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description Publicationkeyboard_double_arrow_right Article , Journal 2002 ItalyPublisher:Elsevier BV Avdeev, S; Bidoli, V; Casolino, M; De Grandis, E; Furano, G; Morselli, A; NARICI, LIVIO; DE PASCALE, MARIA PIA; PICOZZA, PIERGIORGIO; REALI, ENZO; SPARVOLI, ROBERTA; Boezio, M; Carlson, P; Bonvicini, W; Vacchi, A; Zampa, N; Castellini, G; Fuglesang, C; Galper, A; Khodarovich, A; Ozerov, Y; Popov, A; Vavilov, N; Mazzenga, G; Ricci, M; Sannita, W; Spillantini, P.;The phenomenon of light flashes (LF) in eyes for people in space has been investigated onboard Mir. Data on particles hitting the eye have been collected with the SilEye detectors, and correlated with human observations. It is found that a nucleus in the radiation environment of Mir has roughly a 1% probability to cause an LF, whereas the proton probability is almost three orders of magnitude less. As a function of LET, the LF probability increases above 10 keV/micrometer, reaching about 5% at around 50 keV/micrometer.
Acta Astronautica arrow_drop_down Archivio della Ricerca - Università di Roma Tor vergataArticle . 2002Data sources: Archivio della Ricerca - Università di Roma Tor vergataArchivio della Ricerca - Università di Roma Tor vergataArticle . 2002Data 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.
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For further information contact us at helpdesk@openaire.eu36 citations 36 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!
more_vert Acta Astronautica arrow_drop_down Archivio della Ricerca - Università di Roma Tor vergataArticle . 2002Data sources: Archivio della Ricerca - Università di Roma Tor vergataArchivio della Ricerca - Università di Roma Tor vergataArticle . 2002Data 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=10.1016/s0094-5765(01)00190-4&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2023Embargo end date: 01 Jan 2023 Italy, Italy, Italy, Italy, Slovenia, Italy, Australia, France, Germany, United Kingdom, Italy, AustraliaPublisher:American Astronomical Society D. A. Smith; S. Abdollahi; M. Ajello; M. Bailes; L. Baldini; J. Ballet; M. G. Baring; C. Bassa; J. Becerra Gonzalez; R. Bellazzini; A. Berretta; B. Bhattacharyya; E. Bissaldi; R. Bonino; E. Bottacini; J. Bregeon; P. Bruel; M. Burgay; T. H. Burnett; R. A. Cameron; F. Camilo; R. Caputo; P. A. Caraveo; E. Cavazzuti; G. Chiaro; S. Ciprini; C. J. Clark; I. Cognard; A. Corongiu; P. Cristarella Orestano; M. Crnogorcevic; A. Cuoco; S. Cutini; F. D’Ammando; A. de Angelis; M. E. DeCesar; S. De Gaetano; R. de Menezes; J. Deneva; F. de Palma; N. Di Lalla; F. Dirirsa; L. Di Venere; A. Domínguez; D. Dumora; S. J. Fegan; E. C. Ferrara; A. Fiori; H. Fleischhack; C. Flynn; A. Franckowiak; P. C. C. Freire; Y. Fukazawa; P. Fusco; G. Galanti; V. Gammaldi; F. Gargano; D. Gasparrini; F. Giacchino; N. Giglietto; F. Giordano; M. Giroletti; D. Green; I. A. Grenier; L. Guillemot; S. Guiriec; M. Gustafsson; A. K. Harding; E. Hays; J. W. Hewitt; D. Horan; X. Hou; F. Jankowski; R. P. Johnson; T. J. Johnson; S. Johnston; J. Kataoka; M. J. Keith; M. Kerr; M. Kramer; M. Kuss; L. Latronico; S.-H. Lee; D. Li; J. Li; B. Limyansky; F. Longo; F. Loparco; L. Lorusso; M. N. Lovellette; M. Lower; P. Lubrano; A. G. Lyne; Y. Maan; S. Maldera; R. N. Manchester; A. Manfreda; M. Marelli; G. Martí-Devesa; M. N. Mazziotta; J. E. McEnery; I. Mereu; P. F. Michelson; M. Mickaliger; W. Mitthumsiri; T. Mizuno; A. A. Moiseev; M. E. Monzani; A. Morselli; M. Negro; R. Nemmen; L. Nieder; E. Nuss; N. Omodei; M. Orienti; E. Orlando; J. F. Ormes; M. Palatiello; D. Paneque; G. Panzarini; A. Parthasarathy; M. Persic; M. Pesce-Rollins; R. Pillera; H. Poon; T. A. Porter; A. Possenti; G. Principe; S. Rainò; R. Rando; S. M. Ransom; P. S. Ray; M. Razzano; S. Razzaque; A. Reimer; O. Reimer; N. Renault-Tinacci; R. W. Romani; M. Sánchez-Conde; P. M. Saz Parkinson; L. Scotton; D. Serini; C. Sgrò; R. Shannon; V. Sharma; Z. Shen; E. J. Siskind; G. Spandre; P. Spinelli; B. W. Stappers; T. E. Stephens; D. J. Suson; S. Tabassum; H. Tajima; D. Tak; G. Theureau; D. J. Thompson; O. Tibolla; D. F. Torres; J. Valverde; C. Venter; Z. Wadiasingh; N. Wang; N. Wang; P. Wang; P. Weltevrede; K. Wood; J. Yan; G. Zaharijas; C. Zhang; W. Zhu;handle: 20.500.12556/RUNG-8758 , 11568/1225127 , 11589/264401 , 11587/517606 , 2318/1947773 , 11586/473196 , 1959.3/476456
Abstract We present 294 pulsars found in GeV data from the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope. Another 33 millisecond pulsars (MSPs) discovered in deep radio searches of LAT sources will likely reveal pulsations once phase-connected rotation ephemerides are achieved. A further dozen optical and/or X-ray binary systems colocated with LAT sources also likely harbor gamma-ray MSPs. This catalog thus reports roughly 340 gamma-ray pulsars and candidates, 10% of all known pulsars, compared to ≤11 known before Fermi. Half of the gamma-ray pulsars are young. Of these, the half that are undetected in radio have a broader Galactic latitude distribution than the young radio-loud pulsars. The others are MSPs, with six undetected in radio. Overall, ≥236 are bright enough above 50 MeV to fit the pulse profile, the energy spectrum, or both. For the common two-peaked profiles, the gamma-ray peak closest to the magnetic pole crossing generally has a softer spectrum. The spectral energy distributions tend to narrow as the spindown power E ̇ decreases to its observed minimum near 1033 erg s−1, approaching the shape for synchrotron radiation from monoenergetic electrons. We calculate gamma-ray luminosities when distances are available. Our all-sky gamma-ray sensitivity map is useful for population syntheses. The electronic catalog version provides gamma-ray pulsar ephemerides, properties, and fit results to guide and be compared with modeling results.
