detailed characterization of the synchrotron peak with Swift and NuSTAR. During the campaign, the nearby BL Lac object was observed in both a quiescent and an elevated state. The broadband campaign includes observations with NuSTAR, MAGIC, VERITAS, the Fermi Large Area Telescope, Swift X-ray Telescope and UV Optical Telescope, various ground-based optical instruments, including the GASP-WEBT program, as well as radio observations by OVRO, Metsahovi, and the F-Gamma consortium. Some of the MAGIC observations were affected by a sand layer from the Saharan desert, and had to be corrected using event-by-event corrections derived with a Light Detection and Ranging (LIDAR) facility. This is the first time that LIDAR information is used to produce a physics result with Cherenkov Telescope data taken during adverse atmospheric conditions, and hence sets a precedent for the current and future ground-based gamma-ray instruments. The NuSTAR instrument provides unprecedented sensitivity in hard X-rays, showing the source to display a spectral energy distribution (SED) between 3 and 79 keV consistent with a log-parabolic spectrum and hard X-ray variability on hour timescales. None (of the four extended NuSTAR observations) show evidence of the onset of inverse-Compton emission at hard X-ray energies. We apply a single-zone equilibrium synchrotron self-Compton (SSC) model to five simultaneous broadband SEDs. We find that the SSC model can reproduce the observed broadband states through a decrease in the magnetic field strength coinciding with an increase in the luminosity and hardness of the relativistic leptons responsible for the high-energy emission. KW - BL Lacertae objects: general KW - galaxies: individual (Markarian 501) KW - X-rays: galaxies Y1 - 2015 U6 - https://doi.org/10.1088/0004-637X/812/1/65 SN - 0004-637X SN - 1538-4357 VL - 812 IS - 1 PB - IOP Publ. Ltd. CY - Bristol ER - TY - JOUR A1 - De Angelis, A. A1 - Tatischeff, V. A1 - Grenier, I. A. A1 - McEnery, J. A1 - Mallamaci, Manuela A1 - Tavani, M. A1 - Oberlack, U. A1 - Hanlon, L. A1 - Walter, R. A1 - Argan, A. A1 - Von Ballmoos, P. A1 - Bulgarelli, A. A1 - Bykov, A. A1 - Hernanz, M. A1 - Kanbach, G. A1 - Kuvvetli, I. A1 - Pearce, M. A1 - Zdziarski, A. A1 - Conrad, J. A1 - Ghisellini, G. A1 - Harding, A. A1 - Isern, J. A1 - Leising, M. A1 - Longo, F. A1 - Madejski, G. A1 - Martinez, M. A1 - Mazziotta, Mario Nicola A1 - Paredes, J. M. A1 - Pohl, Martin A1 - Rando, R. A1 - Razzano, M. A1 - Aboudan, A. A1 - Ackermann, M. A1 - Addazi, A. A1 - Ajello, M. A1 - Albertus, C. A1 - Alvarez, J. M. A1 - Ambrosi, G. A1 - Anton, S. A1 - Antonelli, L. A. A1 - Babic, A. A1 - Baibussinov, B. A1 - Balbom, M. A1 - Baldini, L. A1 - Balman, S. A1 - Bambi, C. A1 - Barres de Almeida, U. A1 - Barrio, J. A. A1 - Bartels, R. A1 - Bastieri, D. A1 - Bednarek, W. A1 - Bernard, D. A1 - Bernardini, E. A1 - Bernasconi, T. A1 - Bertucci, B. A1 - Biland, A. A1 - Bissaldi, E. A1 - Boettcher, M. A1 - Bonvicini, V. A1 - Bosch-Ramon, V. A1 - Bottacini, E. A1 - Bozhilov, V. A1 - Bretz, T. A1 - Branchesi, M. A1 - Brdar, V. A1 - Bringmann, T. A1 - Brogna, A. A1 - Jorgensen, C. Budtz A1 - Busetto, G. A1 - Buson, S. A1 - Busso, M. A1 - Caccianiga, A. A1 - Camera, S. A1 - Campana, R. A1 - Caraveo, P. A1 - Cardillo, M. A1 - Carlson, P. A1 - Celestin, S. A1 - Cermeno, M. A1 - Chen, A. A1 - Cheung, C. C. A1 - Churazov, E. A1 - Ciprini, S. A1 - Coc, A. A1 - Colafrancesco, S. A1 - Coleiro, A. A1 - Collmar, W. A1 - Coppi, P. A1 - Curado da Silva, R. A1 - Cutini, S. A1 - De Lotto, B. A1 - de Martino, D. A1 - De Rosa, A. A1 - Del Santo, M. A1 - Delgado, L. A1 - Diehl, R. A1 - Dietrich, S. A1 - Dolgov, A. D. A1 - Dominguez, A. A1 - Prester, D. Dominis A1 - Donnarumma, I. A1 - Dorner, D. A1 - Doro, M. A1 - Dutra, M. A1 - Elsaesser, D. A1 - Fabrizio, M. A1 - Fernandez-Barral, A. A1 - Fioretti, V. A1 - Foffano, L. A1 - Formato, V. A1 - Fornengo, N. A1 - Foschini, L. A1 - Franceschini, A. A1 - Franckowiak, A. A1 - Funk, S. A1 - Fuschino, F. A1 - Gaggero, D. A1 - Galanti, G. A1 - Gargano, F. A1 - Gasparrini, D. A1 - Gehrz, R. A1 - Giammaria, P. A1 - Giglietto, N. A1 - Giommi, P. A1 - Giordano, F. A1 - Giroletti, M. A1 - Ghirlanda, G. A1 - Godinovic, N. A1 - Gouiffes, C. A1 - Grove, J. E. A1 - Hamadache, C. A1 - Hartmann, D. H. A1 - Hayashida, M. A1 - Hryczuk, A. A1 - Jean, P. A1 - Johnson, T. A1 - Jose, J. A1 - Kaufmann, S. A1 - Khelifi, B. A1 - Kiener, J. A1 - Knodlseder, J. A1 - Kolem, M. A1 - Kopp, J. A1 - Kozhuharov, V. A1 - Labanti, C. A1 - Lalkovski, S. A1 - Laurent, P. A1 - Limousin, O. A1 - Linares, M. A1 - Lindfors, E. A1 - Lindner, M. A1 - Liu, J. A1 - Lombardi, S. A1 - Loparco, F. A1 - Lopez-Coto, R. A1 - Lopez Moya, M. A1 - Lott, B. A1 - Lubrano, P. A1 - Malyshev, D. A1 - Mankuzhiyil, N. A1 - Mannheim, K. A1 - Marcha, M. J. A1 - Marciano, A. A1 - Marcote, B. A1 - Mariotti, M. A1 - Marisaldi, M. A1 - McBreen, S. A1 - Mereghetti, S. A1 - Merle, A. A1 - Mignani, R. A1 - Minervini, G. A1 - Moiseev, A. A1 - Morselli, A. A1 - Moura, F. A1 - Nakazawa, K. A1 - Nava, L. A1 - Nieto, D. A1 - Orienti, M. A1 - Orio, M. A1 - Orlando, E. A1 - Orleanski, P. A1 - Paiano, S. A1 - Paoletti, R. A1 - Papitto, A. A1 - Pasquato, M. A1 - Patricelli, B. A1 - Perez-Garcia, M. A. A1 - Persic, M. A1 - Piano, G. A1 - Pichel, A. A1 - Pimenta, M. A1 - Pittori, C. A1 - Porter, T. A1 - Poutanen, J. A1 - Prandini, E. A1 - Prantzos, N. A1 - Produit, N. A1 - Profumo, S. A1 - Queiroz, F. S. A1 - Raino, S. A1 - Raklev, A. A1 - Regis, M. A1 - Reichardt, I. A1 - Rephaeli, Y. A1 - Rico, J. A1 - Rodejohann, W. A1 - Fernandez, G. Rodriguez A1 - Roncadelli, M. A1 - Roso, L. A1 - Rovero, A. A1 - Ruffini, R. A1 - Sala, G. A1 - Sanchez-Conde, M. A. A1 - Santangelo, Andrea A1 - Parkinson, P. Saz A1 - Sbarrato, T. A1 - Shearer, A. A1 - Shellard, R. A1 - Short, K. A1 - Siegert, T. A1 - Siqueira, C. A1 - Spinelli, P. A1 - Stamerra, A. A1 - Starrfield, S. A1 - Strong, A. A1 - Strumke, I. A1 - Tavecchio, F. A1 - Taverna, R. A1 - Terzic, T. A1 - Thompson, D. J. A1 - Tibolla, O. A1 - Torres, D. F. A1 - Turolla, R. A1 - Ulyanov, A. A1 - Ursi, A. A1 - Vacchi, A. A1 - Van den Abeele, J. A1 - Vankova-Kirilovai, G. A1 - Venter, C. A1 - Verrecchia, F. A1 - Vincent, P. A1 - Wang, X. A1 - Weniger, C. A1 - Wu, X. A1 - Zaharijas, G. A1 - Zampieri, L. A1 - Zane, S. A1 - Zimmer, S. A1 - Zoglauer, A. T1 - Science with e-ASTROGAM A space mission for MeV-GeV gamma-ray