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description Publicationkeyboard_double_arrow_right Article , Preprint 2023Embargo end date: 01 Jan 2023 France, Czech Republic, Italy, France, Germany, Spain, France, Germany, Spain, France, France, Czech RepublicPublisher:American Astronomical Society Funded by:MIUR, EC | CTA-PP, EC | ESCAPE +5 projectsMIUR ,EC| CTA-PP ,EC| ESCAPE ,EC| PROBIST ,EC| PREBIST ,DFG ,EC| CTA-DEV ,EC| INFIERIAbe, H.; Abe, K.; Artero, M.; Hackfeld, J.; Hadasch, D.; Hahn, A.; Hashiyama, K.; Hassan, T.; Hayashi, K.; Heckmann, L.; Heller, M.; Herrera Llorente, J.; Hirotani, K.; Asano, K.; Hoffmann, D.; Horns, D.; Houles, J.; Hrabovsky, M.; Hrupec, D.; Hui, D.; Hütten, M.; Iarlori, M.; Imazawa, R.; Inada, T.; Aubert, P.; Inome, Y.; Ioka, K.; Iori, M.; Ishio, K.; Iwamura, Y.; Jacquemont, M.; Martinez, I. Jimenez; Jurysek, J.; Kagaya, M.; Karas, V.; Baktash, A.; Katagiri, H.; Kataoka, J.; Kerszberg, D.; Kobayashi, Y.; Kong, A.; Kubo, H.; Kushida, J.; Lainez, M.; Lamanna, G.; Lamastra, A.; Bamba, A.; Le Flour, T.; Linhoff, M.; Longo, F.; López-Coto, R.; López-Moya, M.; López-Oramas, A.; Loporchio, S.; Lorini, A.; Luque-Escamilla, P. L.; Majumdar, P.; Larriva, A. Baquero; Makariev, M.; Mandat, D.; Manganaro, M.; Manicò, G.; Mannheim, K.; Mariotti, M.; Marquez, P.; Marsella, G.; Martí, J.; Martinez, O.; Baroncelli, L.; Martínez, G.; Martínez, M.; Marusevec, P.; Mas-Aguilar, A.; Maurin, G.; Mazin, D.; Guillen, E. Mestre; Micanovic, S.; Miceli, D.; Miener, T.; de Almeida, U. Barres; Miranda, J. M.; Mirzoyan, R.; Mizuno, T.; Gonzalez, M. Molero; Molina, E.; Montaruli, T.; Monteiro, I.; Moralejo, A.; Morcuende, D.; Morselli, A.; Barrio, J. A.; Mrakovcic, K.; Murase, K.; Nagai, A.; Nagataki, S.; Nakamori, T.; Nickel, L.; Nievas, M.; Nishijima, K.; Noda, K.; Nosek, D.; Batkovic, I.; Nozaki, S.; Ohishi, M.; Ohtani, Y.; Oka, T.; Okazaki, N.; Okumura, A.; Orito, R.; Otero-Santos, J.; Palatiello, M.; Paneque, D.; Abe, S.; Baxter, J.; Pantaleo, F. R.; Paoletti, R.; Paredes, J. M.; Pech, M.; Pecimotika, M.; Peresano, M.; Pérez, A.; Pietropaolo, E.; Pirola, G.; Plard, C.; Becerra González, J.; Podobnik, F.; Poireau, V.; Polo, M.; Pons, E.; Prandini, E.; Prast, J.; Principe, G.; Priyadarshi, C.; Prouza, M.; Rando, R.; Bernardini, E.; Rhode, W.; Ribó, M.; Rizi, V.; Fernandez, G. Rodriguez; Ruiz, J. E.; Saito, T.; Sakurai, S.; Sanchez, D. A.; Šarić, T.; Sato, Y.; Bernardos, M. I.; Saturni, F. G.; Schleicher, B.; Schmuckermaier, F.; Schubert, J. L.; Schussler, F.; Schweizer, T.; Seglar Arroyo, M.; Silvia, R.; Sitarek, J.; Sliusar, V.; Medrano, J. Bernete; Spolon, A.; Strišković, J.; Strzys, M.; Suda, Y.; Sunada, Y.; Tajima, H.; Takahashi, H.; Takahashi, M.; Takata, J.; Takeishi, R.; Berti, A.; Tam, P. H. T.; Tanaka, S. J.; Tateishi, D.; Tejedor, L. A.; Temnikov, P.; Terada, Y.; Terauchi, K.; Terzic, T.; Teshima, M.; Tluczykont, M.; Bhattacharjee, P.; Tokanai, F.; Torres, D. F.; Travnicek, P.; Truzzi, S.; Tutone, A.; Uhlrich, G.; Vacula, M.; Vallania, P.; van Scherpenberg, J.; Vázquez Acosta, M.; Biederbeck, N.; Verguilov, V.; Viale, I.; Vigliano, A.; Vigorito, C. F.; Vitale, V.; Voutsinas, G.; Vovk, I.; Vuillaume, T.; Walter, R.;Abstract The Cherenkov Telescope