Archivio Istituziona... arrow_drop_down Università degli Studi di Bari Aldo Moro: CINECA IRISArticle . 2023Full-Text: https://hdl.handle.net/11586/473196Data sources: Bielefeld Academic Search Engine (BASE)Repository of University of Nova GoricaArticle . 2023Data sources: Repository of University of Nova GoricaThe University of Manchester - Institutional RepositoryArticle . 2023Data sources: The University of Manchester - Institutional RepositoryArchive de l'Observatoire de Paris (HAL)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: HALArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Archivio della Ricerca - Università di PisaArticle . 2023Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2023Swinburne University of Technology: Swinburne Research BankArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: 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/acee67&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 81 citations 81 popularity Top 10% influence Top 10% impulse Top 1% Powered by BIP!
more_vert Archivio Istituziona... arrow_drop_down Università degli Studi di Bari Aldo Moro: CINECA IRISArticle . 2023Full-Text: https://hdl.handle.net/11586/473196Data sources: Bielefeld Academic Search Engine (BASE)Repository of University of Nova GoricaArticle . 2023Data sources: Repository of University of Nova GoricaThe University of Manchester - Institutional RepositoryArticle . 2023Data sources: The University of Manchester - Institutional RepositoryArchive de l'Observatoire de Paris (HAL)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: HALArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Archivio della Ricerca - Università di PisaArticle . 2023Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2023Swinburne University of Technology: Swinburne Research BankArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: 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/acee67&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 1999 ItalyPublisher:EDP Sciences TAVANI M.; BARBIELLINI G.; CARAVEO P.; COCCO V.; COSTA E.; DI COCCO G.; LABANTI C.; LONGO F.; MEREGHETTI S.; MORSELLI A.; PELLIZZONI A.; PICOZZA P.; PIRO L.; PREST, MICHELA; VERCELLONE S.;doi: 10.1051/aas:1999357
handle: 11383/1489900
AGILE is a gamma-ray mission planned to be operating as an Observatory during the period 2002-2005. Its baseline instrument is designed to detect gamma rays in the band. AGILE's good sensitivity, very large field of view ( of the whole sky), and excellent timing capability ( ms deadtime) are ideal to study gamma-ray bursts (GRBs). AGILE is expected to detect ~10 GRBs per year at energies above 100 MeV. The Super–AGILE option might be able to localize GRBs within a few arcminutes and provide additional information in the hard X-ray band. A rapid alert program is an essential part of the scientific goals of the AGILE Observatory.
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=10.1051/aas:1999357&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 3 citations 3 popularity Average influence Average impulse Average Powered by BIP!
more_vert 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=10.1051/aas:1999357&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type , Preprint , Journal 2019Embargo end date: 01 Jan 2019 Netherlands, Poland, Netherlands, United Kingdom, France, Slovenia, Switzerland, France, France, Brazil, Australia, Germany, France, Croatia, Netherlands, Germany, Netherlands, France, France, France, United Kingdom, Netherlands, France, United Kingdom, Croatia, France, Spain, France, France, Germany, Germany, United Kingdom, Italy, Spain, France, Chile, France, Australia, FrancePublisher:Elsevier BV Publicly fundedFunded by:NSERC, UKRI | RootDetect: Remote Detect..., EC | INFIERI +3 projectsNSERC ,UKRI| RootDetect: Remote Detection and Precision Management of Root Health ,EC| INFIERI ,EC| CTA-PP ,EC| PROBIST ,EC| CTA-DEVM. Ostrowski; N. Renault-Tinacci; T. Suomijärvi; Takeshi Nakamori; T.R.N. Ekoume; Maria Chernyakova; Tomohiro Inada; Maria Concetta Maccarone; Alison Mitchell; A. Nagai; Andrea Bulgarelli; Geoff Romeo; A. Berti; Antonio Stamerra; R. de Cássia dos Anjos; R. J. White; Carlo Vigorito; Helene Sol; G. Ferrand; V. Vitale; F. Di Pierro; Massimo Persic; Daniel Morcuende; Jonathan Blazek; Marita Krause; Vito Conforti; S. Rainò; Ruben Alfaro; Saverio Lombardi; D. Zavrtanik; German Martinez; Luisa Arrabito; Konstancja Satalecka; Gianluca Giavitto; Pierre Brun; Jacco Vink; M. de Naurois; M. V. Fonseca; E. Fiandrini; Pietro Bruno; Fuyuki Tokanai; M. Nöthe; H.-S. Zechlin; Jaime Rosado; C. J. Todero Peixoto; Eva Sciacca; M. Prouza; T. Greenshaw; V. I. Zhdanov; J. J. Rodríguez Vázquez; M. Mariotti; Konrad Bernlöhr; J. Knapp; G. Ambrosi; R. López-Coto; N. Otte; M. Polo; V. Vassiliev; Alessandro Costa; G. S. Varner; S. Fegan; P. Cumani; M. López; G. Chiaro; F. Cassol; Diego F. Torres; Diego F. Torres; Pol Bordas; Paweł Świerk; A. M. Lopez; Daniele Gaggero; Daniele Gaggero; L. Freixas Coromina; M. Will; I. Agudo; Maxim V. Barkov; S. Karkar; B. De Lotto; E. Mach; Luca Zampieri; Jürgen Knödlseder; G. Bonnoli; T. Di Girolamo; D. della Volpe; Tarek M. Hassan; A. M. Brown; Anatolii Zenin; Hidetoshi Sano; V. De Caprio; R. Millul; Sebastian Diebold; Julien Lefaucheur; R. J. García López; Marc Ribó; Rodrigo Nemmen; G. Fontaine; S. Flis; G. Emery; T. Tam; Konstantinos N. Gourgouliatos; L. Mohrmann; Nu. Komin; E. Fedorova; C. Alispach; Z. Ou; Juan Cortina; Takashi Saito; Elena Amato; Elisabetta Bissaldi; Shanta M. Zimmer; J. Gironnet; G. Pareschi; Sylvain Chaty; S. Vercellone; Maria Magdalena González; I. Oya; Heide Costantini; Daniel Nieto; Marek Nikolajuk; Farinaldo S. Queiroz; Jonathan S. Lapington; M. Perri; J. Becerra González; B. Khélifi; L. Di Venere; Juan Abel Barrio; A. Rugliancich; Łukasz Stawarz; E. O. Angüner; E. de Oña Wilhelmi; T. Nagayoshi; N. Parmiggiani; Miroslav Hrabovsky; D. de Martino; T. Montaruli; Thomas Murach; M. Iori; Vincenzo Testa; Bohdan