astrophysics JF - Journal of High Energy Astrophysics Y1 - 2018 U6 - https://doi.org/10.1016/j.jheap.2018.07.001 SN - 2214-4048 SN - 2214-4056 VL - 19 SP - 1 EP - 106 PB - Elsevier CY - Amsterdam ER - TY - JOUR A1 - Chipman, Ariel D. A1 - Ferrier, David E. K. A1 - Brena, Carlo A1 - Qu, Jiaxin A1 - Hughes, Daniel S. T. A1 - Schroeder, Reinhard A1 - Torres-Oliva, Montserrat A1 - Znassi, Nadia A1 - Jiang, Huaiyang A1 - Almeida, Francisca C. A1 - Alonso, Claudio R. A1 - Apostolou, Zivkos A1 - Aqrawi, Peshtewani A1 - Arthur, Wallace A1 - Barna, Jennifer C. J. A1 - Blankenburg, Kerstin P. A1 - Brites, Daniela A1 - Capella-Gutierrez, Salvador A1 - Coyle, Marcus A1 - Dearden, Peter K. A1 - Du Pasquier, Louis A1 - Duncan, Elizabeth J. A1 - Ebert, Dieter A1 - Eibner, Cornelius A1 - Erikson, Galina A1 - Evans, Peter D. A1 - Extavour, Cassandra G. A1 - Francisco, Liezl A1 - Gabaldon, Toni A1 - Gillis, William J. A1 - Goodwin-Horn, Elizabeth A. A1 - Green, Jack E. A1 - Griffiths-Jones, Sam A1 - Grimmelikhuijzen, Cornelis J. P. A1 - Gubbala, Sai A1 - Guigo, Roderic A1 - Han, Yi A1 - Hauser, Frank A1 - Havlak, Paul A1 - Hayden, Luke A1 - Helbing, Sophie A1 - Holder, Michael A1 - Hui, Jerome H. L. A1 - Hunn, Julia P. A1 - Hunnekuhl, Vera S. A1 - Jackson, LaRonda A1 - Javaid, Mehwish A1 - Jhangiani, Shalini N. A1 - Jiggins, Francis M. A1 - Jones, Tamsin E. A1 - Kaiser, Tobias S. A1 - Kalra, Divya A1 - Kenny, Nathan J. A1 - Korchina, Viktoriya A1 - Kovar, Christie L. A1 - Kraus, F. Bernhard A1 - Lapraz, Francois A1 - Lee, Sandra L. A1 - Lv, Jie A1 - Mandapat, Christigale A1 - Manning, Gerard A1 - Mariotti, Marco A1 - Mata, Robert A1 - Mathew, Tittu A1 - Neumann, Tobias A1 - Newsham, Irene A1 - Ngo, Dinh N. A1 - Ninova, Maria A1 - Okwuonu, Geoffrey A1 - Ongeri, Fiona A1 - Palmer, William J. A1 - Patil, Shobha A1 - Patraquim, Pedro A1 - Pham, Christopher A1 - Pu, Ling-Ling A1 - Putman, Nicholas H. A1 - Rabouille, Catherine A1 - Ramos, Olivia Mendivil A1 - Rhodes, Adelaide C. A1 - Robertson, Helen E. A1 - Robertson, Hugh M. A1 - Ronshaugen, Matthew A1 - Rozas, Julio A1 - Saada, Nehad A1 - Sanchez-Gracia, Alejandro A1 - Scherer, Steven E. A1 - Schurko, Andrew M. A1 - Siggens, Kenneth W. A1 - Simmons, DeNard A1 - Stief, Anna A1 - Stolle, Eckart A1 - Telford, Maximilian J. A1 - Tessmar-Raible, Kristin A1 - Thornton, Rebecca A1 - van der Zee, Maurijn A1 - von Haeseler, Arndt A1 - Williams, James M. A1 - Willis, Judith H. A1 - Wu, Yuanqing A1 - Zou, Xiaoyan A1 - Lawson, Daniel A1 - Muzny, Donna M. A1 - Worley, Kim C. A1 - Gibbs, Richard A. A1 - Akam, Michael A1 - Richards, Stephen T1 - The first myriapod genome sequence reveals conservative arthropod gene content and genome organisation in the centipede Strigamia maritima JF - PLoS biology N2 - Myriapods (e. g., centipedes and millipedes) display a simple homonomous body plan relative to other arthropods. All members of the class are terrestrial, but they attained terrestriality independently of insects. Myriapoda is the only arthropod class not represented by a sequenced genome. We present an analysis of the genome of the centipede Strigamia maritima. It retains a compact genome that has undergone less gene loss and shuffling than