Book.
1830 - Gale Group | NCCO Corvey
... very low-grade metamorphosed rocks in six areas (Schwarzburg Anticline, Berga Anticline, Doberlug Syncline, North Saxon Anticline, ... all other areas. (2) The core of the Schwarzburg Anticline, which is overprinted by greenschist facies conditions ... the same area. (3) Cadomian sediments from the Schwarzburg Anticline show an input of younger felsic crust. ( ...
Tópico(s): Paleontology and Stratigraphy of Fossils
2002 - Elsevier BV | Tectonophysics
W. Dittenberger, Dr. H. Toepfer, Ed. Damköhler, Professor S. Lüttich, Dr. H. Toepfer, Dr. O. Koepert,
... Thüringen 1894, Die Wald-Und Wasserverhältnisse Des Fürstentums Schwarzburg-Sondershausen Nach Offiziellen Angaben, Privaten Mitteilungen Und Eigenen ...
1895 - Gale Group | NCCO-STM 1of2
Ulf Linnemann, Axel Gerdes, Mandy Hofmann, Linda Marko,
... zircon of Neoproterozoic to Fortunian siliciclastics from the Schwarzburg Antiform in the Saxo-Thuringian Zone (NE Bohemian ...
Tópico(s): Geochemistry and Geologic Mapping
2013 - Elsevier BV | Precambrian Research
S. P. T. PRIDEAUX, , W. NORTON, G. WHITE, JOHN C. MEDD., FRANCIS J. S. HOPWOOD, , MARLBOROUGH., CHARLES CAMPBELL, , LLOYD WISE, , GUY H. SCHOLEFIELD, , JOHN C. R. COLOMB., By ERNEST LAW., BARRISTER-AT-LAW., COUNTESS SOPHIA TOLSTOY., FREDK. SHERLOCK.,
... Exeter., Mr. William Cheariton., Prince Karl Günther Of Schwarzburg., Mr. E. D. Carver., Obituary, Sir Mathew Gosset, ...
1909 - Gale Group | TDA
B. Troesken, F. Willig, Klaus Schwarzburg, A. Ehert, Mark T. Spitler,
... 300 and 5 KB. Troesken, F. Willig, K. Schwarzburg, A. Ehert, and M. SpitlerCite this: J. Phys. ...
Tópico(s): nanoparticles nucleation surface interactions
1995 - American Chemical Society | The Journal of Physical Chemistry
... mm x 21 mm. Photographer: Anonymous. Elizabeth of Schwarzburg Rudolstadt Born Octr. 1st 1833.
0000 - Gale Group | NCCO Photography
... flysch stage (Lower Carboniferous) is nearly completely developed (Schwarzburg anticline). In contrast, Neoproterozoic sedimentation at least in ... terranes and of the autochthonous Proterozoic of the Schwarzburg anticline enclosed in the Palaeozoic of the Saxo- ...
Tópico(s): High-pressure geophysics and materials
1995 - Elsevier BV | Precambrian Research
... Inquests Colonel Home Purves, Count Frederick Gunther of Schwarzburg-Rudolstadt Births, Marriages, and Deaths Multiple Classified Advertising ...
1867 - Gale Group | Sunday Times HA GDA
J. Mahrt, F. Willig, W. Storck, D. Weiß, R. Kietzmann, Klaus Schwarzburg, Barbara J. Tufts, B. Troesken,
... Willig, W. Storck, D. Weiss, R. Kietzmann, K. Schwarzburg, B. Tufts, and B. TroeskenCite this: J. Phys. ...
Tópico(s): Lipid Membrane Structure and Behavior
1994 - American Chemical Society | The Journal of Physical Chemistry
Book.
1844 - Gale Group | NCCO Corvey
... and likely a different effect. Aemilie Juliane von Schwarzburg-Rudolstadt (1637-1706) replaced the female persona men ...
Tópico(s): Historical Studies on Reproduction, Gender, Health, and Societal Changes
2003 - Binghamton University | Journal of women's history
Hannes Hempel, Tom J. Savenjie, Martin Stolterfoht, Jens Neu, Michele Failla, Vaisakh C. Paingad, P. Kužel, Edwin J. Heilweil, Jacob A. Spies, Markus Schleuning, Jiashang Zhao, Dennis Friedrich, Klaus Schwarzburg, Laurens D. A. Siebbeles, Patrick Dörflinger, Vladimir Dyakonov, Ryuzi Katoh, Min Ji Hong, John G. Labram, Maurizio Monti, Edward Butler‐Caddle, James Lloyd‐Hughes, Mohammad M. Taheri, Jason B. Baxter, Timothy J. Magnanelli, Simon Luo, Joseph M. Cardon, Shane Ardo, Thomas Unold,
Abstract Mobilities and lifetimes of photogenerated charge carriers are core properties of photovoltaic materials and can both be characterized by contactless terahertz or microwave measurements. Here, the expertise from fifteen laboratories is combined to quantitatively model the current‐voltage characteristics of a solar cell from such measurements. To this end, the impact of measurement conditions, alternate interpretations, and experimental inter‐laboratory variations are discussed using a (Cs, ...