Hnatyk; M. Fiori; Lenka Tomankova; Juan Carlos Rodríguez-Ramírez; Reiko Orito; Petr Janecek; Satoshi Fukami; David A. Williams; A. Burtovoi; Enrico Cascone; Reshmi Mukherjee; Etienne Lyard; Marcello Giroletti; Petar Temnikov; F. Salesa Greus; Q. Feng; R. Paoletti; Diego Falceta-Gonçalves; Stefan Kimeswenger; A. Kong; L. P. Taylor; Daniela Maria Ribeiro; Philip Kaaret; G. Morlino; R. D. Parsons; D. Nosek; Michael Zacharias; I. Sadeh; Fabio Iocco; Hidetoshi Kubo; M. Hayashida; N. Hiroshima; Rodrigo Guedes Lang; Martin Pohl; M. Vecchi; M. Vecchi; M. Nievas Rosillo; Fulvio Gianotti; A. Fiasson; M. Garczarczyk; F. Arqueros; N. Produit; A. Morselli; Thomas Lohse; Francesco Longo; D. Dominis Prester; Manuel Meyer; M. Zavrtanik; Matteo Cerruti; Enrico Congiu; J. Kushida; Jakub Juryšek; Jakub Juryšek; Paramita Barai; Agnieszka Slowikowska; Y. Kobayashi; Ermanno Pietropaolo; Q. Piel; L. Tosti; B. Bertucci; Michael G. Burton; J. M. Paredes;doi: 10.1016/j.astropartphys.2019.04.001 , 10.3204/pubdb-2019-02176 , 10.48550/arxiv.1904.01426 , 10.5167/uzh-185554
handle: 2066/204317 , https://repository.ubn.ru.nl/handle/2066/204317 , 11588/836701 , 11588/1002980 , 11368/2948845 , 11245.1/15060f98-9266-4cbe-b13f-d5eb36bfca84 , 11370/56c95366-7d1c-41bc-8642-89d81f7b2d08 , 20.500.14243/384369 , 10261/189767 , 11365/1082110 , 11449/188943 , 20.500.12556/RUNG-4481-6fc900a7-bfd6-9d11-ce01-125b62caf538 , 11577/3303347 , 11390/1148589 , 11578/310854 , 11573/1279912 , 11568/1151989 , 11589/176927 , 11391/1449632 , 11697/136912 , 11587/447196 , 2158/1353568 , 2318/1771875 , 11586/348637 , 2440/121474 , 10900/99174
doi: 10.1016/j.astropartphys.2019.04.001 , 10.3204/pubdb-2019-02176 , 10.48550/arxiv.1904.01426 , 10.5167/uzh-185554
handle: 2066/204317 , https://repository.ubn.ru.nl/handle/2066/204317 , 11588/836701 , 11588/1002980 , 11368/2948845 , 11245.1/15060f98-9266-4cbe-b13f-d5eb36bfca84 , 11370/56c95366-7d1c-41bc-8642-89d81f7b2d08 , 20.500.14243/384369 , 10261/189767 , 11365/1082110 , 11449/188943 , 20.500.12556/RUNG-4481-6fc900a7-bfd6-9d11-ce01-125b62caf538 , 11577/3303347 , 11390/1148589 , 11578/310854 , 11573/1279912 , 11568/1151989 , 11589/176927 , 11391/1449632 , 11697/136912 , 11587/447196 , 2158/1353568 , 2318/1771875 , 11586/348637 , 2440/121474 , 10900/99174
The Cherenkov Telescope Array (CTA) is the major next-generation observatory for ground-based very-high-energy gamma-ray astronomy. It will improve the sensitivity of current ground-based instruments by a factor of five to twenty, depending on the energy, greatly improving both their angular and energy resolutions over four decades in energy (from 20 GeV to 300 TeV). This achievement will be possible by using tens of imaging Cherenkov telescopes of three successive sizes. They will be arranged into two arrays, one per hemisphere, located on the La Palma island (Spain) and in Paranal (Chile). We present here the optimised and final telescope arrays for both CTA sites, as well as their foreseen performance, resulting from the analysis of three different large-scale Monte Carlo productions. Astroparticle physics 111, 35 - 53 (2019). doi:10.1016/j.astropartphys.2019.04.001 Published by Elsevier Science, Amsterdam [u.a.]
CORE arrow_drop_down Usiena air - Università di SienaArticle . 2019License: CC BY NC NDData sources: Usiena air - Università di SienaArchivio istituzionale della ricerca - Università IUAV di VeneziaArticle . 2019License: CC BY NC NDUniversità degli Studi di Siena: USiena airArticle . 2019Full-Text: http://hdl.handle.net/11365/1082110Data sources: Bielefeld Academic Search Engine (BASE)Universidade Estadual Paulista São Paulo: Repositório Institucional UNESPArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Croatian Scientific Bibliography - CROSBIArticle . 2019Data sources: Croatian Scientific Bibliography - CROSBIRecolector de Ciencia Abierta, RECOLECTAArticle . 2019Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2019 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2019 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle PhysicsArticle . 2019License: CC BY NC SAData sources: Universiteit van Amsterdam Digital Academic RepositoryAstroparticle PhysicsArticle . 2019License: taverneData sources: University of Groningen Research PortalUniversity of Bath's research portalArticle . 2019Data sources: University of Bath's research portalOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2019Data sources: OA@INAF - Istituto Nazionale di AstrofisicaUniversiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2019Data sources: Bielefeld Academic Search Engine (BASE)Zurich Open Repository and ArchiveArticle . 2019 . Peer-reviewedData sources: Zurich Open Repository and ArchiveRepository of University of Nova GoricaArticle . 2019Data sources: Repository of University of Nova GoricaArchivio della Ricerca - Università di PisaArticle . 2019Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2019Flore (Florence Research Repository)Article . 2019Data sources: Flore (Florence Research Repository)Università degli Studi di Bari Aldo Moro: CINECA IRISArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2019Data sources: Bielefeld Academic Search Engine (BASE)Pontificia Universidad Católica de Chile: Repositorio UCArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)University of Western Sydney (UWS): Research DirectArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Institut National de la Recherche Agronomique: ProdINRAArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: HALArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)The University of Adelaide: Digital LibraryArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Eberhard Karls University Tübingen: Publication SystemArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2019Data 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=10.1016/j.astropartphys.2019.04.001&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 40 citations 40 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!