Array (CTA) is a next-generation ground-based observatory for gamma-ray astronomy at very high energies. The Large-Sized Telescope prototype (LST-1) is located at the CTA-North site, on the Canary Island of La Palma. LSTs are designed to provide optimal performance in the lowest part of the energy range covered by CTA, down to ≃20 GeV. LST-1 started performing astronomical observations in 2019 November, during its commissioning phase, and it has been taking data ever since. We present the first LST-1 observations of the Crab Nebula, the standard candle of very-high-energy gamma-ray astronomy, and use them, together with simulations, to assess the performance of the telescope. LST-1 has reached the expected performance during its commissioning period—only a minor adjustment of the preexisting simulations was needed to match the telescope’s behavior. The energy threshold at trigger level is around 20 GeV, rising to ≃30 GeV after data analysis. Performance parameters depend strongly on energy, and on the strength of the gamma-ray selection cuts in the analysis: angular resolution ranges from 0.°12–0.°40, and energy resolution from 15%–50%. Flux sensitivity is around 1.1% of the Crab Nebula flux above 250 GeV for a 50 hr observation (12% for 30 minutes). The spectral energy distribution (in the 0.03–30 TeV range) and the light curve obtained for the Crab Nebula agree with previous measurements, considering statistical and systematic uncertainties. A clear periodic signal is also detected from the pulsar at the center of the Nebula.
Archivio istituziona... arrow_drop_down Archivio istituzionale della ricerca - Università degli Studi di UdineArticle . 2023License: CC BYRecolector de Ciencia Abierta, RECOLECTAArticle . 2023 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARepository of the Czech Academy of SciencesArticle . 2023Data sources: Repository of the Czech Academy of SciencesDiposit Digital de la Universitat de BarcelonaArticle . 2023Data sources: Diposit Digital de la Universitat de BarcelonaIRIS - Università degli Studi di CataniaArticle . 2023Data sources: IRIS - Università degli Studi di Cataniahttps://dx.doi.org/10.48550/ar...Article . 2023License: arXiv Non-Exclusive DistributionData sources: DataciteThe Astrophysical JournalArticle . 2023 . Peer-reviewedData sources: European Union Open Data PortalUniversité Savoie Mont Blanc: HALArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ace89d&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 16 citations 16 popularity Top 10% influence Top 10% impulse Top 10% 
Powered by BIP!visibility 57visibility views 57 download downloads 92 Powered by
more_vert Archivio istituziona... arrow_drop_down Archivio istituzionale della ricerca - Università degli Studi di UdineArticle . 2023License: CC BYRecolector de Ciencia Abierta, RECOLECTAArticle . 2023 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARepository of the Czech Academy of SciencesArticle . 2023Data sources: Repository of the Czech Academy of SciencesDiposit Digital de la Universitat de BarcelonaArticle . 2023Data sources: Diposit Digital de la Universitat de BarcelonaIRIS - Università degli Studi di CataniaArticle . 