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...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:arXiv.org 2015-11
Hauptverfasser: 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
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue
container_start_page
container_title arXiv.org
container_volume
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
fullrecord <record><control><sourceid>proquest_arxiv</sourceid><recordid>TN_cdi_arxiv_primary_1511_06778</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2079097047</sourcerecordid><originalsourceid>FETCH-LOGICAL-a527-39052a19097fffa388f32bf3b4acfda4f2e02039d7d39f79e0e5f5c636f7a91f3</originalsourceid><addsrcrecordid>eNotj0tLw0AUhQdBsNT-AFcOuJTEO3MzmcxSglWhIGj24baZqynNw0lS9N_bh6uz-TjnfELcKIiTzBh4oPBT72NllIohtTa7EDONqKIs0fpKLIZhCwA6tdoYnIn74stLNYxy6UNTyxWN8mPqfWi7Pcl337TUjjKnkXbd57W4ZNoNfvGfc1Esn4r8JVq9Pb_mj6uIjLYROjCalANnmZkwyxj1mnGd0IYrSlh70ICushU6ts6DN2w2KaZsySnGubg9155Myj7UDYXf8mhUnowOxN2Z6EP3PflhLLfdFNrDp1KDPS5DYvEPZf9Mdg</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2079097047</pqid></control><display><type>article</type><title>The 1st Fermi Lat Supernova Remnant Catalog</title><source>Freely Accessible Journals</source><source>arXiv.org</source><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</creator><creatorcontrib>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</creatorcontrib><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><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, Tom</creator><creator>Grenier, I A</creator><creator>Horan, Deirdre</creator><creator>Hou, X</creator><creator>Iafrate, Giulia</creator><creator>Jogler, Tobias</creator><creator>Katagiri, Hideaki</creator><creator>Katsuta, Junichiro</creator><creator>Kerr, Matthew</creator><creator>Laffon, Helene</creator><creator>Latronico, Luca</creator><creator>J Li</creator><creator>L Li</creator><creator>Loparco, Francesco</creator><creator>Lovellette, Michael N</creator><creator>Lubrano, Pasquale</creator><creator>Magill, J</creator><creator>Marelli, Martino</creator><creator>Mayer, Michael</creator><creator>Mazziotta, M N</creator><creator>Michelson, Peter F</creator><creator>Mizuno, Tsunefumi</creator><creator>Moiseev, Alexander A</creator><creator>Monzani, Maria Elena</creator><creator>Moretti, E</creator><creator>Morselli, Aldo</creator><creator>Moskalenko, Igor V</creator><creator>Murgia, Simona</creator><creator>Orienti, Monica</creator><creator>Orlando, Elena</creator><creator>Ormes, Jonathan F</creator><creator>Paneque, David</creator><creator>Perkins, J S</creator><creator>Pesce-Rollins, Melissa</creator><creator>Pivato, Giovanna</creator><creator>Porter, Troy</creator><creator>S Rain`o</creator><creator>Razzano, Massimiliano</creator><creator>Razzaque, Soebur</creator><creator>Reimer, Olaf</creator><creator>Renaud, Matthieu</creator><creator>Reposeur, Thierry</creator><creator>Rousseau, Romain</creator><creator>Schmid, J</creator><creator>C Sgr`o</creator><creator>Siskind, Eric J</creator><creator>Spada, Francesca</creator><creator>Strong, Andrew W</creator><creator>Tajima, Hiro</creator><creator>Takahashi, Hiromitsu</creator><creator>Tanaka, T</creator><creator>Tibaldo, L</creator><creator>Tibolla, Omar</creator><creator>Prof Diego F Torres</creator><creator>Tosti, Gino</creator><creator>Troja, Eleonora</creator><creator>Uchiyama, Yasunobu</creator><creator>Vianello, G</creator><creator>Wells, B</creator><creator>Wood, Kent</creator><creator>Wood, 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 &amp; 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
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-12T19%3A36%3A04IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%201st%20Fermi%20Lat%20Supernova%20Remnant%20Catalog&rft.jtitle=arXiv.org&rft.au=Acero,%20Fabio&rft.date=2015-11-20&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.1511.06778&rft_dat=%3Cproquest_arxiv%3E2079097047%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2079097047&rft_id=info:pmid/&rfr_iscdi=true