visibility 79visibility views 79 download downloads 124 Powered bymore_vert CORE arrow_drop_down Usiena air - Università di SienaArticle . 2019License: CC BY NC NDData sources: Usiena air - Università di SienaArchivio istituzionale della ricerca - Università IUAV di VeneziaArticle . 2019License: CC BY NC NDUniversità degli Studi di Siena: USiena airArticle . 2019Full-Text: http://hdl.handle.net/11365/1082110Data sources: Bielefeld Academic Search Engine (BASE)Universidade Estadual Paulista São Paulo: Repositório Institucional UNESPArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Croatian Scientific Bibliography - CROSBIArticle . 2019Data sources: Croatian Scientific Bibliography - CROSBIRecolector de Ciencia Abierta, RECOLECTAArticle . 2019Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2019 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2019 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle PhysicsArticle . 2019License: CC BY NC SAData sources: Universiteit van Amsterdam Digital Academic RepositoryAstroparticle PhysicsArticle . 2019License: taverneData sources: University of Groningen Research PortalUniversity of Bath's research portalArticle . 2019Data sources: University of Bath's research portalOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2019Data sources: OA@INAF - Istituto Nazionale di AstrofisicaUniversiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2019Data sources: Bielefeld Academic Search Engine (BASE)Zurich Open Repository and ArchiveArticle . 2019 . Peer-reviewedData sources: Zurich Open Repository and ArchiveRepository of University of Nova GoricaArticle . 2019Data sources: Repository of University of Nova GoricaArchivio della Ricerca - Università di PisaArticle . 2019Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2019Flore (Florence Research Repository)Article . 2019Data sources: Flore (Florence Research Repository)Università degli Studi di Bari Aldo Moro: CINECA IRISArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2019Data sources: Bielefeld Academic Search Engine (BASE)Pontificia Universidad Católica de Chile: Repositorio UCArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)University of Western Sydney (UWS): Research DirectArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Institut National de la Recherche Agronomique: ProdINRAArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: HALArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)The University of Adelaide: Digital LibraryArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Eberhard Karls University Tübingen: Publication SystemArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2019Data 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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For further information contact us at helpdesk@openaire.eudescription 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.
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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.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2004 ItalyPublisher:American Astronomical Society Papini P.; Piccardi S.; Spillantini P.; Vannuccini E.; Ambriola M.; Bellotti R.; Cafagna F.; Ciacio F.; Circella M.; De Marzo C. N.; Bartalucci S.; Ricci M.; Bergström D.; Carlson P.; Francke T.; Hansen P.; Mocchiutti E.; Boezio M.; Bonvicini V.; Schiavon P.; Vacchi A.; Zampa N.; Bravar U.; Stochaj S. J.; Casolino M.; De Pascale M. P.; Morselli A.; Picozza P.; Sparvoli R.; Hof M.; Kremer J.; Menn W.; Simon M.; Mitchell J. W.; Ormes J. F.; Stephens S. A.; Streitmatter R. E.; Suffert M.;doi: 10.1086/424027
handle: 11368/1909078 , 11390/1125294
We report the first measurement of the deuterium abundance in cosmic rays above 10 GeV nucleon � 1 of kinetic energy. The data were collected by the balloon-borne experiment CAPRICE98, which was flown on 1998 May 28–29 from Fort Sumner, New Mexico. The detector configuration included the NMSU-WiZard/CAPRICE superconducting magnet spectrometer equipped with a gas RICH detector, a silicon-tungsten calorimeter, and a time-of-flight system. By combining the information from the spectrometer and the RICH detector, it was possible to separate deuterons from protons in the kinetic energy range from 12 to 22 GeV nucleon � 1 .I n order to estimate the proton background and the deuteron selection efficiency, we developed an empirical model for the response of the instrument, based on the data collected in this experiment. The analysis procedure is described in this paper, and the result on the absolute flux of deuterium is presented. We found that the deuterium abundance at high energy is consistent with the hypothesis that the propagation mechanism of light nuclei is the same as that of heavier secondary components. Subject headings: balloons — cosmic rays — Galaxy: abundances — ISM: abundances
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.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 25 citations 25 popularity Top 10% influence Top 10% impulse Average Powered by BIP!
more_vert 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=10.1086/424027&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Conference object , Other literature type 2006 ItalyPublisher:Elsevier BV Claudia Cecchi; Francesca Marcucci; Marco Frailis; Alessandro De Angelis; P. Boinee; F. Gargano; Andrea Lionetto; Gino Tosti; M. Pepe; Luca Latronico; Luca Baldini; P. Lubrano; A. Morselli; Michael Kuss; Gloria Spandre; N. Giglietto; M. N. Mazziotta; Riccardo Rando; Massimo Fiorucci; Nicola Omodei; Denis Bastieri; G. Cabras; R. Giannitrapani; Dario Favretto; Dario Favretto; M. Razzano; Edoardo Milotti; M. Brigida; F. Loparco; Francesco Longo;handle: 11368/2338341 , 11577/2828999 , 11390/858636 , 11568/108568 , 11589/14515 , 11391/995277
This paper presents the simulation of the GLAST high energy gamma-ray telescope. The simulation package, written in C++, is based on the Geant4 toolkit, and it is integrated into a general framework used to process events. A detailed simulation of the electronic signals inside Silicon detectors has been provided and it is used for the particle tracking, which is handled by a dedicated software. A unique repository for the geometrical description of the detector has been realized using the XML language and a C++ library to access this information has been designed and implemented. As first application of the GLAST LAT software, one day of simulated data has been produced. This paper outlines the contribution developed by the Italian GLAST software group.
Open Access Reposito... arrow_drop_down Nuclear Physics B - Proceedings SupplementsArticle . 2006 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefArchivio istituzionale della ricerca - Università di TriesteConference object . 2006Archivio della Ricerca - Università di PisaConference object . 2006Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale della Ricerca - Politecnico di BariConference object . 2006Archivio istituzionale della ricerca - Università di TriesteConference object . 2006add 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.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen 3 citations 3 popularity Average influence Average impulse Average Powered by BIP!
more_vert Open Access Reposito... arrow_drop_down Nuclear Physics B - Proceedings SupplementsArticle . 2006 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefArchivio istituzionale della ricerca - Università di TriesteConference object . 2006Archivio della Ricerca - Università di PisaConference object . 2006Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale della Ricerca - Politecnico di BariConference object . 2006Archivio istituzionale della ricerca - Università di TriesteConference object . 2006add 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=10.1016/j.nuclphysbps.2005.04.062&type=result"></script>'); --> </script>
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description Publicationkeyboard_double_arrow_right Article , Journal 2002 ItalyPublisher:Elsevier BV Avdeev, S; Bidoli, V; Casolino, M; De Grandis, E; Furano, G; Morselli, A; NARICI, LIVIO; DE PASCALE, MARIA PIA; PICOZZA, PIERGIORGIO; REALI, ENZO; SPARVOLI, ROBERTA; Boezio, M; Carlson, P; Bonvicini, W; Vacchi, A; Zampa, N; Castellini, G; Fuglesang, C; Galper, A; Khodarovich, A; Ozerov, Y; Popov, A; Vavilov, N; Mazzenga, G; Ricci, M; Sannita, W; Spillantini, P.;The phenomenon of light flashes (LF) in eyes for people in space has been investigated onboard Mir. Data on particles hitting the eye have been collected with the SilEye detectors, and correlated with human observations. It is found that a nucleus in the radiation environment of Mir has roughly a 1% probability to cause an LF, whereas the proton probability is almost three orders of magnitude less. As a function of LET, the LF probability increases above 10 keV/micrometer, reaching about 5% at around 50 keV/micrometer.
