1 Ocak 2014 Konferans bildirisi Açık Erişim

Saha, Lab; Ergin, Tulun; Majumdar, Pratik; Bozkurt, Mustafa

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{
  "@context": "https://schema.org/", 
  "@id": 99673, 
  "@type": "ScholarlyArticle", 
  "creator": [
    {
      "@type": "Person", 
      "affiliation": "Saha Inst Nucl Phys, Kolkata 700064, India", 
      "name": "Saha, Lab"
    }, 
    {
      "@type": "Person", 
      "affiliation": "Tubitak Space Technol Res Inst, TR-06531 Ankara, Turkey", 
      "name": "Ergin, Tulun"
    }, 
    {
      "@type": "Person", 
      "affiliation": "Saha Inst Nucl Phys, Kolkata 700064, India", 
      "name": "Majumdar, Pratik"
    }, 
    {
      "@type": "Person", 
      "affiliation": "Bogazici Univ, Phys Dept, TR-34134 Istanbul, Turkey", 
      "name": "Bozkurt, Mustafa"
    }
  ], 
  "datePublished": "2014-01-01", 
  "description": "We have analyzed Chandra X-ray data from different parts of the shell of young supernova remnant (SNR) in the energy range of 0.7 - 8 keV. We observed that X-ray flux level varies over different shell regions of the source. Implications of X-ray observation will be discussed here. We also analyzed Fermi-LAT data in the energy range 0.5 - 50 GeV for the source. The differential spectrum obtained in this way fits with simple power-law. We also present here multi-wavelength modeling of the source considering archival radio and TeV data along with Chandra and Fermi-LAT data.", 
  "headline": "Locating the TeV gamma-rays from the shell regions of Cassiopeia A", 
  "identifier": 99673, 
  "image": "https://aperta.ulakbim.gov.tr/static/img/logo/aperta_logo_with_icon.svg", 
  "license": "http://www.opendefinition.org/licenses/cc-by", 
  "name": "Locating the TeV gamma-rays from the shell regions of Cassiopeia A", 
  "url": "https://aperta.ulakbim.gov.tr/record/99673"
}