The 1st Fermi Lat Supernova Remnant Catalog
To uniformly determine the properties of supernova remnants (SNRs) at high energies, we have developed the first systematic survey at energies from 1 to 100 GeV using data from the Fermi Large Area Telescope. Based on the spatial overlap of sources detected at GeV energies with SNRs known from radio...
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creator | Acero, Fabio Ackermann, Markus Ajello, Marco Baldini, Luca Ballet, Jean Bellazzini, Ronaldo Bissaldi, E Blandford, Roger Bloom, E D Bonino, Raffaella Bottacini, Eugenio Buson, S Caliandro, G A Cameron, Rob A Caputo, R Caragiulo, Micaela Casandjian, Jean Marc Cecchi, Claudia Chiang, J Ciprini, Stefano Claus, R Cohen, J M Cohen-Tanugi, Johann Cominsky, L R Condon, B D'Ammando, F Angelis, A Digel, S W Venere, L Drell, Persis S Drlica-Wagner, Alex Franckowiak, Anna Funk, Stefan Gargano, Fabio Giglietto, Nicola Giommi, Paolo Giroletti, Marcello Glanzman, Tom Grenier, I A Horan, Deirdre Hou, X Iafrate, Giulia Jogler, Tobias Katagiri, Hideaki Katsuta, Junichiro Kerr, Matthew Laffon, Helene Latronico, Luca J Li L Li Loparco, Francesco Lovellette, Michael N Lubrano, Pasquale Magill, J Marelli, Martino Mayer, Michael Mazziotta, M N Michelson, Peter F Mizuno, Tsunefumi Moiseev, Alexander A Monzani, Maria Elena Moretti, E Morselli, Aldo Moskalenko, Igor V Murgia, Simona Orienti, Monica Orlando, Elena Ormes, Jonathan F Paneque, David Perkins, J S Pesce-Rollins, Melissa Pivato, Giovanna Porter, Troy S Rain`o Razzano, Massimiliano Razzaque, Soebur Reimer, Olaf Renaud, Matthieu Reposeur, Thierry Rousseau, Romain Schmid, J C Sgr`o Siskind, Eric J Spada, Francesca Strong, Andrew W Tajima, Hiro Takahashi, Hiromitsu Tanaka, T Tibaldo, L Tibolla, Omar Prof Diego F Torres Tosti, Gino Troja, Eleonora Uchiyama, Yasunobu Vianello, G Wells, B Wood, Kent Wood, M Yassine, Manal Zimmer, Stephan |
description | To uniformly determine the properties of supernova remnants (SNRs) at high energies, we have developed the first systematic survey at energies from 1 to 100 GeV using data from the Fermi Large Area Telescope. Based on the spatial overlap of sources detected at GeV energies with SNRs known from radio surveys, we classify 30 sources as likely GeV SNRs. We also report 14 marginal associations and 245 flux upper limits. A mock catalog in which the positions of known remnants are scrambled in Galactic longitude, allows us to determine an upper limit of 22% on the number of GeV candidates falsely identified as SNRs. We have also developed a method to estimate spectral and spatial systematic errors arising from the diffuse interstellar emission model, a key component of all Galactic Fermi LAT analyses. By studying remnants uniformly in aggregate, we measure the GeV properties common to these objects and provide a crucial context for the detailed modeling of individual SNRs. Combining our GeV results with multiwavelength (MW) data, including radio, X-ray, and TeV, demonstrates the need for improvements to previously sufficient, simple models describing the GeV and radio emission from these objects. We model the GeV and MW emission from SNRs in aggregate to constrain their maximal contribution to observed Galactic cosmic rays. |
doi_str_mv | 10.48550/arxiv.1511.06778 |
format | Article |
