1 Ocak 2017 Konferans bildirisi Açık Erişim

Bhattacharjee, Pooja; Majumdar, Pratik; Ergin, Tulun; Saha, Lab; Joarder, Partha S.

Dublin Core

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  <dc:creator>Bhattacharjee, Pooja</dc:creator>
  <dc:creator>Majumdar, Pratik</dc:creator>
  <dc:creator>Ergin, Tulun</dc:creator>
  <dc:creator>Saha, Lab</dc:creator>
  <dc:creator>Joarder, Partha S.</dc:creator>
  <dc:date>2017-01-01</dc:date>
  <dc:description>We investigate the supernova remnant (SNR) 3C 397 and its neighboring pulsar PSR J1906+0722 in high energy gamma rays by using nearly six years of archival data of Large Area Telescope on board Fermi Gamma Ray Space Telescope (Fermi-LAT). The off-pulse analysis of gamma-ray flux from the location of PSR J1906+0722 reveals an excess emission which is found to be very close to the radio location of 3C 397. Here, we present the preliminary results of this gamma-ray analysis of 3C 397 and PSR J1906+0722.</dc:description>
  <dc:identifier>https://aperta.ulakbim.gov.trrecord/97951</dc:identifier>
  <dc:identifier>oai:zenodo.org:97951</dc:identifier>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>http://www.opendefinition.org/licenses/cc-by</dc:rights>
  <dc:title>Investigating the region of 3C 397 in High Energy Gamma rays</dc:title>
  <dc:type>info:eu-repo/semantics/conferencePaper</dc:type>
  <dc:type>publication-conferencepaper</dc:type>
</oai_dc:dc>