Acta Astronautica arrow_drop_down Archivio della Ricerca - Università di Roma Tor vergataArticle . 2002Data sources: Archivio della Ricerca - Università di Roma Tor vergataArchivio della Ricerca - Università di Roma Tor vergataArticle . 2002Data 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.
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For further information contact us at helpdesk@openaire.eu36 citations 36 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!
more_vert Acta Astronautica arrow_drop_down Archivio della Ricerca - Università di Roma Tor vergataArticle . 2002Data sources: Archivio della Ricerca - Università di Roma Tor vergataArchivio della Ricerca - Università di Roma Tor vergataArticle . 2002Data 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=10.1016/s0094-5765(01)00190-4&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2023Embargo end date: 01 Jan 2023 Italy, Italy, Italy, Italy, Slovenia, Italy, Australia, France, Germany, United Kingdom, Italy, AustraliaPublisher:American Astronomical Society D. A. Smith; S. Abdollahi; M. Ajello; M. Bailes; L. Baldini; J. Ballet; M. G. Baring; C. Bassa; J. Becerra Gonzalez; R. Bellazzini; A. Berretta; B. Bhattacharyya; E. Bissaldi; R. Bonino; E. Bottacini; J. Bregeon; P. Bruel; M. Burgay; T. H. Burnett; R. A. Cameron; F. Camilo; R. Caputo; P. A. Caraveo; E. Cavazzuti; G. Chiaro; S. Ciprini; C. J. Clark; I. Cognard; A. Corongiu; P. Cristarella Orestano; M. Crnogorcevic; A. Cuoco; S. Cutini; F. D’Ammando; A. de Angelis; M. E. DeCesar; S. De Gaetano; R. de Menezes; J. Deneva; F. de Palma; N. Di Lalla; F. Dirirsa; L. Di Venere; A. Domínguez; D. Dumora; S. J. Fegan; E. C. Ferrara; A. Fiori; H. Fleischhack; C. Flynn; A. Franckowiak; P. C. C. Freire; Y. Fukazawa; P. Fusco; G. Galanti; V. Gammaldi; F. Gargano; D. Gasparrini; F. Giacchino; N. Giglietto; F. Giordano; M. Giroletti; D. Green; I. A. Grenier; L. Guillemot; S. Guiriec; M. Gustafsson; A. K. Harding; E. Hays; J. W. Hewitt; D. Horan; X. Hou; F. Jankowski; R. P. Johnson; T. J. Johnson; S. Johnston; J. Kataoka; M. J. Keith; M. Kerr; M. Kramer; M. Kuss; L. Latronico; S.-H. Lee; D. Li; J. Li; B. Limyansky; F. Longo; F. Loparco; L. Lorusso; M. N. Lovellette; M. Lower; P. Lubrano; A. G. Lyne; Y. Maan; S. Maldera; R. N. Manchester; A. Manfreda; M. Marelli; G. Martí-Devesa; M. N. Mazziotta; J. E. McEnery; I. Mereu; P. F. Michelson; M. Mickaliger; W. Mitthumsiri; T. Mizuno; A. A. Moiseev; M. E. Monzani; A. Morselli; M. Negro; R. Nemmen; L. Nieder; E. Nuss; N. Omodei; M. Orienti; E. Orlando; J. F. Ormes; M. Palatiello; D. Paneque; G. Panzarini; A. Parthasarathy; M. Persic; M. Pesce-Rollins; R. Pillera; H. Poon; T. A. Porter; A. Possenti; G. Principe; S. Rainò; R. Rando; S. M. Ransom; P. S. Ray; M. Razzano; S. Razzaque; A. Reimer; O. Reimer; N. Renault-Tinacci; R. W. Romani; M. Sánchez-Conde; P. M. Saz Parkinson; L. Scotton; D. Serini; C. Sgrò; R. Shannon; V. Sharma; Z. Shen; E. J. Siskind; G. Spandre; P. Spinelli; B. W. Stappers; T. E. Stephens; D. J. Suson; S. Tabassum; H. Tajima; D. Tak; G. Theureau; D. J. Thompson; O. Tibolla; D. F. Torres; J. Valverde; C. Venter; Z. Wadiasingh; N. Wang; N. Wang; P. Wang; P. Weltevrede; K. Wood; J. Yan; G. Zaharijas; C. Zhang; W. Zhu;handle: 20.500.12556/RUNG-8758 , 11568/1225127 , 11589/264401 , 11587/517606 , 2318/1947773 , 11586/473196 , 1959.3/476456
Abstract We present 294 pulsars found in GeV data from the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope. Another 33 millisecond pulsars (MSPs) discovered in deep radio searches of LAT sources will likely reveal pulsations once phase-connected rotation ephemerides are achieved. A further dozen optical and/or X-ray binary systems colocated with LAT sources also likely harbor gamma-ray MSPs. This catalog thus reports roughly 340 gamma-ray pulsars and candidates, 10% of all known pulsars, compared to ≤11 known before Fermi. Half of the gamma-ray pulsars are young. Of these, the half that are undetected in radio have a broader Galactic latitude distribution than the young radio-loud pulsars. The others are MSPs, with six undetected in radio. Overall, ≥236 are bright enough above 50 MeV to fit the pulse profile, the energy spectrum, or both. For the common two-peaked profiles, the gamma-ray peak closest to the magnetic pole crossing generally has a softer spectrum. The spectral energy distributions tend to narrow as the spindown power E ̇ decreases to its observed minimum near 1033 erg s−1, approaching the shape for synchrotron radiation from monoenergetic electrons. We calculate gamma-ray luminosities when distances are available. Our all-sky gamma-ray sensitivity map is useful for population syntheses. The electronic catalog version provides gamma-ray pulsar ephemerides, properties, and fit results to guide and be compared with modeling results.