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Based on the spatial overlap of sources detected at GeV energies with SNRs known from radio surveys, we classify 30 sources as likely GeV SNRs. We also report 14 marginal associations and 245 flux upper limits. A mock catalog in which the positions of known remnants are scrambled in Galactic longitude, allows us to determine an upper limit of 22% on the number of GeV candidates falsely identified as SNRs. We have also developed a method to estimate spectral and spatial systematic errors arising from the diffuse interstellar emission model, a key component of all Galactic Fermi LAT analyses. By studying remnants uniformly in aggregate, we measure the GeV properties common to these objects and provide a crucial context for the detailed modeling of individual SNRs. Combining our GeV results with multiwavelength (MW) data, including radio, X-ray, and TeV, demonstrates the need for improvements to previously sufficient, simple models describing the GeV and radio emission from these objects. We model the GeV and MW emission from SNRs in aggregate to constrain their maximal contribution to observed Galactic cosmic rays.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1511.06778</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Cosmic rays ; Emission analysis ; Galactic cosmic rays ; Interstellar ; Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics ; Radio emission ; Radio sources (astronomy) ; Supernova remnants ; Systematic errors</subject><ispartof>arXiv.org, 2015-11</ispartof><rights>2015. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,781,785,886,27930</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.1511.06778$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.3847/0067-0049/224/1/8$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Acero, Fabio</creatorcontrib><creatorcontrib>Ackermann, Markus</creatorcontrib><creatorcontrib>Ajello, Marco</creatorcontrib><creatorcontrib>Baldini, Luca</creatorcontrib><creatorcontrib>Ballet, Jean</creatorcontrib><creatorcontrib>Bellazzini, Ronaldo</creatorcontrib><creatorcontrib>Bissaldi, E</creatorcontrib><creatorcontrib>Blandford, Roger</creatorcontrib><creatorcontrib>Bloom, E D</creatorcontrib><creatorcontrib>Bonino, Raffaella</creatorcontrib><creatorcontrib>Bottacini, Eugenio</creatorcontrib><creatorcontrib>Buson, S</creatorcontrib><creatorcontrib>Caliandro, G A</creatorcontrib><creatorcontrib>Cameron, Rob A</creatorcontrib><creatorcontrib>Caputo, R</creatorcontrib><creatorcontrib>Caragiulo, Micaela</creatorcontrib><creatorcontrib>Casandjian, Jean Marc</creatorcontrib><creatorcontrib>Cecchi, Claudia</creatorcontrib><creatorcontrib>Chiang, J</creatorcontrib><creatorcontrib>Ciprini, Stefano</creatorcontrib><creatorcontrib>Claus, R</creatorcontrib><creatorcontrib>Cohen, J M</creatorcontrib><creatorcontrib>Cohen-Tanugi, Johann</creatorcontrib><creatorcontrib>Cominsky, L R</creatorcontrib><creatorcontrib>Condon, B</creatorcontrib><creatorcontrib>D'Ammando, F</creatorcontrib><creatorcontrib>Angelis, A</creatorcontrib><creatorcontrib>Digel, S W</creatorcontrib><creatorcontrib>Venere, L</creatorcontrib><creatorcontrib>Drell, Persis S</creatorcontrib><creatorcontrib>Drlica-Wagner, Alex</creatorcontrib><creatorcontrib>Franckowiak, Anna</creatorcontrib><creatorcontrib>Funk, Stefan</creatorcontrib><creatorcontrib>Gargano, Fabio</creatorcontrib><creatorcontrib>Giglietto, Nicola</creatorcontrib><creatorcontrib>Giommi, Paolo</creatorcontrib><creatorcontrib>Giroletti, Marcello</creatorcontrib><creatorcontrib>Glanzman, Tom</creatorcontrib><creatorcontrib>Grenier, I