The Swift-XRT Deep Serendipitous Survey

この論文をさがす

説明

The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan

The Swift-XRT Deep Serendipitous Survey is a large ( approximately 32.5 deg.(sup 2)) rather deep ( 0.5 - 2 keV flux limit approximately 7 x 10(sup -16) erg cm(sup -2) s(sup -1)) X-ray survey obtained by searching for serendipitous sources around 372 Gamma Ray Burst (GRB) observed with the XRT telescope on board of the Swift satellite, from January 2005 to December 2008. Here, we report on the strategy, design and execution of the survey, and we present first results on the catalog of point-like X-ray sources detected in the observations carried out between January 2005 to June 2007 (237 fields). For the high Galactic latitude fields (i.e. absolute value of b > = 20 deg.), we also present the X-ray number counts (i.e. LogN-LogS), that is consistent with previous results.

Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science

資料番号: AA0064574154

レポート番号: JAXA-SP-09-008E

収録刊行物

詳細情報 詳細情報について

  • CRID
    1050292561218726912
  • NII論文ID
    120006828556
  • NII書誌ID
    AA11984031
  • ISSN
    1349113X
  • Web Site
    http://id.nii.ac.jp/1696/00005080/
  • 本文言語コード
    en
  • 資料種別
    conference paper
  • データソース種別
    • IRDB
    • CiNii Articles

問題の指摘

ページトップへ