2023Data sources: IRIS - Università degli Studi di Cataniahttps://dx.doi.org/10.48550/ar...Article . 2023License: arXiv Non-Exclusive DistributionData sources: DataciteThe Astrophysical JournalArticle . 2023 . Peer-reviewedData sources: European Union Open Data PortalUniversité Savoie Mont Blanc: HALArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ace89d&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Journal 2021Embargo end date: 01 Jan 2021 Australia, France, France, France, Germany, Australia, France, France, Poland, France, France, Italy, France, France, France, Netherlands, Germany, France, GermanyPublisher:American Association for the Advancement of Science (AAAS) Publicly fundedS. Steinmassl; Sebastian Panny; Alexandre Marcowith; Regis Terrier; S. Sailer; Alison Mitchell; D. Jankowsky; Garret Cotter; Werner Hofmann; Michael Backes; Michael Backes; M. Spir-Jacob; Davit Zargaryan; Davit Zargaryan; Sabrina Casanova; Kleopas Shiningayamwe; A. Montanari; Jacek Niemiec; Dieter Horns; E. Kasai; Jonathan Mackey; C. Levy; J. Devin; Gavin Rowell; Jim Hinton; K. Nakashima; M. Seglar-Arroyo; R. Marx; R. Marx; L. Mohrmann; M. Renaud; Samuel Zouari; Jimmy N.S. Shapopi; Rafal Moderski; D. A. Sanchez; M. de Bony de Lavergne; F. Ait Benkhali; Christian Stegmann; C. Arcaro; A.M. Taylor; K. L. Page; Hassan Abdalla; D. Berge; S. Fegan; V. Joshi; Yasunobu Uchiyama; Łukasz Stawarz; B. Bi; Yvonne Becherini; E. O. Angüner; K. Kosack; Jim Davies; Thomas Murach; Sylvia Zhu; James E. M. Watson; T. Chand; Markus Holler; L. Dirson; J. Dyks; A. Priyana Noel; A. Zech; V. Barbosa Martins; L. Rinchiuso; A. S. Seyffert; S. Chandra; V. Marandon; Maria Haupt; V. Sahakian; Frank M. Rieger; Natalia Żywucka; Iryna Lypova; Hester Schutte; M. Panter; Axel Donath; P. A. Evans; Stefan Wagner; J. Zorn; Mohanraj Senniappan; F. Schüssler; Celine Armand; F. Werner; Tomasz Bulik; E. de Ona Wilhelmi; Hambeleleni Ndiyavala; A. Lemiere; M. Curyło; A. A. Zdziarski; N. Shafi; Victor Doroshenko; C. van Rensburg; Riaan Steenkamp; Felix Aharonian; Felix Aharonian; Felix Aharonian; Misao Sasaki; Johannes Veh; Monica Barnard; Stefan Klepser; R. Konno; Tom Armstrong; H. Prokoph; M. Tsirou; M. A. Kastendieck; M. Scalici; Andreas Specovius; M. Lemoine-Goumard; L. Olivera-Nieto; G. Fichet de Clairfontaine; Michal Ostrowski; H. Ashkar; Samuel Timothy Spencer; S. Raab; Roberta Zanin; H. Odaka; Włodek Kluźniak; Rachel Simoni; J.-P. Lenain; Andrea Santangelo; J.F. Glicenstein; B. Peyaud; J.-P. Ernenwein; G. Hermann; Clemens Hoischen; Domenico Tiziani; Felix Jankowsky; D. Malyshev; Carlo Romoli; F. Eichhorn; J. Schäfer; Pierre Brun; Christopher J. Duffy; A. Dmytriiev; Anna Barnacka; M. Zacharias; M. Zacharias; A. Djannati-Ataï; M. Büchele; V. Baghmanyan; Tadayuki Takahashi; Armelle Jardin-Blicq; Stefan Funk; D. Huber; A. Reimer; R. J. White; J. Bolmont; G. Vasileiadis; R. D. Parsons; G. Martí-Devesa; Dmitriy Kostunin; T. Tam; L. Giunti; L. Giunti; Elisabetta Bissaldi; Elisabetta Bissaldi; K. Egberts; Gianluca Giavitto; Jacco Vink; M. de Naurois; I. Jung-Richardt; Constantin Steppa; Konrad Bernlöhr; J. H. E. Thiersen; Bruno Khelifi; Paolo Marchegiani; M. Hörbe; E. Ruiz-Velasco; L. Oakes; Michael Kreter; Q. Piel; A. W. Chen; A. Wierzcholska; Dmitry Khangulyan; Lenka Tomankova; P. Reichherzer; Marek Jamrozy; G. Fontaine; Helene Sol; M.-H. Grondin; C. Moore; Yu Wun Wong; Isak Delberth Davids; G. Pühlhofer; S. Pita; B. Rudak; Kirsty Feijen; M. Bryan; P. Vincent; P. T. O'Brien; Nu. Komin; Christo Venter; Christoph Deil; Lei Sun; Mischa Breuhaus; Jhilik Majumdar; Joachim Hahn; T. Tavernier; A. Fiasson; D. A. Prokhorov; Michael Punch; Michael Punch;pmid: 34083487
