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Volumn 325, Issue 5942, 2009, Pages 840-844

Detection of 16 gamma-ray pulsars through blind frequency searches using the Fermi LAT

(179)  Abdo, A A a   Ackermann, M b   Ajello, M b   Anderson, B c   Atwood, W B c   Axelsson, M d,e   Baldini, L f   Ballet, J g   Barbiellini, G h,i   Baring, M G j   Bastieri, D k,l   Baughman, B M m   Bechtol, K b   Bellazzini, R f   Berenji, B b   Bignami, G F n   Blandford, R D b   Bloom, E D b   Bonamente, E o,p   Borgland, A W b   more..


Author keywords

[No Author keywords available]

Indexed keywords

DETECTION METHOD; ENERGETICS; GAMMA RAY RADIATION; RADIATIVE TRANSFER;

EID: 68949203700     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1175558     Document Type: Article
Times cited : (399)

References (40)
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    • Abdo, A.A.1
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    • (2009)
  • 18
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    • thesis, Harvard University
    • S. M. Ransom, thesis, Harvard University (2001).
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    • Ransom, S.M.1
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    • published online 16 October 2008 (10.1126/science.1165572)
    • A. A. Abdo et al., Science 322, 1218 (2008); published online 16 October 2008 (10.1126/science.1165572).
    • (2008) Science , vol.322 , pp. 1218
    • Abdo, A.A.1
  • 40
    • 68949210242 scopus 로고    scopus 로고
    • note
    • The Fermi LAT Collaboration is supported by NASA and the U.S. Department of Energy; the Commissariat à l'Energie Atomique and CNRS/Institut National de Physique Nucléaire et de Physique des Particules (France); the Agenzia Spaziale Italiana, Istituto Nazionale di Fisica Nucleare, and Istituto Nazionale di Astrofisica (Italy); the Ministry of Education, Culture, Sports, Science and Technology, High Energy Accelerator Research Organization (KEK), and Japan Aerospace Exploration Agency (Japan); and the K. A. Wallenberg Foundation, Swedish Research Council, and National Space Board (Sweden). Much of this work was carried out on the Pleiades supercomputer at the Department of Astronomy, University of California, Santa Cruz. This work made extensive use of the ATNF pulsar database. We thank N. Gehrels for granting Swift/XRT time to explore the LAT error circles, the Swift MOC staff for performing the observations, F. Camilo and S. Ransom for contributions, and M. Roberts for useful discussions.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.