Tópico(s): Chalcogenide Semiconductor Thin Films
2022 - Wiley | Advanced Energy Materials
Petr Kraft, Ulf Linnemann, Michal Mergl, Jana Bruthansová, Lukáš Laibl, Gerd Geyer,
... together with relics of another preserved in the Schwarzburg Anticline, represents the main exposures in the Bohemian ...
Tópico(s): Paleontology and Stratigraphy of Fossils
2022 - Geological Society of London | Geological Society London Special Publications
Sebastián Caicedo‐Dávila, René Gunder, J.A. Marquez, S. Levcenko, Klaus Schwarzburg, Thomas Unold, Daniel Abou‐Ras,
The phase mixture CsPb2Br5/CsPbBr3 has raised interest as a promising material system for light emission, light detection, and even for photovoltaic devices owing to its high luminescence yield and improved device performance when compared with pure CsPbBr3 devices. Given that CsPb2Br5 and CsPbBr3 exhibit similar formation enthalpies, thermal treatment can induce phase transformations between them. The influence of that transformation on the optoelectronic properties is still unclear. In the present ...
Tópico(s): Luminescence Properties of Advanced Materials
2020 - American Chemical Society | The Journal of Physical Chemistry C
Judith Benz-Schwarzburg, Susana Monsó, Ludwig Huber,
Humans interact with animals in numerous ways and on numerous levels. We are indeed living in an “animal”s world,’ in the sense that our lives are very much intertwined with the lives of animals. This also means that animals, like those dogs we commonly refer to as our pets, are living in a “human’s world” in the sense that it is us, not them, who, to a large degree, define and manage the interactions we have with them. In this sense, the human-animal relationship is nothing we should romanticize: ...
Tópico(s): Psychology of Moral and Emotional Judgment
2020 - Frontiers Media | Frontiers in Psychology
Mario Borgwardt, Johannes Mahl, Friedrich Roth, Lukas Wenthaus, Felix Brauße, Monika Blum, Klaus Schwarzburg, Guiji Liu, Francesca M. Toma, Oliver Geßner,
Progress in the development of plasmon-enabled light-harvesting technologies requires a better understanding of their fundamental operating principles and current limitations. Here, we employ picosecond time-resolved X-ray photoemission spectroscopy to investigate photoinduced electron transfer in a plasmonic model system composed of 20 nm sized gold nanoparticles (NPs) attached to a nanoporous film of TiO2. The measurement provides direct, quantitative access to transient local charge distributions ...
Tópico(s): Advanced Photocatalysis Techniques
2020 - American Chemical Society | The Journal of Physical Chemistry Letters
Christian Nawroth, Jan Langbein, M. Coulon, Vivian Gabor, Susann Oesterwind, Judith Benz-Schwarzburg, Eberhard von Borell,
Farm animal welfare is a major concern for society and food production. To more accurately evaluate animal farming in general and to avoid exposing farm animals to poor welfare situations, it is necessary to understand not only their behavioural but also their cognitive needs and capacities. Thus, general knowledge of how farm animals perceive and interact with their environment is of major importance for a range of stakeholders, from citizens to politicians to cognitive ethologists to philosophers. ...
Tópico(s): Wildlife Ecology and Conservation
2019 - Frontiers Media | Frontiers in Veterinary Science
Mario Borgwardt, Stefan T. Omelchenko, Marco Favaro, Paul Plate, Christian Höhn, Daniel Abou‐Ras, Klaus Schwarzburg, Roel van de Krol, Harry A. Atwater, Nathan S. Lewis, Rainer Eichberger, Dennis Friedrich,
Abstract Cuprous oxide (Cu 2 O) is a promising material for solar-driven water splitting to produce hydrogen. However, the relatively small accessible photovoltage limits the development of efficient Cu 2 O based photocathodes. Here, femtosecond time-resolved two-photon photoemission spectroscopy has been used to probe the electronic structure and dynamics of photoexcited charge carriers at the Cu 2 O surface as well as the interface between Cu 2 O and a platinum (Pt) adlayer. By referencing ultrafast ...
