The first Fermi LAT SNR catalog (1SC) Virtual Observatory Resource

Authors
  1. Acero F.
  2. Ackermann M.
  3. Ajello M.
  4. Baldini L.
  5. Ballet J.
  6. Barbiellini G.,Bastieri D.
  7. Bellazzini R.
  8. Bissaldi E.
  9. Blandford R.D.
  10. Bloom E.D.,Bonino R.
  11. Bottacini E.
  12. Brandt T.J.
  13. Bregeon J.
  14. Bruel P.
  15. Buehler R.,Buson S.
  16. Caliandro G.A.
  17. Cameron R.A.
  18. Caputo R.
  19. Caragiulo M.,Caraveo P.A.
  20. Casandjian J.M.
  21. Cavazzuti E.
  22. Cecchi C.
  23. Chekhtman A.,Chiang J.
  24. Chiaro G.
  25. Ciprini S.
  26. Claus R.
  27. Cohen J.M.
  28. Cohen-Tanugi J.,Cominsky L.R.
  29. Condon B.
  30. Conrad J.
  31. Cutini S.
  32. D'Ammando F.,de Angelis A.
  33. de Palma F.
  34. Desiante R.
  35. Digel S.W.
  36. Di Venere L.,Drell P.S.
  37. Drlica-Wagner A.
  38. Favuzzi C.
  39. Ferrara E.C.
  40. Franckowiak A.,Fukazawa Y.
  41. Funk S.
  42. Fusco P.
  43. Gargano F.
  44. Gasparrini D.
  45. Giglietto N.,Giommi P.
  46. Giordano F.
  47. Giroletti M.
  48. Glanzman T.
  49. Godfrey G.,Gomez-Vargas G.A.
  50. Grenier I.A.
  51. Grondin M.-H.
  52. Guillemot L.
  53. Guiriec S.,Gustafsson M.
  54. Hadasch D.
  55. Harding A.K.
  56. Hayashida M.
  57. Hays E.,Hewitt J.W.
  58. Hill A.B.
  59. Horan D.
  60. Hou X.
  61. Iafrate G.
  62. Jogler T.,Johannesson G.
  63. Johnson A.S.
  64. Kamae T.
  65. Katagiri H.
  66. Kataoka J.,Katsuta J.
  67. Kerr M.
  68. Knodlseder J.
  69. Kocevski D.
  70. Kuss M.
  71. Laffon H.,Lande J.
  72. Larsson S.
  73. Latronico L.
  74. Lemoine-Goumard M.
  75. Li J.
  76. Li L.,Longo F.
  77. Loparco F.
  78. Lovellette M.N.
  79. Lubrano P.
  80. Magill J.
  81. Maldera S.,Marelli M.
  82. Mayer M.
  83. Mazziotta M.N.
  84. Michelson P.F.
  85. Mitthumsiri W.,Mizuno T.
  86. Moiseev A.A.
  87. Monzani M.E.
  88. Moretti E.
  89. Morselli A.,Moskalenko I.V.
  90. Murgia S.
  91. Nemmen R.
  92. Nuss E.
  93. Ohsugi T.
  94. Omodei N.,Orienti M.
  95. Orlando E.
  96. Ormes J.F.
  97. Paneque D.
  98. Perkins J.S.,Pesce-Rollins M.
  99. Petrosian V.
  100. Piron F.
  101. Pivato G.
  102. Porter T.A.
  103. Raino S.,Rando R.
  104. Razzano M.
  105. Razzaque S.
  106. Reimer A.
  107. Reimer O.
  108. Renaud M.,Reposeur T.
  109. Rousseau R.
  110. Saz Parkinson P.M.
  111. Schmid J.
  112. Schulz A.,Sgro C.
  113. Siskind E.J.
  114. Spada F.
  115. Spandre G.
  116. Spinelli P.
  117. Strong A.W.,Suson D.J.
  118. Tajima H.
  119. Takahashi H.
  120. Tanaka T.
  121. Thayer J.B.
  122. Thompson D.J.,Tibaldo L.
  123. Tibolla O.
  124. Torres D.F.
  125. Tosti G.
  126. Troja E.
  127. Uchiyama Y.,Vianello G.
  128. Wells B.
  129. Wood K.S.
  130. Wood M.
  131. Yassine M.
  132. den Hartog P.R.,Zimmer S.
    133. Published by
    CDS
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 100GeV 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.

Keywords
  1. supernova-remnants
  2. gamma-ray-astronomy
  3. surveys
  4. stellar-distance
Bibliographic source Bibcode
2016ApJS..224....8A
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/224/8
IVOA Identifier IVOID
ivo://CDS.VizieR/J/ApJS/224/8
Document Object Identifer DOI
doi:10.26093/cds/vizier.22240008

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/224/8
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/224/8
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/224/8
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/224/8/catalog?
https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/224/8/catalog?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/224/8/catalog?
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/224/8/mwinfo?
https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/224/8/mwinfo?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/224/8/mwinfo?

History

2016-08-22T09:09:07Z
Resource record created
2016-08-22T09:09:07Z
Created
2018-09-13T08:11:45Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr