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description 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.
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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 , 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.
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description 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.
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 , 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.
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