Tópico(s): Electronic and Structural Properties of Oxides
2019 - Nature Portfolio | Nature Communications
Susana Monsó, Judith Benz-Schwarzburg, Annika Bremhorst,
It has been argued that some animals are moral subjects, that is, beings who are capable of behaving on the basis of moral motivations (Rowlands 2011, 2012, 2017). In this paper, we do not challenge this claim. Instead, we presuppose its plausibility in order to explore what ethical consequences follow from it. Using the capabilities approach (Nussbaum 2004, 2007), we argue that beings who are moral subjects are entitled to enjoy positive opportunities for the flourishing of their moral capabilities, ...
Tópico(s): Animal Behavior and Welfare Studies
2018 - Springer Science+Business Media | The Journal of Ethics
J.A. Marquez, Helena Stange, Charles J. Hages, Norbert Schaefer, S. Levcenko, Sergio Giraldo, Edgardo Saucedo, Klaus Schwarzburg, Daniel Abou‐Ras, Alex Redinger, Manuela Klaus, Christoph Genzel, Thomas Unold, Roland Mainz,
The selenization of metallic Cu–Zn–Sn–Ge precursors is a promising route for the fabrication of low-cost and efficient kesterite thin-film solar cells. Nowadays, efficiencies of kesterite solar cells are still below 13%. For Cu(In,Ga)Se2 solar cells, the formation of compositional gradients along the depth of the absorber layer has been demonstrated to be a key requirement for producing thin-film solar cells with conversion efficiencies above the 22% level. No clear understanding has been reached ...
Tópico(s): Copper-based nanomaterials and applications
2017 - American Chemical Society | Chemistry of Materials
Matthias M. May, David Lackner, Jens Ohlmann, Frank Dimroth, Roel van de Krol, Thomas Hannappel, Klaus Schwarzburg,
We discuss benchmarking considerations for multi-junction solar fuel absorbers and investigate the effects of spectral shaping by catalyst nanoparticles on design criteria.
Tópico(s): Perovskite Materials and Applications
2017 - Royal Society of Chemistry | Sustainable Energy & Fuels
Madelaine Leitsberger, Judith Benz-Schwarzburg, Herwig Grimm,
Tópico(s): Animal and Plant Science Education
2016 - Springer Science+Business Media | Journal of Agricultural and Environmental Ethics
Christian Tessarek, Stefanie Fladischer, C. Dieker, George Sarau, B. Hoffmann, Muhammad Y. Bashouti, Manuela Göbelt, Martin Heilmann, M. Lätzel, Eduard Butzen, S. Figge, A. Gust, Katja Höflich, Thorsten Feichtner, Matthias Büchele, Klaus Schwarzburg, Erdmann Spiecker, Silke Christiansen,
Vertically aligned hexagonal InN nanorods were grown mask-free by conventional metal–organic vapor phase epitaxy without any foreign catalyst. The In droplets on top of the nanorods indicate a self-catalytic vapor–liquid–solid growth mode. A systematic study on important growth parameters has been carried out for the optimization of nanorod morphology. The nanorod N-polarity, induced by high temperature nitridation of the sapphire substrate, is necessary to achieve vertical growth. Hydrogen, usually ...
Tópico(s): Nanowire Synthesis and Applications
2016 - American Chemical Society | Nano Letters
A. Abramowski, F. Aharonian, F. Ait Benkhali, A. G. Akhperjanian, E. O. Angüner, Michael Backes, S. Balenderan, A. Balzer, A. Barnacka, Y. Becherini, J. Becker Tjus, D. Berge, S. Bernhard, K. Bernlöhr, E. Birsin, J. Biteau, M. Böttcher, C. Boisson, J. Bolmont, P. Bordas, J. Bregeon, F. Brun, P. Brun, M. Bryan, T. Bulik, S. Carrigan, S. Casanova, P. M. Chadwick, N. Chakraborty, R. Chalmé-Calvet, R. C. G. Chaves, M. Chrétien, S. Colafrancesco, G. Cologna, J. M. Conrad, C. Couturier, Y. Cui, M. Dalton, I. D. Davids, B. Degrange, C. Deil, P. deWilt, A. Djannati-Ataı̈, W. Domainko, Axel Donath, L. O’C. Drury, G. Dubus, K. Dutson, J. Dyks, M. Dyrda, T. Edwards, K. Egberts, P. Eger, P. Espigat, C. Farnier, S. Fegan, F. Feinstein, M. V. Fernandes, D. Fernández, A. Fiaßon, G. Fontaine, A. Förster, M. Füßling, S. Gabici, M. Gajdus, Y. A. Gallant, T. Garrigoux, G. Giavitto, B. Giebels, J. F. Glicenstein, D. Gottschall, M.-H. Grondin, M. Grudzińska, D. Hadsch, S. Häffner, Joachim Hahn, J. Harris, G. Heinzelmann, G. Henri, G. Hermann, O. Hervet, Andreas Hillert, J. A. Hinton, W. Hofmann, P. Hofverberg, M. Holler, D. Horns, A. Ivascenko, A. Jachołkowska, C. Jahn, M. Jamrozy, M. Janiak, F. Jankowsky, I. Jung, M. A. Kastendieck, K. Katarzyński, U. Katz, S. Kaufmann, B. Khélifi, M. Kieffer, S. Klepser, D. Klochkov, W. Kluźniak, D. Kolitzus, Nu. Komin, K. Kosack, S. Krakau, F. Krayzel, P. P. Krüger, H. Laffon, G. Lamanna, J. Lefaucheur, V. Lefranc, A. Lemière, M. Lemoine‐Goumard, J.-P. Lenain, T. Lohse, A. Lopatin, C.-C. Lu, V. Marandon, A. Marcowith, R. Marx, G. Maurin, Nigel Maxted, M. Mayer, T. J. L. McComb, J. Méhault, P. J. Meintjes, U. Menzler, M. Meyer, Alison Mitchell, R. Moderski, M. Mohamed, K. Morå, E. Moulin, T. Murach, M. de Naurois, J. Niemiec, S. J. Nolan, L. Oakes, Hirokazu Odaka, S. Ohm, B. Opitz, M. Ostrowski, R. Mirzoyan, M. Panter, R. D. Parsons, M. Paz Arribas, N. W. Pekeur, G. Pelletier, J. Pérez, P.‐O. Petrucci, B. Peyaud, S. Pita, H. Poon, G. Pühlhofer, M. Punch, A. Quirrenbach, S. Raab, I. Reichardt, A. Reimer, O. Reimer, M. Renaud, R. de los Reyes, Frank Rieger, L. Rob, C. Romoli, S. Rosier-Lees, Gavin Rowell, B. Rudak, C. B. Rulten, V. Sahakian, D. Salek, D. A. Sanchez⋆, A. Santangelo, R. Schlickeiser, F. Schüßler, A. Schulz, U. Schwanke, S. Schwarzburg, S. Schwemmer, H. Sol, F. Spanier, G. Spengler, F. Spies, Ł. Stawarz, R. Steenkamp, C. Stegmann, F. Stinzing, K. Stycz, I. Sushch, J.‐P. Tavernet, T. Tavernier, A. M. Taylor, R. Terrier, M. Tluczykont, C. Trichard, K. Valerius, C. van Eldik, B. van Soelen, G. Vasileiadis, J. Veh, C. Venter, A. Viana, P. Vincent, Jacco Vink, H. J. Völk, F. Volpe, M. Vorster, Thomas Vuillaume, P. Wagner, R. M. Wagner, M. J. Ward, M. Weidinger, Q. Weitzel, R. White, A. Wierzcholska, P. Willmann, A. Wörnlein, D. Wouters, R. Yang, V. Zabalza, D. Zaborov, M. Zacharias, A. A. Zdziarski, A. Zech, H.-S. Zechlin,
Very high energy (VHE, E > 100 GeV) γ-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 γ-ray flaring being caused by the injection of ...
Tópico(s): Gamma-ray bursts and supernovae
2015 - IOP Publishing | The Astrophysical Journal
A. Abramowski, F. Aharonian, F. Ait Benkhali, A. G. Akhperjanian, E. O. Angüner, Michael Backes, S. Balenderan, A. Balzer, A. Barnacka, Y. Becherini, J. Becker Tjus, D. Berge, S. Bernhard, K. Bernlöhr, E. Birsin, J. Biteau, M. Böttcher, C. Boisson, J. Bolmont, P. Bordas, J. Bregeon, F. Brun, P. Brun, M. Bryan, T. Bulik, S. Carrigan, S. Casanova, P. M. Chadwick, N. Chakraborty, R. Chalmé-Calvet, R. C. G. Chaves, M. Chrétien, S. Colafrancesco, G. Cologna, J. M. Conrad, C. Couturier, Y. Cui, I. D. Davids, B. Degrange, C. Deil, P. deWilt, A. Djannati-Ataï, W. Domainko, Axel Donath, L. O’C. Drury, G. Dubus, K. Dutson, J. Dyks, M. Dyrda, T. Edwards, K. Egberts, P. Eger, P. Espigat, C. Farnier, S. Fegan, F. Feinstein, M. V. Fernandes, D. Fernández, A. Fiaßon, G. Fontaine, A. Förster, M. Füßling, S. Gabici, M. Gajdus, Y. A. Gallant, T. Garrigoux, G. Giavitto, B. Giebels, J. F. Glicenstein, D. Gottschall, M.-H. Grondin, M. Grudzińska, D. Hadasch, S. Häffner, J. Hahn, J. Harris, G. Heinzelmann, G. Henri, G. Hermann, O. Hervet, Andreas Hillert, J. A. Hinton, W. Hofmann, P. Hofverberg, M. Holler, D. Horns, A. Ivascenko, A. Jachołkowska, C. Jahn, M. Jamrozy, M. Janiak, F. Jankowsky, I. Jung-Richardt, M. A. Kastendieck, K. Katarzyński, U. Katz, S. Kaufmann, B. Khélifi, M. Kieffer, S. Klepser, D. Klochkov, W. Kluźniak, D. Kolitzus, Nu. Komin, K. Kosack, S. Krakau, F. Krayzel, P. P. Krüger, H. Laffon, G. Lamanna, J. Lefaucheur, V. Lefranc, A. Lemière, M. Lemoine‐Goumard, J.-P. Lenain, T. Lohse, A. Lopatin, C. Lu, V. Marandon, A. Marcowith, R. Marx, G. Maurin, Nigel Maxted, M. Mayer, T. J. L. McComb, J. Méhault, P. J. Meintjes, U. Menzler, M. Meyer, Alison Mitchell, R. Moderski, M. Mohamed, K. Morå, E. Moulin, T. Murach, M. de Naurois, J. Niemiec, S. J. Nolan, L. Oakes, Hirokazu Odaka, S. Ohm, B. Opitz, M. Ostrowski, R. Mirzoyan, M. Panter, R. D. Parsons, M. Paz Arribas, N. W. Pekeur, G. Pelletier, P-O Petrucci, B. Peyaud, S. Pita, H. Poon, G. Pühlhofer, M. Punch, A. Quirrenbach, S. Raab, I. Reichardt, A. Reimer, O. Reimer, M. Renaud, R. de los Reyes, Frank Rieger, C. Romoli, S. Rosier-Lees, Gavin Rowell, B. Rudak, C. B. Rulten, V. Sahakian, D. Salek, D. A. Sanchez⋆, A. Santangelo, R. Schlickeiser, F. Schüßler, A. Schulz, U. Schwanke, S. Schwarzburg, S. Schwemmer, H. Sol, F. Spanier, G. Spengler, F. Spies, Ł. Stawarz, R. Steenkamp, C. Stegmann, F. Stinzing, K. Stycz, I. Sushch, J.‐P. Tavernet, T. Tavernier, A. M. Taylor, R. Terrier, M. Tluczykont, C. Trichard, K. Valerius, C. van Eldik, B. van Soelen, G. Vasileiadis, J. Veh, C. Venter, A. Viana, P. Vincent, Jacco Vink, H. J. Völk, F. Volpe, M. Vorster, Thomas Vuillaume, S. J. Wagner, P. Wagner, R. M. Wagner, M. J. Ward, M. Weidinger, Q. Weitzel, R. White, A. Wierzcholska, P. Willmann, A. Wörnlein, D. Wouters, R. Yang, V. Zabalza, D. Zaborov, M. Zacharias, A. A. Zdziarski, A. Zech, H.-S. Zechlin,
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 ∼9 h of on-off observations. Upper limits on the velocity averaged cross section, ⟨σv⟩, for the annihilation of dark matter particles with masses in the range of ∼300 GeV to ∼10 TeV are derived. In contrast to previous constraints derived from ...