A</creatorcontrib><creatorcontrib>Horan, Deirdre</creatorcontrib><creatorcontrib>Hou, X</creatorcontrib><creatorcontrib>Iafrate, Giulia</creatorcontrib><creatorcontrib>Jogler, Tobias</creatorcontrib><creatorcontrib>Katagiri, Hideaki</creatorcontrib><creatorcontrib>Katsuta, Junichiro</creatorcontrib><creatorcontrib>Kerr, Matthew</creatorcontrib><creatorcontrib>Laffon, Helene</creatorcontrib><creatorcontrib>Latronico, Luca</creatorcontrib><creatorcontrib>J Li</creatorcontrib><creatorcontrib>L Li</creatorcontrib><creatorcontrib>Loparco, Francesco</creatorcontrib><creatorcontrib>Lovellette, Michael N</creatorcontrib><creatorcontrib>Lubrano, Pasquale</creatorcontrib><creatorcontrib>Magill, J</creatorcontrib><creatorcontrib>Marelli, Martino</creatorcontrib><creatorcontrib>Mayer, Michael</creatorcontrib><creatorcontrib>Mazziotta, M N</creatorcontrib><creatorcontrib>Michelson, Peter F</creatorcontrib><creatorcontrib>Mizuno, Tsunefumi</creatorcontrib><creatorcontrib>Moiseev, Alexander A</creatorcontrib><creatorcontrib>Monzani, Maria Elena</creatorcontrib><creatorcontrib>Moretti, E</creatorcontrib><creatorcontrib>Morselli, Aldo</creatorcontrib><creatorcontrib>Moskalenko, Igor V</creatorcontrib><creatorcontrib>Murgia, Simona</creatorcontrib><creatorcontrib>Orienti, Monica</creatorcontrib><creatorcontrib>Orlando, Elena</creatorcontrib><creatorcontrib>Ormes, Jonathan F</creatorcontrib><creatorcontrib>Paneque, David</creatorcontrib><creatorcontrib>Perkins, J S</creatorcontrib><creatorcontrib>Pesce-Rollins, Melissa</creatorcontrib><creatorcontrib>Pivato, Giovanna</creatorcontrib><creatorcontrib>Porter, Troy</creatorcontrib><creatorcontrib>S Rain`o</creatorcontrib><creatorcontrib>Razzano, Massimiliano</creatorcontrib><creatorcontrib>Razzaque, Soebur</creatorcontrib><creatorcontrib>Reimer, Olaf</creatorcontrib><creatorcontrib>Renaud, Matthieu</creatorcontrib><creatorcontrib>Reposeur, Thierry</creatorcontrib><creatorcontrib>Rousseau, Romain</creatorcontrib><creatorcontrib>Schmid, J</creatorcontrib><creatorcontrib>C Sgr`o</creatorcontrib><creatorcontrib>Siskind, Eric J</creatorcontrib><creatorcontrib>Spada, Francesca</creatorcontrib><creatorcontrib>Strong, Andrew W</creatorcontrib><creatorcontrib>Tajima, Hiro</creatorcontrib><creatorcontrib>Takahashi, Hiromitsu</creatorcontrib><creatorcontrib>Tanaka, T</creatorcontrib><creatorcontrib>Tibaldo, L</creatorcontrib><creatorcontrib>Tibolla, Omar</creatorcontrib><creatorcontrib>Prof Diego F Torres</creatorcontrib><creatorcontrib>Tosti, Gino</creatorcontrib><creatorcontrib>Troja, Eleonora</creatorcontrib><creatorcontrib>Uchiyama, Yasunobu</creatorcontrib><creatorcontrib>Vianello, G</creatorcontrib><creatorcontrib>Wells, B</creatorcontrib><creatorcontrib>Wood, Kent</creatorcontrib><creatorcontrib>Wood, M</creatorcontrib><creatorcontrib>Yassine, Manal</creatorcontrib><creatorcontrib>Zimmer, Stephan</creatorcontrib><title>The 1st Fermi Lat Supernova Remnant Catalog</title><title>arXiv.org</title><description>To uniformly determine the properties of supernova remnants (SNRs) at high energies, we have developed the first systematic survey at energies from 1 to 100 GeV using data from the Fermi Large Area Telescope. Based on the spatial overlap of sources detected at GeV energies with SNRs known from radio surveys, we classify 30 sources as likely GeV SNRs. We also report 14 marginal associations and 245 flux upper limits. A mock catalog in which the positions of known remnants are scrambled in Galactic longitude, allows us to determine an upper limit of 22% on the number of GeV candidates falsely identified as SNRs. We have also developed a method to estimate spectral and spatial systematic errors arising from the diffuse interstellar emission model, a