An intrinsic gamma-ray burst afterglow Long gamma-ray bursts (GRBs) are emitted by relativistic jets generated during the collapse of a massive star in a distant galaxy. The GRB itself lasts only a few seconds but is followed by an afterglow that can persist for hours or days. The H.E.S.S. Collaboration observed the afterglow of GRB 190829A, a nearby long GRB. The proximity of this burst allowed it to be detected at tera–electron volt energies that would otherwise be absorbed in the intergalactic medium. By analyzing the spectrum and light curve at x-ray and gamma-ray wavelengths, the authors show that the afterglow cannot be explained by standard models. Science , abe8560, this issue p. 1081
Archivio Istituziona... arrow_drop_down Archivio Istituzionale della Ricerca - Politecnico di BariArticle . 2021Universiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2021Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2021Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: HALArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)The University of Adelaide: Digital LibraryArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)Eberhard Karls University Tübingen: Publication SystemArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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description Publicationkeyboard_double_arrow_right Article , Preprint 2023Embargo end date: 01 Jan 2023 France, Czech Republic, Italy, France, Germany, Spain, France, Germany, Spain, France, France, Czech RepublicPublisher:American Astronomical Society Funded by:MIUR, EC | CTA-PP, EC | ESCAPE +5 projectsMIUR ,EC| CTA-PP ,EC| ESCAPE ,EC| PROBIST ,EC| PREBIST ,DFG ,EC| CTA-DEV ,EC| INFIERIAbe, H.; Abe, K.; Artero, M.; Hackfeld, J.; Hadasch, D.; Hahn, A.; Hashiyama, K.; Hassan, T.; Hayashi, K.; Heckmann, L.; Heller, M.; Herrera Llorente, J.; Hirotani, K.; Asano, K.; Hoffmann, D.; Horns, D.; Houles, J.; Hrabovsky, M.; Hrupec, D.; Hui, D.; Hütten, M.; Iarlori, M.; Imazawa, R.; Inada, T.; Aubert, P.; Inome, Y.; Ioka, K.; Iori, M.; Ishio, K.; Iwamura, Y.; Jacquemont, M.; Martinez, I. Jimenez; Jurysek, J.; Kagaya, M.; Karas, V.; Baktash, A.; Katagiri, H.; Kataoka, J.; Kerszberg, D.; Kobayashi, Y.; Kong, A.; Kubo, H.; Kushida, J.; Lainez, M.; Lamanna, G.; Lamastra, A.; Bamba, A.; Le Flour, T.; Linhoff, M.; Longo, F.; López-Coto, R.; López-Moya, M.; López-Oramas, A.; Loporchio, S.; Lorini, A.; Luque-Escamilla, P. L.; Majumdar, P.; Larriva, A. Baquero; Makariev, M.; Mandat, D.; Manganaro, M.; Manicò, G.; Mannheim, K.; Mariotti, M.; Marquez, P.; Marsella, G.; Martí, J.; Martinez, O.; Baroncelli, L.; Martínez, G.; Martínez, M.; Marusevec, P.; Mas-Aguilar, A.; Maurin, G.; Mazin, D.; Guillen, E. Mestre; Micanovic, S.; Miceli, D.; Miener, T.; de