previously sequenced arthropods, and many orthologues of genes conserved from the bilaterian ancestor that have been lost in insects. Our analysis locates many genes in conserved macro-synteny contexts, and many small-scale examples of gene clustering. We describe several examples where S. maritima shows different solutions from insects to similar problems. The insect olfactory receptor gene family is absent from S. maritima, and olfaction in air is likely effected by expansion of other receptor gene families. For some genes S. maritima has evolved paralogues to generate coding sequence diversity, where insects use alternate splicing. This is most striking for the Dscam gene, which in Drosophila generates more than 100,000 alternate splice forms, but in S. maritima is encoded by over 100 paralogues. We see an intriguing linkage between the absence of any known photosensory proteins in a blind organism and the additional absence of canonical circadian clock genes. The phylogenetic position of myriapods allows us to identify where in arthropod phylogeny several particular molecular mechanisms and traits emerged. For example, we conclude that juvenile hormone signalling evolved with the emergence of the exoskeleton in the arthropods and that RR-1 containing cuticle proteins evolved in the lineage leading to Mandibulata. We also identify when various gene expansions and losses occurred. The genome of S. maritima offers us a unique glimpse into the ancestral arthropod genome, while also displaying many adaptations to its specific life history. Y1 - 2014 U6 - https://doi.org/10.1371/journal.pbio.1002005 SN - 1545-7885 VL - 12 IS - 11 PB - PLoS CY - San Fransisco ER - TY - JOUR A1 - Bernardi, Rafael L. A1 - Berdja, Amokrane A1 - Dani Guzman, Christian A1 - Torres-Torriti, Miguel A1 - Roth, Martin M. T1 - Restoration of images with a spatially varying PSF of the T80-S telescope optical model using neural networks JF - Monthly notices of the Royal Astronomical Society N2 - Most image restoration methods in astronomy rely upon probabilistic tools that infer the best solution for a deconvolution problem. They achieve good performances when the point spread function (PSF) is spatially invariant in the image plane. However, this condition is not always satisfied in real optical systems. We propose a new method for the restoration of images affected by static and anisotropic aberrations using Deep Neural Networks that can be directly applied to sky images. The network is trained using simulated sky images corresponding to the T80-S Telescope optical model, a 80-cm survey imager at Cerro Tololo (Chile), which are synthesized using a Zernike polynomial representation of the optical system. Once trained, the network can be used directly on sky images, outputting a corrected version of the image that has a constant and known PSF across its field of view. The method is to be tested on the T80-S Telescope. We present the method and results on synthetic data. KW - methods: statistical KW - techniques: image processing Y1 - 2021 U6 - https://doi.org/10.1093/mnras/stab3400 SN - 0035-8711 SN - 1365-2966 VL - 510 IS - 3 SP - 4284 EP - 4294 PB - Oxford Univ. Press CY - Oxford ER -