Archivio Istituziona... arrow_drop_down Università degli Studi di Bari Aldo Moro: CINECA IRISArticle . 2023Full-Text: https://hdl.handle.net/11586/473196Data sources: Bielefeld Academic Search Engine (BASE)Repository of University of Nova GoricaArticle . 2023Data sources: Repository of University of Nova GoricaThe University of Manchester - Institutional RepositoryArticle . 2023Data sources: The University of Manchester - Institutional RepositoryArchive de l'Observatoire de Paris (HAL)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: HALArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Archivio della Ricerca - Università di PisaArticle . 2023Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2023Swinburne University of Technology: Swinburne Research BankArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: 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.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 81 citations 81 popularity Top 10% influence Top 10% impulse Top 1% Powered by BIP!
more_vert Archivio Istituziona... arrow_drop_down Università degli Studi di Bari Aldo Moro: CINECA IRISArticle . 2023Full-Text: https://hdl.handle.net/11586/473196Data sources: Bielefeld Academic Search Engine (BASE)Repository of University of Nova GoricaArticle . 2023Data sources: Repository of University of Nova GoricaThe University of Manchester - Institutional RepositoryArticle . 2023Data sources: The University of Manchester - Institutional RepositoryArchive de l'Observatoire de Paris (HAL)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: HALArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Archivio della Ricerca - Università di PisaArticle . 2023Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2023Swinburne University of Technology: Swinburne Research BankArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2023Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2023Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: 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.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 1999 ItalyPublisher:EDP Sciences TAVANI M.; BARBIELLINI G.; CARAVEO P.; COCCO V.; COSTA E.; DI COCCO G.; LABANTI C.; LONGO F.; MEREGHETTI S.; MORSELLI A.; PELLIZZONI A.; PICOZZA P.; PIRO L.; PREST, MICHELA; VERCELLONE S.;doi: 10.1051/aas:1999357
handle: 11383/1489900
AGILE is a gamma-ray mission planned to be operating as an Observatory during the period 2002-2005. Its baseline instrument is designed to detect gamma rays in the band. AGILE's good sensitivity, very large field of view ( of the whole sky), and excellent timing capability ( ms deadtime) are ideal to study gamma-ray bursts (GRBs). AGILE is expected to detect ~10 GRBs per year at energies above 100 MeV. The Super–AGILE option might be able to localize GRBs within a few arcminutes and provide additional information in the hard X-ray band. A rapid alert program is an essential part of the scientific goals of the AGILE Observatory.
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.
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For further information contact us at helpdesk@openaire.euAccess Routesbronze 3 citations 3 popularity Average influence Average impulse Average Powered by BIP!
more_vert 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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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type , Preprint , Journal 2019Embargo end date: 01 Jan 2019 Netherlands, Poland, Netherlands, United Kingdom, France, Slovenia, Switzerland, France, France, Brazil, Australia, Germany, France, Croatia, Netherlands, Germany, Netherlands, France, France, France, United Kingdom, Netherlands, France, United Kingdom, Croatia, France, Spain, France, France, Germany, Germany, United Kingdom, Italy, Spain, France, Chile, France, Australia, FrancePublisher:Elsevier BV Publicly fundedFunded by:NSERC, UKRI | RootDetect: Remote Detect..., EC | INFIERI +3 projectsNSERC ,UKRI| RootDetect: Remote Detection and Precision Management of Root Health ,EC| INFIERI ,EC| CTA-PP ,EC| PROBIST ,EC| CTA-DEVM. Ostrowski; N. Renault-Tinacci; T. Suomijärvi; Takeshi Nakamori; T.R.N. Ekoume; Maria Chernyakova; Tomohiro Inada; Maria Concetta Maccarone; Alison Mitchell; A. Nagai; Andrea Bulgarelli; Geoff Romeo; A. Berti; Antonio Stamerra; R. de Cássia dos Anjos; R. J. White; Carlo Vigorito; Helene Sol; G. Ferrand; V. Vitale; F. Di Pierro; Massimo Persic; Daniel Morcuende; Jonathan Blazek; Marita Krause; Vito Conforti; S. Rainò; Ruben Alfaro; Saverio Lombardi; D. Zavrtanik; German Martinez; Luisa Arrabito; Konstancja Satalecka; Gianluca Giavitto; Pierre Brun; Jacco Vink; M. de Naurois; M. V. Fonseca; E. Fiandrini; Pietro Bruno; Fuyuki Tokanai; M. Nöthe; H.-S. Zechlin; Jaime Rosado; C. J. Todero Peixoto; Eva Sciacca; M. Prouza; T. Greenshaw; V. I. Zhdanov; J. J. Rodríguez Vázquez; M. Mariotti; Konrad Bernlöhr; J. Knapp; G. Ambrosi; R. López-Coto; N. Otte; M. Polo; V. Vassiliev; Alessandro Costa; G. S. Varner; S. Fegan; P. Cumani; M. López; G. Chiaro; F. Cassol; Diego F. Torres; Diego F. Torres; Pol Bordas; Paweł Świerk; A. M. Lopez; Daniele Gaggero; Daniele Gaggero; L. Freixas Coromina; M. Will; I. Agudo; Maxim V. Barkov; S. Karkar; B. De Lotto; E. Mach; Luca Zampieri; Jürgen Knödlseder; G. Bonnoli; T. Di Girolamo; D. della Volpe; Tarek M. Hassan; A. M. Brown; Anatolii Zenin; Hidetoshi Sano; V. De Caprio; R. Millul; Sebastian Diebold; Julien Lefaucheur; R. J. García López; Marc Ribó; Rodrigo Nemmen; G. Fontaine; S. Flis; G. Emery; T. Tam; Konstantinos N. Gourgouliatos; L. Mohrmann; Nu. Komin; E. Fedorova; C. Alispach; Z. Ou; Juan Cortina; Takashi Saito; Elena Amato; Elisabetta Bissaldi; Shanta M. Zimmer; J. Gironnet; G. Pareschi; Sylvain Chaty; S. Vercellone; Maria Magdalena González; I. Oya; Heide Costantini; Daniel Nieto; Marek Nikolajuk; Farinaldo S. Queiroz; Jonathan S. Lapington; M. Perri; J. Becerra González; B. Khélifi; L. Di Venere; Juan Abel Barrio; A. Rugliancich; Łukasz Stawarz; E. O. Angüner; E. de Oña Wilhelmi; T. Nagayoshi; N. Parmiggiani; Miroslav Hrabovsky; D. de