Tópico(s): Cosmology and Gravitation Theories
2015 - American Physical Society | Physical Review Letters
A. Abramowski, F. Aharonian, F. Ait Benkhali, A. G. Akhperjanian, E. O. Angüner, Michael Backes, S. Balenderan, A. Balzer, A. Barnacka, Y. Becherini, J. Becker Tjus, D. Berge, S. Bernhard, K. Bernlöhr, E. Birsin, J. Biteau, M. Böttcher, C. Boisson, J. Bolmont, P. Bordas, J. Bregeon, F. Brun, P. Brun, M. Bryan, T. Bulik, S. Carrigan, S. Casanova, P. M. Chadwick, N. Chakraborty, R. Chalmé-Calvet, R. C. G. Chaves, M. Chrétien, S. Colafrancesco, G. Cologna, J. M. Conrad, C. Couturier, Y. Cui, I. D. Davids, B. Degrange, C. Deil, P. deWilt, A. Djannati-Ataï, W. Domainko, Axel Donath, L. O’C. Drury, G. Dubus, K. Dutson, J. Dyks, M. Dyrda, T. Edwards, K. Egberts, P. Eger, P. Espigat, C. Farnier, S. Fegan, F. Feinstein, M. V. Fernandes, D. Fernández, A. Fiasson, G. Fontaine, A. Förster, M. Füßling, S. Gabici, M. Gajdus, Y. A. Gallant, T. Garrigoux, G. Giavitto, B. Giebels, J. F. Glicenstein, D. Gottschall, M.-H. Grondin, M. Grudzińska, D. Hadasch, S. Häffner, Joachim Hahn, J. Harris, G. Heinzelmann, G. Henri, G. Hermann, O. Hervet, Andreas Hillert, J. A. Hinton, W. Hofmann, P. Hofverberg, M. Holler, D. Horns, A. Ivascenko, A. Jacholkowska, C. Jahn, M. Jamrozy, M. Janiak, F. Jankowsky, I. Jung-Richardt, M. A. Kastendieck, K. Katarzyński, U. Katz, S. Kaufmann, B. Khélifi, M. Kieffer, S. Klepser, D. Klochkov, W. Kluźniak, D. Kolitzus, Nu. Komin, K. Kosack, S. Krakau, F. Krayzel, P. P. Krüger, H. Laffon, G. Lamanna, J. Lefaucheur, V. Lefranc, A. Lemière, M. Lemoine-Goumard, J.-P. Lenain, T. Lohse, A. Lopatin, C.-C. Lu, V. Marandon, A. Marcowith, R. Marx, G. Maurin, Nigel Maxted, Martin G. F. Mayer, T. J. L. McComb, J. Méhault, P. J. Meintjes, U. Menzler, M. Meyer, Alison Mitchell, R. Moderski, M. Mohamed, K. S. Caballero‐Mora, E. Moulin, T. Murach, M. de Naurois, J. Niemiec, S. J. Nolan, L. Oakes, Hirokazu Odaka, S. Ohm, B. Opitz, M. Ostrowski, R. Mirzoyan, M. Panter, R. D. Parsons, M. Paz Arribas, N. W. Pekeur, G. Pelletier, P.‐O. Petrucci, B. Peyaud, S. Pita, H. Poon, G. Pühlhofer, M. Punch, A. Quirrenbach, S. Raab, I. Reichardt, A. Reimer, O. Reimer, M. Renaud, R. de los Reyes, Frank Rieger, C. Romoli, S. Rosier-Lees, Gavin Rowell, B. Rudak, C. B. Rulten, V. Sahakian, D. Salek, D. A. Sanchez⋆, A. Santangelo, R. Schlickeiser, F. Schüßler, A. Schulz, U. Schwanke, S. Schwarzburg, S. Schwemmer, H. Sol, F. Spanier, G. Spengler, F. Spies, Ł. Stawarz, R. Steenkamp, C. Stegmann, F. Stinzing, K. Stycz, I. Sushch, J.‐P. Tavernet, T. Tavernier, A. M. Taylor, R. Terrier, M. Tluczykont, C. Trichard, K. Valerius, C. van Eldik, B. van Soelen, G. Vasileiadis, J. Veh, C. Venter, A. Viana, P. Vincent, Jacco Vink, H. J. Völk, F. Volpe, M. Vorster, Thomas Vuillaume, S. J. Wagner, P. Wagner, R. M. Wagner, M. J. Ward, M. Weidinger, Q. Weitzel, R. White, A. Wierzcholska, P. Willmann, A. Wörnlein, D. Wouters, R. Yang, V. Zabalza, D. Zaborov, M. Zacharias, A. A. Zdziarski, A. Zech, H.-S. Zechlin,
Puppis A is an interesting ~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 an 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 ...