key component of all Galactic Fermi LAT analyses. By studying remnants uniformly in aggregate, we measure the GeV properties common to these objects and provide a crucial context for the detailed modeling of individual SNRs. Combining our GeV results with multiwavelength (MW) data, including radio, X-ray, and TeV, demonstrates the need for improvements to previously sufficient, simple models describing the GeV and radio emission from these objects. We model the GeV and MW emission from SNRs in aggregate to constrain their maximal contribution to observed Galactic cosmic rays.</description><subject>Cosmic rays</subject><subject>Emission analysis</subject><subject>Galactic cosmic rays</subject><subject>Interstellar</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Radio emission</subject><subject>Radio sources (astronomy)</subject><subject>Supernova remnants</subject><subject>Systematic errors</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotj0tLw0AUhQdBsNT-AFcOuJTEO3MzmcxSglWhIGj24baZqynNw0lS9N_bh6uz-TjnfELcKIiTzBh4oPBT72NllIohtTa7EDONqKIs0fpKLIZhCwA6tdoYnIn74stLNYxy6UNTyxWN8mPqfWi7Pcl337TUjjKnkXbd57W4ZNoNfvGfc1Esn4r8JVq9Pb_mj6uIjLYROjCalANnmZkwyxj1mnGd0IYrSlh70ICushU6ts6DN2w2KaZsySnGubg9155Myj7UDYXf8mhUnowOxN2Z6EP3PflhLLfdFNrDp1KDPS5DYvEPZf9Mdg</recordid><startdate>20151120</startdate><enddate>20151120</enddate><creator>Acero, Fabio</creator><creator>Ackermann, Markus</creator><creator>Ajello, Marco</creator><creator>Baldini, Luca</creator><creator>Ballet, Jean</creator><creator>Bellazzini, Ronaldo</creator><creator>Bissaldi, E</creator><creator>Blandford, Roger</creator><creator>Bloom, E D</creator><creator>Bonino, Raffaella</creator><creator>Bottacini, Eugenio</creator><creator>Buson, S</creator><creator>Caliandro, G A</creator><creator>Cameron, Rob A</creator><creator>Caputo, R</creator><creator>Caragiulo, Micaela</creator><creator>Casandjian, Jean Marc</creator><creator>Cecchi, Claudia</creator><creator>Chiang, J</creator><creator>Ciprini, Stefano</creator><creator>Claus, R</creator><creator>Cohen, J M</creator><creator>Cohen-Tanugi, Johann</creator><creator>Cominsky, L R</creator><creator>Condon, B</creator><creator>D'Ammando, F</creator><creator>Angelis, A</creator><creator>Digel, S W</creator><creator>Venere, L</creator><creator>Drell, Persis S</creator><creator>Drlica-Wagner, Alex</creator><creator>Franckowiak, Anna</creator><creator>Funk, Stefan</creator><creator>Gargano, Fabio</creator><creator>Giglietto, Nicola</creator><creator>Giommi, Paolo</creator><creator>Giroletti, Marcello</creator><creator>Glanzman, 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M</creator><creator>Yassine, Manal</creator><creator>Zimmer, Stephan</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20151120</creationdate><title>The 1st Fermi Lat Supernova Remnant Catalog</title><author>Acero, Fabio ; Ackermann, Markus ; Ajello, Marco ; Baldini, Luca ; Ballet, Jean ; Bellazzini, Ronaldo ; Bissaldi, E ; Blandford, Roger ; Bloom, E D ; Bonino, Raffaella ; Bottacini, Eugenio ; Buson, S ; Caliandro, G A ; Cameron, Rob A ; Caputo, R ; Caragiulo, Micaela ; Casandjian, Jean Marc ; Cecchi, Claudia ; Chiang, J ; Ciprini, Stefano ; Claus, R ; Cohen, J M ; Cohen-Tanugi, Johann ; Cominsky, L R ; Condon, B ; D'Ammando, F ; Angelis, A ; Digel, S W ; Venere, L ; Drell, Persis S ; Drlica-Wagner, Alex ; Franckowiak, Anna ; Funk, Stefan ; Gargano, Fabio ; Giglietto, Nicola ; Giommi, Paolo ; Giroletti, Marcello ; Glanzman, Tom ; Grenier, I A ; Horan, Deirdre ; Hou, X ; Iafrate, Giulia ; Jogler, Tobias ; Katagiri, Hideaki ; Katsuta, Junichiro ; Kerr, Matthew ; Laffon, Helene ; Latronico, Luca ; J Li ; L Li ; Loparco, Francesco ; Lovellette, Michael N ; Lubrano, Pasquale ; Magill, J ; Marelli, Martino ; Mayer, Michael ; Mazziotta, M N ; Michelson, Peter F ; Mizuno, Tsunefumi ; Moiseev, Alexander A ; Monzani, Maria Elena ; Moretti, E ; Morselli, Aldo ; Moskalenko, Igor V ; Murgia, Simona ; Orienti, Monica ; Orlando, Elena ; Ormes, Jonathan F ; Paneque, David ; Perkins, J S ; Pesce-Rollins, Melissa ; Pivato, Giovanna ; Porter, Troy ; S Rain`o ; Razzano, Massimiliano ; Razzaque, Soebur ; Reimer, Olaf ; Renaud, Matthieu ; Reposeur, Thierry ; Rousseau, Romain ; Schmid, J ; C Sgr`o ; Siskind, Eric J ; Spada, Francesca ; Strong, Andrew W ; Tajima, Hiro ; Takahashi, Hiromitsu ; Tanaka, T ; Tibaldo, L ; Tibolla, Omar ; Prof Diego F Torres ; Tosti, Gino ; Troja, Eleonora ; Uchiyama, Yasunobu ; Vianello, G ; Wells, B ; Wood, Kent ; Wood, M ; Yassine, Manal ; Zimmer, Stephan</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a527-39052a19097fffa388f32bf3b4acfda4f2e02039d7d39f79e0e5f5c636f7a91f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Cosmic rays</topic><topic>Emission analysis</topic><topic>Galactic cosmic rays</topic><topic>Interstellar</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Radio emission</topic><topic>Radio sources (astronomy)</topic><topic>Supernova remnants</topic><topic>Systematic errors</topic><toplevel>online_resources</toplevel><creatorcontrib>Acero, Fabio</creatorcontrib><creatorcontrib>Ackermann, Markus</creatorcontrib><creatorcontrib>Ajello, Marco</creatorcontrib><creatorcontrib>Baldini, Luca</creatorcontrib><creatorcontrib>Ballet, Jean</creatorcontrib><creatorcontrib>Bellazzini, Ronaldo</creatorcontrib><creatorcontrib>Bissaldi, E</creatorcontrib><creatorcontrib>Blandford, Roger</creatorcontrib><creatorcontrib>Bloom, E D</creatorcontrib><creatorcontrib>Bonino, Raffaella</creatorcontrib><creatorcontrib>Bottacini, Eugenio</creatorcontrib><creatorcontrib>Buson, S</creatorcontrib><creatorcontrib>Caliandro, G A</creatorcontrib><creatorcontrib>Cameron, Rob A</creatorcontrib><creatorcontrib>Caputo, R</creatorcontrib><creatorcontrib>Caragiulo, Micaela</creatorcontrib><creatorcontrib>Casandjian, Jean Marc</creatorcontrib><creatorcontrib>Cecchi, Claudia</creatorcontrib><creatorcontrib>Chiang, J</creatorcontrib><creatorcontrib>Ciprini, Stefano</creatorcontrib><creatorcontrib>Claus, R</creatorcontrib><creatorcontrib>Cohen, J M</creatorcontrib><creatorcontrib>Cohen-Tanugi, Johann</creatorcontrib><creatorcontrib>Cominsky, L R</creatorcontrib><creatorcontrib>Condon, B</creatorcontrib><creatorcontrib>D'Ammando, F</creatorcontrib><creatorcontrib>Angelis, A</creatorcontrib><creatorcontrib>Digel, S W</creatorcontrib><creatorcontrib>Venere, L</creatorcontrib><creatorcontrib>Drell, Persis S</creatorcontrib><creatorcontrib>Drlica-Wagner, Alex</creatorcontrib><creatorcontrib>Franckowiak, Anna</creatorcontrib><creatorcontrib>Funk, Stefan</creatorcontrib><creatorcontrib>Gargano, Fabio</creatorcontrib><creatorcontrib>Giglietto, Nicola</creatorcontrib><creatorcontrib>Giommi, Paolo</creatorcontrib><creatorcontrib>Giroletti, Marcello</creatorcontrib><creatorcontrib>Glanzman, Tom</creatorcontrib><creatorcontrib>Grenier, I A</creatorcontrib><creatorcontrib>Horan, Deirdre</creatorcontrib><creatorcontrib>Hou, X</creatorcontrib><creatorcontrib>Iafrate, Giulia</creatorcontrib><creatorcontrib>Jogler, Tobias</creatorcontrib><creatorcontrib>Katagiri, Hideaki</creatorcontrib><creatorcontrib>Katsuta, Junichiro</creatorcontrib><creatorcontrib>Kerr, Matthew</creatorcontrib><creatorcontrib>Laffon, Helene</creatorcontrib><creatorcontrib>Latronico, Luca</creatorcontrib><creatorcontrib>J