Martino; T. Montaruli; Thomas Murach; M. Iori; Vincenzo Testa; Bohdan Hnatyk; M. Fiori; Lenka Tomankova; Juan Carlos Rodríguez-Ramírez; Reiko Orito; Petr Janecek; Satoshi Fukami; David A. Williams; A. Burtovoi; Enrico Cascone; Reshmi Mukherjee; Etienne Lyard; Marcello Giroletti; Petar Temnikov; F. Salesa Greus; Q. Feng; R. Paoletti; Diego Falceta-Gonçalves; Stefan Kimeswenger; A. Kong; L. P. Taylor; Daniela Maria Ribeiro; Philip Kaaret; G. Morlino; R. D. Parsons; D. Nosek; Michael Zacharias; I. Sadeh; Fabio Iocco; Hidetoshi Kubo; M. Hayashida; N. Hiroshima; Rodrigo Guedes Lang; Martin Pohl; M. Vecchi; M. Vecchi; M. Nievas Rosillo; Fulvio Gianotti; A. Fiasson; M. Garczarczyk; F. Arqueros; N. Produit; A. Morselli; Thomas Lohse; Francesco Longo; D. Dominis Prester; Manuel Meyer; M. Zavrtanik; Matteo Cerruti; Enrico Congiu; J. Kushida; Jakub Juryšek; Jakub Juryšek; Paramita Barai; Agnieszka Slowikowska; Y. Kobayashi; Ermanno Pietropaolo; Q. Piel; L. Tosti; B. Bertucci; Michael G. Burton; J. M. Paredes;doi: 10.1016/j.astropartphys.2019.04.001 , 10.3204/pubdb-2019-02176 , 10.48550/arxiv.1904.01426 , 10.5167/uzh-185554
handle: 2066/204317 , https://repository.ubn.ru.nl/handle/2066/204317 , 11588/836701 , 11588/1002980 , 11368/2948845 , 11245.1/15060f98-9266-4cbe-b13f-d5eb36bfca84 , 11370/56c95366-7d1c-41bc-8642-89d81f7b2d08 , 20.500.14243/384369 , 10261/189767 , 11365/1082110 , 11449/188943 , 20.500.12556/RUNG-4481-6fc900a7-bfd6-9d11-ce01-125b62caf538 , 11577/3303347 , 11390/1148589 , 11578/310854 , 11573/1279912 , 11568/1151989 , 11589/176927 , 11391/1449632 , 11697/136912 , 11587/447196 , 2158/1353568 , 2318/1771875 , 11586/348637 , 2440/121474 , 10900/99174
doi: 10.1016/j.astropartphys.2019.04.001 , 10.3204/pubdb-2019-02176 , 10.48550/arxiv.1904.01426 , 10.5167/uzh-185554
handle: 2066/204317 , https://repository.ubn.ru.nl/handle/2066/204317 , 11588/836701 , 11588/1002980 , 11368/2948845 , 11245.1/15060f98-9266-4cbe-b13f-d5eb36bfca84 , 11370/56c95366-7d1c-41bc-8642-89d81f7b2d08 , 20.500.14243/384369 , 10261/189767 , 11365/1082110 , 11449/188943 , 20.500.12556/RUNG-4481-6fc900a7-bfd6-9d11-ce01-125b62caf538 , 11577/3303347 , 11390/1148589 , 11578/310854 , 11573/1279912 , 11568/1151989 , 11589/176927 , 11391/1449632 , 11697/136912 , 11587/447196 , 2158/1353568 , 2318/1771875 , 11586/348637 , 2440/121474 , 10900/99174
The Cherenkov Telescope Array (CTA) is the major next-generation observatory for ground-based very-high-energy gamma-ray astronomy. It will improve the sensitivity of current ground-based instruments by a factor of five to twenty, depending on the energy, greatly improving both their angular and energy resolutions over four decades in energy (from 20 GeV to 300 TeV). This achievement will be possible by using tens of imaging Cherenkov telescopes of three successive sizes. They will be arranged into two arrays, one per hemisphere, located on the La Palma island (Spain) and in Paranal (Chile). We present here the optimised and final telescope arrays for both CTA sites, as well as their foreseen performance, resulting from the analysis of three different large-scale Monte Carlo productions. Astroparticle physics 111, 35 - 53 (2019). doi:10.1016/j.astropartphys.2019.04.001 Published by Elsevier Science, Amsterdam [u.a.]
CORE arrow_drop_down Usiena air - Università di SienaArticle . 2019License: CC BY NC NDData sources: Usiena air - Università di SienaArchivio istituzionale della ricerca - Università IUAV di VeneziaArticle . 2019License: CC BY NC NDUniversità degli Studi di Siena: USiena airArticle . 2019Full-Text: http://hdl.handle.net/11365/1082110Data sources: Bielefeld Academic Search Engine (BASE)Universidade Estadual Paulista São Paulo: Repositório Institucional UNESPArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Croatian Scientific Bibliography - CROSBIArticle . 2019Data sources: Croatian Scientific Bibliography - CROSBIRecolector de Ciencia Abierta, RECOLECTAArticle . 2019Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2019 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2019 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle PhysicsArticle . 2019License: CC BY NC SAData sources: Universiteit van Amsterdam Digital Academic RepositoryAstroparticle PhysicsArticle . 2019License: taverneData sources: University of Groningen Research PortalUniversity of Bath's research portalArticle . 2019Data sources: University of Bath's research portalOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2019Data sources: OA@INAF - Istituto Nazionale di AstrofisicaUniversiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2019Data sources: Bielefeld Academic Search Engine (BASE)Zurich Open Repository and ArchiveArticle . 2019 . Peer-reviewedData sources: Zurich Open Repository and ArchiveRepository of University of Nova GoricaArticle . 2019Data sources: Repository of University of Nova GoricaArchivio della Ricerca - Università di PisaArticle . 2019Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2019Flore (Florence Research Repository)Article . 2019Data sources: Flore (Florence Research Repository)Università degli Studi di Bari Aldo Moro: CINECA IRISArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2019Data sources: Bielefeld Academic Search Engine (BASE)Pontificia Universidad Católica de Chile: Repositorio UCArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)University of Western Sydney (UWS): Research DirectArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Institut National de la Recherche Agronomique: ProdINRAArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: HALArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)The University of Adelaide: Digital LibraryArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Eberhard Karls University Tübingen: Publication SystemArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2019Data 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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For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 40 citations 40 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!