Tópico(s): Dark Matter and Cosmic Phenomena
2015 - EDP Sciences | Astronomy and Astrophysics
A. Abramowski, F. Aharonian, F. Ait Benkhali, A. G. Akhperjanian, E. O. Angüner, Michael Backes, S. Balenderan, A. Balzer, A. Barnacka, Y. Becherini, J. Becker Tjus, D. Berge, S. Bernhard, K. Bernlöhr, E. Birsin, J. Biteau, M. Böttcher, C. Boisson, J. Bolmont, P. Bordas, J. Bregeon, F. Brun, P. Brun, M. Bryan, T. Bulik, S. Carrigan, S. Casanova, P. M. Chadwick, Nachiketa Chakraborty, R. Chalme-Calvet, R. C. G. Chaves, M. Chrétien, S. Colafrancesco, G. Cologna, J. Conrad, C. Couturier, Y. Cui, M. Dalton, I. D. Davids, B. Degrange, Christoph Deil, Phoebe de Wilt, A. Djannati-Ataï, Wilfried Domainko, Axel Donath, L. O’C. Drury, G. Dubus, K. Dutson, J. Dyks, M. Dyrda, T. Edwards, K. Egberts, Peter Eger, P. Espigat, C. Farnier, S. Fegan, F. Feinstein, M. V. Fernandes, D. Fernandez, A. Fiasson, G. Fontaine, Andreas Foerster, M. Füßling, S. Gabici, M. Gajdus, Y. A. Gallant, T. Garrigoux, G. Giavitto, B. Giebels, J. F. Glicenstein, D. Gottschall, M.-H. Grondin, M. Grudzińska, D. Hadasch, S. Häffner, Joachim Hahn, J. Harris, G. Heinzelmann, G. Henri, G. Hermann, O. Hervet, A. Hillert, J. A. Hinton, W. Hofmann, P. Hofverberg, M. Holler, D. Horns, A. Ivascenko, A. Jachołkowska, C. Jahn, M. Jamrozy, M. Janiak, F. Jankowsky, I. Jung, M. A. Kastendieck, K. Katarzyński, U. Katz, S. Kaufmann, B. Khélifi, M. Kieffer, S. Klepser, D. Klochkov, W. Kluźniak, D. Kolitzus, Nu. Komin, K. Kosack, S. Krakau, F. Krayzel, P. P. Krüger, H. Laffon, G. Lamanna, J. Lefaucheur, V. Lefranc, A. Lemière, M. Lemoine-Goumard, J.-P. Lenain, T. Lohse, A. Lopatin, Chia-Chun Lu, V. Marandon, A. Marcowith, R. Marx, G. Maurin, Nigel Maxted, Martin G. F. Mayer, T. J. L. McComb, J. Méhault, P. J. Meintjes, U. Menzler, M. Meyer, A. Mitchell, R. Moderski, M. Mohamed, K. Morå, E. Moulin, T. Murach, M. de Naurois, J. Niemiec, S. J. Nolan, L. Oakes, H. Odaka, S. Ohm, B. Opitz, M. Ostrowski, R. Mirzoyan, M. Panter, R. D. Parsons, M. Paz Arribas, N. W. Pekeur, G. Pelletier, J. Perez, P.-O. Petrucci, B. Peyaud, S. Pita, H. Poon, G. Pühlhofer, M. Punch, A. Quirrenbach, S. Raab, I. Reichardt, A. Reimer, O. Reimer, M. Renaud, R. de los Reyes, Frank Rieger, L. Rob, C. Romoli, S. Rosier-Lees, Gavin Rowell, B. Rudak, C. B. Rulten, D. Salek, D. A. Sanchez⋆, A. Santangelo, R. Schlickeiser, F. Schüßler, A. Schulz, U. Schwanke, S. Schwarzburg, S. Schwemmer, H. Sol, F. Spanier, G. Spengler, F. Spies, Ł. Stawarz, R. Steenkamp, C. Stegmann, F. Stinzing, K. Stycz, I. Sushch, J.‐P. Tavernet, T. Tavernier, A. M. Taylor, R. Terrier, M. Tluczykont, C. Trichard, K. Valerius, C. van Eldik, B. van Soelen, G. Vasileiadis, J. Veh, C. Venter, A. Viana, P. Vincent, Jacco Vink, H. J. Voêlk, Francesca Volpe, M. Vorster, T. Vuillaume, S. J. Wagner, P. Wagner, R. M. Wagner, M. J. Ward, M. Weidinger, Q. Weitzel, R. White, A. Wierzcholska, P. Willmann, A. Wörnlein, D. Wouters, Ruizhi Yang, V. Zabalza, D. Zaborov, M. Zacharias, A. A. Zdziarski, A. Zech, H.-S. Zechlin,
A light on the origin of cosmic rays There's a new lab for studying the origins of cosmic rays: our neighbor galaxy, the Large Magellanic Cloud. Astronomers are now making progress on this topic by examining the gamma rays that are produced when cosmic rays interact with gas or lower-energy photons. The H.E.S.S. Collaboration has detected three sources of gamma rays in a variety of forms in the galactic satellite to the Milky Way. The sources include the pulsar wind nebula of N 157B, the supernova ...