Almeida, U. Barres; Miranda, J. M.; Mirzoyan, R.; Mizuno, T.; Gonzalez, M. Molero; Molina, E.; Montaruli, T.; Monteiro, I.; Moralejo, A.; Morcuende, D.; Morselli, A.; Barrio, J. A.; Mrakovcic, K.; Murase, K.; Nagai, A.; Nagataki, S.; Nakamori, T.; Nickel, L.; Nievas, M.; Nishijima, K.; Noda, K.; Nosek, D.; Batkovic, I.; Nozaki, S.; Ohishi, M.; Ohtani, Y.; Oka, T.; Okazaki, N.; Okumura, A.; Orito, R.; Otero-Santos, J.; Palatiello, M.; Paneque, D.; Abe, S.; Baxter, J.; Pantaleo, F. R.; Paoletti, R.; Paredes, J. M.; Pech, M.; Pecimotika, M.; Peresano, M.; Pérez, A.; Pietropaolo, E.; Pirola, G.; Plard, C.; Becerra González, J.; Podobnik, F.; Poireau, V.; Polo, M.; Pons, E.; Prandini, E.; Prast, J.; Principe, G.; Priyadarshi, C.; Prouza, M.; Rando, R.; Bernardini, E.; Rhode, W.; Ribó, M.; Rizi, V.; Fernandez, G. Rodriguez; Ruiz, J. E.; Saito, T.; Sakurai, S.; Sanchez, D. A.; Šarić, T.; Sato, Y.; Bernardos, M. I.; Saturni, F. G.; Schleicher, B.; Schmuckermaier, F.; Schubert, J. L.; Schussler, F.; Schweizer, T.; Seglar Arroyo, M.; Silvia, R.; Sitarek, J.; Sliusar, V.; Medrano, J. Bernete; Spolon, A.; Strišković, J.; Strzys, M.; Suda, Y.; Sunada, Y.; Tajima, H.; Takahashi, H.; Takahashi, M.; Takata, J.; Takeishi, R.; Berti, A.; Tam, P. H. T.; Tanaka, S. J.; Tateishi, D.; Tejedor, L. A.; Temnikov, P.; Terada, Y.; Terauchi, K.; Terzic, T.; Teshima, M.; Tluczykont, M.; Bhattacharjee, P.; Tokanai, F.; Torres, D. F.; Travnicek, P.; Truzzi, S.; Tutone, A.; Uhlrich, G.; Vacula, M.; Vallania, P.; van Scherpenberg, J.; Vázquez Acosta, M.; Biederbeck, N.; Verguilov, V.; Viale, I.; Vigliano, A.; Vigorito, C. F.; Vitale, V.; Voutsinas, G.; Vovk, I.; Vuillaume, T.; Walter, R.;Abstract The Cherenkov Telescope Array (CTA) is a next-generation ground-based observatory for gamma-ray astronomy at very high energies. The Large-Sized Telescope prototype (LST-1) is located at the CTA-North site, on the Canary Island of La Palma. LSTs are designed to provide optimal performance in the lowest part of the energy range covered by CTA, down to ≃20 GeV. LST-1 started performing astronomical observations in 2019 November, during its commissioning phase, and it has been taking data ever since. We present the first LST-1 observations of the Crab Nebula, the standard candle of very-high-energy gamma-ray astronomy, and use them, together with simulations, to assess the performance of the telescope. LST-1 has reached the expected performance during its commissioning period—only a minor adjustment of the preexisting simulations was needed to match the telescope’s behavior. The energy threshold at trigger level is around 20 GeV, rising to ≃30 GeV after data analysis. Performance parameters depend strongly on energy, and on the strength of the gamma-ray selection cuts in the analysis: angular resolution ranges from 0.°12–0.°40, and energy resolution from 15%–50%. Flux sensitivity is around 1.1% of the Crab Nebula flux above 250 GeV for a 50 hr observation (12% for 30 minutes). The spectral energy distribution (in the 0.03–30 TeV range) and the light curve obtained for the Crab Nebula agree with previous measurements, considering statistical and systematic uncertainties. A clear periodic signal is also detected from the pulsar at the center of the Nebula.