Li</creatorcontrib><creatorcontrib>L Li</creatorcontrib><creatorcontrib>Loparco, Francesco</creatorcontrib><creatorcontrib>Lovellette, Michael N</creatorcontrib><creatorcontrib>Lubrano, Pasquale</creatorcontrib><creatorcontrib>Magill, J</creatorcontrib><creatorcontrib>Marelli, Martino</creatorcontrib><creatorcontrib>Mayer, Michael</creatorcontrib><creatorcontrib>Mazziotta, M N</creatorcontrib><creatorcontrib>Michelson, Peter F</creatorcontrib><creatorcontrib>Mizuno, Tsunefumi</creatorcontrib><creatorcontrib>Moiseev, Alexander A</creatorcontrib><creatorcontrib>Monzani, Maria Elena</creatorcontrib><creatorcontrib>Moretti, E</creatorcontrib><creatorcontrib>Morselli, Aldo</creatorcontrib><creatorcontrib>Moskalenko, Igor V</creatorcontrib><creatorcontrib>Murgia, Simona</creatorcontrib><creatorcontrib>Orienti, Monica</creatorcontrib><creatorcontrib>Orlando, Elena</creatorcontrib><creatorcontrib>Ormes, Jonathan F</creatorcontrib><creatorcontrib>Paneque, David</creatorcontrib><creatorcontrib>Perkins, J S</creatorcontrib><creatorcontrib>Pesce-Rollins, Melissa</creatorcontrib><creatorcontrib>Pivato, Giovanna</creatorcontrib><creatorcontrib>Porter, Troy</creatorcontrib><creatorcontrib>S Rain`o</creatorcontrib><creatorcontrib>Razzano, Massimiliano</creatorcontrib><creatorcontrib>Razzaque, Soebur</creatorcontrib><creatorcontrib>Reimer, Olaf</creatorcontrib><creatorcontrib>Renaud, Matthieu</creatorcontrib><creatorcontrib>Reposeur, Thierry</creatorcontrib><creatorcontrib>Rousseau, Romain</creatorcontrib><creatorcontrib>Schmid, J</creatorcontrib><creatorcontrib>C Sgr`o</creatorcontrib><creatorcontrib>Siskind, Eric J</creatorcontrib><creatorcontrib>Spada, Francesca</creatorcontrib><creatorcontrib>Strong, Andrew W</creatorcontrib><creatorcontrib>Tajima, Hiro</creatorcontrib><creatorcontrib>Takahashi, Hiromitsu</creatorcontrib><creatorcontrib>Tanaka, T</creatorcontrib><creatorcontrib>Tibaldo, L</creatorcontrib><creatorcontrib>Tibolla, Omar</creatorcontrib><creatorcontrib>Prof Diego F Torres</creatorcontrib><creatorcontrib>Tosti, Gino</creatorcontrib><creatorcontrib>Troja, Eleonora</creatorcontrib><creatorcontrib>Uchiyama, Yasunobu</creatorcontrib><creatorcontrib>Vianello, G</creatorcontrib><creatorcontrib>Wells, B</creatorcontrib><creatorcontrib>Wood, Kent</creatorcontrib><creatorcontrib>Wood, M</creatorcontrib><creatorcontrib>Yassine, Manal</creatorcontrib><creatorcontrib>Zimmer, Stephan</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Access via ProQuest (Open Access)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Acero, Fabio</au><au>Ackermann, Markus</au><au>Ajello, Marco</au><au>Baldini, Luca</au><au>Ballet, Jean</au><au>Bellazzini, Ronaldo</au><au>Bissaldi, E</au><au>Blandford, Roger</au><au>Bloom, E D</au><au>Bonino, Raffaella</au><au>Bottacini, Eugenio</au><au>Buson, S</au><au>Caliandro, G A</au><au>Cameron, Rob A</au><au>Caputo, R</au><au>Caragiulo, Micaela</au><au>Casandjian, Jean Marc</au><au>Cecchi, Claudia</au><au>Chiang, J</au><au>Ciprini, Stefano</au><au>Claus, R</au><au>Cohen, J M</au><au>Cohen-Tanugi, Johann</au><au>Cominsky, L R</au><au>Condon, B</au><au>D'Ammando, F</au><au>Angelis, A</au><au>Digel, S W</au><au>Venere, L</au><au>Drell, Persis S</au><au>Drlica-Wagner, Alex</au><au>Franckowiak, Anna</au><au>Funk, Stefan</au><au>Gargano, Fabio</au><au>Giglietto, Nicola</au><au>Giommi, Paolo</au><au>Giroletti, Marcello</au><au>Glanzman, Tom</au><au>Grenier, I