visibility 79visibility views 79 download downloads 124 Powered bymore_vert CORE arrow_drop_down Usiena air - Università di SienaArticle . 2019License: CC BY NC NDData sources: Usiena air - Università di SienaArchivio istituzionale della ricerca - Università IUAV di VeneziaArticle . 2019License: CC BY NC NDUniversità degli Studi di Siena: USiena airArticle . 2019Full-Text: http://hdl.handle.net/11365/1082110Data sources: Bielefeld Academic Search Engine (BASE)Universidade Estadual Paulista São Paulo: Repositório Institucional UNESPArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Croatian Scientific Bibliography - CROSBIArticle . 2019Data sources: Croatian Scientific Bibliography - CROSBIRecolector de Ciencia Abierta, RECOLECTAArticle . 2019Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2019 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticle . 2019 . Peer-reviewedData sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle PhysicsArticle . 2019License: CC BY NC SAData sources: Universiteit van Amsterdam Digital Academic RepositoryAstroparticle PhysicsArticle . 2019License: taverneData sources: University of Groningen Research PortalUniversity of Bath's research portalArticle . 2019Data sources: University of Bath's research portalOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2019Data sources: OA@INAF - Istituto Nazionale di AstrofisicaUniversiteit van Amsterdam: Digital Academic Repository (UvA DARE)Article . 2019Data sources: Bielefeld Academic Search Engine (BASE)Zurich Open Repository and ArchiveArticle . 2019 . Peer-reviewedData sources: Zurich Open Repository and ArchiveRepository of University of Nova GoricaArticle . 2019Data sources: Repository of University of Nova GoricaArchivio della Ricerca - Università di PisaArticle . 2019Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2019Flore (Florence Research Repository)Article . 2019Data sources: Flore (Florence Research Repository)Università degli Studi di Bari Aldo Moro: CINECA IRISArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Université Savoie Mont Blanc: HALArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Archive de l'Observatoire de Paris (HAL)Article . 2019Data sources: Bielefeld Academic Search Engine (BASE)Pontificia Universidad Católica de Chile: Repositorio UCArticle . 2021Data sources: Bielefeld Academic Search Engine (BASE)University of Western Sydney (UWS): Research DirectArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Institut National de la Recherche Agronomique: ProdINRAArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)École Polytechnique, Université Paris-Saclay: HALArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)The University of Adelaide: Digital LibraryArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Eberhard Karls University Tübingen: Publication SystemArticle . 2019Data sources: Bielefeld Academic Search Engine (BASE)Institut national des sciences de l'Univers: HAL-INSUArticle . 2019Data 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.
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For further information contact us at helpdesk@openaire.eudescription 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 , Journal 2004 ItalyPublisher:American Astronomical Society Papini P.; Piccardi S.; Spillantini P.; Vannuccini E.; Ambriola M.; Bellotti R.; Cafagna F.; Ciacio F.; Circella M.; De Marzo C. N.; Bartalucci S.; Ricci M.; Bergström D.; Carlson P.; Francke T.; Hansen P.; Mocchiutti E.; Boezio M.; Bonvicini V.; Schiavon P.; Vacchi A.; Zampa N.; Bravar U.; Stochaj S. J.; Casolino M.; De Pascale M. P.; Morselli A.; Picozza P.; Sparvoli R.; Hof M.; Kremer J.; Menn W.; Simon M.; Mitchell J. W.; Ormes J. F.; Stephens S. A.; Streitmatter R. E.; Suffert M.;doi: 10.1086/424027
handle: 11368/1909078 , 11390/1125294
We report the first measurement of the deuterium abundance in cosmic rays above 10 GeV nucleon � 1 of kinetic energy. The data were collected by the balloon-borne experiment CAPRICE98, which was flown on 1998 May 28–29 from Fort Sumner, New Mexico. The detector configuration included the NMSU-WiZard/CAPRICE superconducting magnet spectrometer equipped with a gas RICH detector, a silicon-tungsten calorimeter, and a time-of-flight system. By combining the information from the spectrometer and the RICH detector, it was possible to separate deuterons from protons in the kinetic energy range from 12 to 22 GeV nucleon � 1 .I n order to estimate the proton background and the deuteron selection efficiency, we developed an empirical model for the response of the instrument, based on the data collected in this experiment. The analysis procedure is described in this paper, and the result on the absolute flux of deuterium is presented. We found that the deuterium abundance at high energy is consistent with the hypothesis that the propagation mechanism of light nuclei is the same as that of heavier secondary components. Subject headings: balloons — cosmic rays — Galaxy: abundances — ISM: abundances
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=10.1086/424027&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 25 citations 25 popularity Top 10% influence Top 10% impulse Average Powered by BIP!
more_vert 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=10.1086/424027&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Conference object , Other literature type 2006 ItalyPublisher:Elsevier BV Claudia Cecchi; Francesca Marcucci; Marco Frailis; Alessandro De Angelis; P. Boinee; F. Gargano; Andrea Lionetto; Gino Tosti; M. Pepe; Luca Latronico; Luca Baldini; P. Lubrano; A. Morselli; Michael Kuss; Gloria Spandre; N. Giglietto; M. N. Mazziotta; Riccardo Rando; Massimo Fiorucci; Nicola Omodei; Denis Bastieri; G. Cabras; R. Giannitrapani; Dario Favretto; Dario Favretto; M. Razzano; Edoardo Milotti; M. Brigida; F. Loparco; Francesco Longo;handle: 11368/2338341 , 11577/2828999 , 11390/858636 , 11568/108568 , 11589/14515 , 11391/995277
This paper presents the simulation of the GLAST high energy gamma-ray telescope. The simulation package, written in C++, is based on the Geant4 toolkit, and it is integrated into a general framework used to process events. A detailed simulation of the electronic signals inside Silicon detectors has been provided and it is used for the particle tracking, which is handled by a dedicated software. A unique repository for the geometrical description of the detector has been realized using the XML language and a C++ library to access this information has been designed and implemented. As first application of the GLAST LAT software, one day of simulated data has been produced. This paper outlines the contribution developed by the Italian GLAST software group.
Open Access Reposito... arrow_drop_down Nuclear Physics B - Proceedings SupplementsArticle . 2006 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefArchivio istituzionale della ricerca - Università di TriesteConference object . 2006Archivio della Ricerca - Università di PisaConference object . 2006Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale della Ricerca - Politecnico di BariConference object . 2006Archivio istituzionale della ricerca - Università di TriesteConference object . 2006add 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=10.1016/j.nuclphysbps.2005.04.062&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen 3 citations 3 popularity Average influence Average impulse Average Powered by BIP!
more_vert Open Access Reposito... arrow_drop_down Nuclear Physics B - Proceedings SupplementsArticle . 2006 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefArchivio istituzionale della ricerca - Università di TriesteConference object . 2006Archivio della Ricerca - Università di PisaConference object . 2006Data sources: Archivio della Ricerca - Università di PisaArchivio Istituzionale della Ricerca - Politecnico di BariConference object . 2006Archivio istituzionale della ricerca - Università di TriesteConference object . 2006add 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=10.1016/j.nuclphysbps.2005.04.062&type=result"></script>'); --> </script>
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