Archivio istituziona... arrow_drop_down Archivio istituzionale della ricerca - Università degli Studi di UdineArticle . 2023License: CC BYRecolector de Ciencia Abierta, RECOLECTAArticle . 2023 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARepository of the Czech Academy of SciencesArticle . 2023Data sources: Repository of the Czech Academy of SciencesDiposit Digital de la Universitat de BarcelonaArticle . 2023Data sources: Diposit Digital de la Universitat de BarcelonaIRIS - Università degli Studi di CataniaArticle . 2023Data sources: IRIS - Università degli Studi di Cataniahttps://dx.doi.org/10.48550/ar...Article . 2023License: arXiv Non-Exclusive DistributionData sources: DataciteThe Astrophysical JournalArticle . 2023 . Peer-reviewedData sources: European Union Open Data PortalUniversité Savoie Mont Blanc: HALArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ace89d&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 16 citations 16 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!visibility 57visibility views 57 download downloads 92 Powered bymore_vert Archivio istituziona... arrow_drop_down Archivio istituzionale della ricerca - Università degli Studi di UdineArticle . 2023License: CC BYRecolector de Ciencia Abierta, RECOLECTAArticle . 2023 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARepository of the Czech Academy of SciencesArticle . 2023Data sources: Repository of the Czech Academy of SciencesDiposit Digital de la Universitat de BarcelonaArticle . 2023Data sources: Diposit Digital de la Universitat de BarcelonaIRIS - Università degli Studi di CataniaArticle . 2023Data sources: IRIS - Università degli Studi di Cataniahttps://dx.doi.org/10.48550/ar...Article . 2023License: arXiv Non-Exclusive DistributionData sources: DataciteThe Astrophysical JournalArticle . 2023 . Peer-reviewedData sources: European Union Open Data PortalUniversité Savoie Mont Blanc: HALArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ace89d&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Journal 2021Embargo end date: 01 Jan 2021 Australia, France, France, France, Germany, Australia, France, France, Poland, France, France, Italy, France, France, France, Netherlands, Germany, France, GermanyPublisher:American Association for the Advancement of Science (AAAS) Publicly fundedS. Steinmassl; Sebastian Panny; Alexandre Marcowith; Regis Terrier; S. Sailer; Alison Mitchell; D. Jankowsky; Garret Cotter; Werner Hofmann; Michael Backes; Michael Backes; M. Spir-Jacob; Davit Zargaryan; Davit Zargaryan; Sabrina Casanova; Kleopas Shiningayamwe; A. Montanari; Jacek Niemiec; Dieter Horns; E. Kasai; Jonathan Mackey; C. Levy; J. Devin; Gavin Rowell; Jim Hinton; K. Nakashima; M. Seglar-Arroyo; R. Marx; R. Marx; L. Mohrmann; M. Renaud; Samuel Zouari; Jimmy N.S. Shapopi; Rafal Moderski; D. A. Sanchez; M. de Bony de Lavergne; F. Ait Benkhali; Christian Stegmann; C. Arcaro; A.M. Taylor; K. L. Page; Hassan Abdalla; D. Berge; S. Fegan; V. Joshi; Yasunobu Uchiyama; Łukasz Stawarz; B. Bi; Yvonne Becherini; E. O. Angüner; K. Kosack; Jim Davies; Thomas Murach; Sylvia Zhu; James E. M. Watson; T. Chand; Markus Holler; L. Dirson; J. Dyks; A. Priyana Noel; A. Zech; V. Barbosa Martins; L. Rinchiuso; A. S. Seyffert; S. Chandra; V. Marandon; Maria Haupt; V. Sahakian; Frank M. Rieger; Natalia Żywucka; Iryna Lypova; Hester Schutte; M. Panter; Axel Donath; P. A. Evans; Stefan Wagner; J. Zorn; Mohanraj Senniappan; F. Schüssler; Celine Armand; F. Werner; Tomasz Bulik; E. de Ona Wilhelmi; Hambeleleni Ndiyavala; A. Lemiere; M. Curyło; A. A. Zdziarski; N. Shafi; Victor Doroshenko; C. van Rensburg; Riaan Steenkamp; Felix Aharonian; Felix Aharonian; Felix Aharonian; Misao Sasaki; Johannes Veh; Monica Barnard; Stefan Klepser; R. Konno; Tom Armstrong; H. Prokoph; M. Tsirou; M. A. Kastendieck; M. Scalici; Andreas Specovius; M. Lemoine-Goumard; L. Olivera-Nieto; G. Fichet de Clairfontaine; Michal Ostrowski; H. Ashkar; Samuel Timothy Spencer; S. Raab; Roberta Zanin; H. Odaka; Włodek Kluźniak; Rachel Simoni; J.