Tópico(s): Neutrino Physics Research
2015 - American Association for the Advancement of Science | Science
H. E. S. S. Collaboration, A. Abramowski, Felix Aharonian, F. Ait Benkhali, A. G. Akhperjanian, E. Angüner, G. Anton, S. Balenderan, A. Balzer, A. Barnacka, Y. Becherini, J. Becker Tjus, K. Bernlöhr, E. Birsin, E. Bissaldi, J. Biteau, M. Böttcher, C. Boisson, J. Bolmont, P. Bordas, J. Brucker, F. Brun, P. Brun, T. Bulik, S. Carrigan, S. Casanova, M. Cerruti, P. M. Chadwick, R. Chalme-Calvet, R. C. G. Chaves, A. Cheesebrough, M. Chrétien, S. Colafrancesco, G. Cologna, J. Conrad, C. Couturier, Y. Cui, M. Dalton, M. K. Daniel, I. D. Davids, B. Degrange, C. Deil, P. deWilt, H. J. Dickinson, A. Djannati-Ataï, W. Domainko, L. O’C. Drury, G. Dubus, K. Dutson, J. Dyks, M. Dyrda, T. Edwards, K. Egberts, P. Eger, P. Espigat, C. Farnier, S. Fegan, F. Feinstein, M. V. Fernandes, D. Fernandez, A. Fiasson, G. Fontaine, A. Förster, M. Füßling, M. Gajdus, Y. A. Gallant, T. Garrigoux, G. Giavitto, B. Giebels, J. F. Glicenstein, M. -H. Grondin, M. Grudzińska, S. Häffner, J. Hahn, J. Harris, G. Heinzelmann, G. Henri, G. Hermann, O. Hervet, A. Hillert, J. A. Hinton, W. Hofmann, P. Hofverberg, M. Holler, D. Horns, A. Jacholkowska, C. Jahn, M. Jamrozy, M. Janiak, F. Jankowsky, I. Jung, M. A. Kastendieck, K. Katarzyński, U. Katz, S. Kaufmann, B. Khélifi, M. Kieffer, S. Klepser, D. Klochkov, W. Kluźniak, T. Kneiske, D. Kolitzus, Nu. Komin, K. Kosack, S. Krakau, F. Krayzel, P. P. Krüger, H. Laffon, G. Lamanna, J. Lefaucheur, A. Lemière, M. Lemoine-Goumard, J.-P. Lenain, D. Lennarz, T. Lohse, A. Lopatin, C.-C. Lu, V. Marandon, A. Marcowith, R. Marx, G. Maurin, Nigel Maxted, M. Mayer, T. J. L. McComb, J. Méhault, P. J. Meintjes, U. Menzler, M. Meyer, R. Moderski, M. Mohamed, E. Moulin, T. Murach, C. L. Naumann, M. de Naurois, J. Niemiec, S. J. Nolan, L. Oakes, S. Ohm, E. de Oña Wilhelmi, B. Opitz, M. Ostrowski, R. Mirzoyan, M. Panter, R. D. Parsons, M. Paz Arribas, N. W. Pekeur, G. Pelletier, J. Perez, P. -O. Petrucci, B. Peyaud, S. Pita, H. Poon, G. Pühlhofer, M. Punch, A. Quirrenbach, S. Raab, M. Raue, A. Reimer, O. Reimer, M. Renaud, R. de los Reyes, Frank Rieger, L. Rob, C. Romoli, S. Rosier-Lees, Gavin Rowell, B. Rudak, C. B. Rulten, V. Sahakian, D. A. Sanchez⋆, A. Santangelo, R. Schlickeiser, F. Schüßler, A. Schulz, U. Schwanke, S. Schwarzburg, S. Schwemmer, H. Sol, G. Spengler, F. Spies, Ł. Stawarz, R. Steenkamp, C. Stegmann, F. Stinzing, K. Stycz, I. Sushch, A. Szostek, J. -P. Tavernet, T. Tavernier, A. M. Taylor, R. Terrier, M. Tluczykont, C. Trichard, K. Valerius, C. van Eldik, Brian van Soelen, G. Vasileiadis, C. Venter, A. Viana, P. Vincent, H. J. Völk, Francesca Volpe, M. Vorster, T. Vuillaume, S. J. Wagner, P. Wagner, M. J. Ward, M. Weidinger, Q. Weitzel, R. White, A. Wierzcholska, P. Willmann, A. Wörnlein, D. Wouters, V. Zabalza, M. Zacharias, A. Zajczyk, A. A. Zdziarski, A. Zech, H.-S. Zechlin,
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) γ-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 ...
Tópico(s): Neutrino Physics Research
2014 - Oxford University Press | Monthly Notices of the Royal Astronomical Society