A</au><au>Horan, Deirdre</au><au>Hou, X</au><au>Iafrate, Giulia</au><au>Jogler, Tobias</au><au>Katagiri, Hideaki</au><au>Katsuta, Junichiro</au><au>Kerr, Matthew</au><au>Laffon, Helene</au><au>Latronico, Luca</au><au>J Li</au><au>L Li</au><au>Loparco, Francesco</au><au>Lovellette, Michael N</au><au>Lubrano, Pasquale</au><au>Magill, J</au><au>Marelli, Martino</au><au>Mayer, Michael</au><au>Mazziotta, M N</au><au>Michelson, Peter F</au><au>Mizuno, Tsunefumi</au><au>Moiseev, Alexander A</au><au>Monzani, Maria Elena</au><au>Moretti, E</au><au>Morselli, Aldo</au><au>Moskalenko, Igor V</au><au>Murgia, Simona</au><au>Orienti, Monica</au><au>Orlando, Elena</au><au>Ormes, Jonathan F</au><au>Paneque, David</au><au>Perkins, J S</au><au>Pesce-Rollins, Melissa</au><au>Pivato, Giovanna</au><au>Porter, Troy</au><au>S Rain`o</au><au>Razzano, Massimiliano</au><au>Razzaque, Soebur</au><au>Reimer, Olaf</au><au>Renaud, Matthieu</au><au>Reposeur, Thierry</au><au>Rousseau, Romain</au><au>Schmid, J</au><au>C Sgr`o</au><au>Siskind, Eric J</au><au>Spada, Francesca</au><au>Strong, Andrew W</au><au>Tajima, Hiro</au><au>Takahashi, Hiromitsu</au><au>Tanaka, T</au><au>Tibaldo, L</au><au>Tibolla, Omar</au><au>Prof Diego F Torres</au><au>Tosti, Gino</au><au>Troja, Eleonora</au><au>Uchiyama, Yasunobu</au><au>Vianello, G</au><au>Wells, B</au><au>Wood, Kent</au><au>Wood, M</au><au>Yassine, Manal</au><au>Zimmer, Stephan</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The 1st Fermi Lat Supernova Remnant Catalog</atitle><jtitle>arXiv.org</jtitle><date>2015-11-20</date><risdate>2015</risdate><eissn>2331-8422</eissn><abstract>To uniformly determine the properties of supernova remnants (SNRs) at high energies, we have developed the first systematic survey at energies from 1 to 100 GeV using data from the Fermi Large Area Telescope. Based on the spatial overlap of sources detected at GeV energies with SNRs known from radio surveys, we classify 30 sources as likely GeV SNRs. We also report 14 marginal associations and 245 flux upper limits. A mock catalog in which the positions of known remnants are scrambled in Galactic longitude, allows us to determine an upper limit of 22% on the number of GeV candidates falsely identified as SNRs. We have also developed a method to estimate spectral and spatial systematic errors arising from the diffuse interstellar emission model, a key component of all Galactic Fermi LAT analyses. By studying remnants uniformly in aggregate, we measure the GeV properties common to these objects and provide a crucial context for the detailed modeling of individual SNRs. Combining our GeV results with multiwavelength (MW) data, including radio, X-ray, and TeV, demonstrates the need for improvements to previously sufficient, simple models describing the GeV and radio emission from these objects. We model the GeV and MW emission from SNRs in aggregate to constrain their maximal contribution to observed Galactic cosmic rays.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1511.06778</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2015-11 |
issn | 2331-8422 |
language | eng |
recordid | cdi_arxiv_primary_1511_06778 |
source | Freely Accessible Journals; arXiv.org |
subjects | Cosmic rays Emission analysis Galactic cosmic rays Interstellar Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Radio emission Radio sources (astronomy) Supernova remnants Systematic errors |
title | The 1st Fermi Lat Supernova Remnant Catalog |
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