-P. Lenain; Andrea Santangelo; J.F. Glicenstein; B. Peyaud; J.-P. Ernenwein; G. Hermann; Clemens Hoischen; Domenico Tiziani; Felix Jankowsky; D. Malyshev; Carlo Romoli; F. Eichhorn; J. Schäfer; Pierre Brun; Christopher J. Duffy; A. Dmytriiev; Anna Barnacka; M. Zacharias; M. Zacharias; A. Djannati-Ataï; M. Büchele; V. Baghmanyan; Tadayuki Takahashi; Armelle Jardin-Blicq; Stefan Funk; D. Huber; A. Reimer; R. J. White; J. Bolmont; G. Vasileiadis; R. D. Parsons; G. Martí-Devesa; Dmitriy Kostunin; T. Tam; L. Giunti; L. Giunti; Elisabetta Bissaldi; Elisabetta Bissaldi; K. Egberts; Gianluca Giavitto; Jacco Vink; M. de Naurois; I. Jung-Richardt; Constantin Steppa; Konrad Bernlöhr; J. H. E. Thiersen; Bruno Khelifi; Paolo Marchegiani; M. Hörbe; E. Ruiz-Velasco; L. Oakes; Michael Kreter; Q. Piel; A. W. Chen; A. Wierzcholska; Dmitry Khangulyan; Lenka Tomankova; P. Reichherzer; Marek Jamrozy; G. Fontaine; Helene Sol; M.-H. Grondin; C. Moore; Yu Wun Wong; Isak Delberth Davids; G. Pühlhofer; S. Pita; B. Rudak; Kirsty Feijen; M. Bryan; P. Vincent; P. T. O'Brien; Nu. Komin; Christo Venter; Christoph Deil; Lei Sun; Mischa Breuhaus; Jhilik Majumdar; Joachim Hahn; T. Tavernier; A. Fiasson; D. A. Prokhorov; Michael Punch; Michael Punch;pmid: 34083487
An intrinsic gamma-ray burst afterglow Long gamma-ray bursts (GRBs) are emitted by relativistic jets generated during the collapse of a massive star in a distant galaxy. The GRB itself lasts only a few seconds but is followed by an afterglow that can persist for hours or days. The H.E.S.S. Collaboration observed the afterglow of GRB 190829A, a nearby long GRB. The proximity of this burst allowed it to be detected at tera–electron volt energies that would otherwise be absorbed in the intergalactic medium. By analyzing the spectrum and light curve at x-ray and gamma-ray wavelengths, the authors show that the afterglow cannot be explained by standard models. Science , abe8560, this issue p. 1081
Archivio Istituziona... arrow_drop_down Archivio Istituzionale della Ricerca - Politecnico di BariArticle . 2021Universiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2021Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2021Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: HALArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)The University of Adelaide: Digital LibraryArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)Eberhard Karls University Tübingen: Publication SystemArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1126/science.abe8560&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 113 citations 113 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!more_vert Archivio Istituziona... arrow_drop_down Archivio Istituzionale della Ricerca - Politecnico di BariArticle . 2021Universiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2021Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2021Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: HALArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)The University of Adelaide: Digital LibraryArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)Eberhard Karls University Tübingen: Publication SystemArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1126/science.abe8560&type=result"></script>'); --> </script>For further information contact us at helpdesk@openaire.eu