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Investigating the region of 3C 397 in High Energy Gamma rays

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


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{
  "@context": "https://schema.org/", 
  "@id": 97951, 
  "@type": "ScholarlyArticle", 
  "creator": [
    {
      "@type": "Person", 
      "name": "Bhattacharjee, Pooja"
    }, 
    {
      "@type": "Person", 
      "affiliation": "HBNI, Saha Inst Nucl Phys, 1-AF Bidhannagar, Kolkata 700064, India", 
      "name": "Majumdar, Pratik"
    }, 
    {
      "@type": "Person", 
      "affiliation": "TUBITAK Space Technol Res Inst, ODTU Campus, TR-06800 Ankara, Turkey", 
      "name": "Ergin, Tulun"
    }, 
    {
      "@type": "Person", 
      "affiliation": "Univ Complutense, E-28040 Madrid, Spain", 
      "name": "Saha, Lab"
    }, 
    {
      "@type": "Person", 
      "name": "Joarder, Partha S."
    }
  ], 
  "datePublished": "2017-01-01", 
  "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.", 
  "headline": "Investigating the region of 3C 397 in High Energy Gamma rays", 
  "identifier": 97951, 
  "image": "https://aperta.ulakbim.gov.tr/static/img/logo/aperta_logo_with_icon.svg", 
  "license": "http://www.opendefinition.org/licenses/cc-by", 
  "name": "Investigating the region of 3C 397 in High Energy Gamma rays", 
  "url": "https://aperta.ulakbim.gov.tr/record/97951"
}
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