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The first fermi lat supernova remnant catalog
KTH, Skolan för teknikvetenskap (SCI), Fysik, Partikel- och astropartikelfysik. AlbaNova, Oskar Klein Ctr Cosmoparticle Phys, Sweden.
KTH, Skolan för teknikvetenskap (SCI), Fysik, Partikel- och astropartikelfysik. AlbaNova, Oskar Klein Ctr Cosmoparticle Phys, Sweden.
Vise andre og tillknytning
Rekke forfattare: 1612016 (engelsk)Inngår i: Astrophysical Journal Supplement Series, ISSN 0067-0049, E-ISSN 1538-4365, Vol. 224, nr 1, artikkel-id 8Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

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 (LAT). 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, we demonstrate 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.

sted, utgiver, år, opplag, sider
Institute of Physics Publishing (IOPP), 2016. Vol. 224, nr 1, artikkel-id 8
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Identifikatorer
URN: urn:nbn:se:kth:diva-189211DOI: 10.3847/0067-0049/224/1/8ISI: 000377050200008Scopus ID: 2-s2.0-84977648287OAI: oai:DiVA.org:kth-189211DiVA, id: diva2:944328
Merknad

QC 20160629

Tilgjengelig fra: 2016-06-29 Laget: 2016-06-29 Sist oppdatert: 2017-11-28bibliografisk kontrollert

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