Suzaku observation of the new Soft Gamma Repeater SGR 0501+4516 in outburst

Authors
  • D. Götz
  • K. Hurley
  • G.L. Israel
  • M. Kokubun
  • K. Makishima
  • S. Mereghetti
  • H. Murakami
  • K. Nakazawa
  • T. Sakamoto
  • L. Stella
  • A. Tiengo
  • R. Turolla
  • S. Yamada
  • K. Yamaoka
  • A. Yoshida
  • S. Zane
Publication date 2009
Journal Astrophysical Journal Letters
Volume | Issue number 693 | 2
Pages (from-to) L122-L126
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract
We present the first Suzaku observation of the new Soft Gamma Repeater, SGR 0501+4516, performed on 2008 August 26, four days after the onset of bursting activity of this new member of the magnetar family. The soft X-ray persistent emission was detected with the X-ray Imaging Spectrometer (XIS) at a 0.5-10 keV flux of 3.8 x 10-(11) erg s(-1) cm(-2), with a spectrum well fitted by an absorbed blackbody plus power-law model. The source pulsation was confirmed at a period of 5.762072 +/- 0.000002 s, and 32 X-ray bursts were detected by the XIS, four of which were also detected at higher energies by the Hard X-ray Detector (HXD). The strongest burst, which occurred at 03:16:16.9 (UTC), was so bright that it caused instrumental saturation, but its precursor phase, lasting for about 200 ms, was detected successfully over the 0.5-200 keV range, with a fluence of similar to 2.1 x 10(-7) erg cm-2 and a peak intensity of about 89 crab. The entire burst fluence is estimated to be similar to 50 times higher. The precursor spectrum was very hard, and well modeled by a combination of two blackbodies. We discuss the bursting activity and X/gamma-ray properties of this newly discovered Soft Gamma Repeater in comparison with other members of the class.
Document type Article
Note DOI: 10.1088/0004-637X/693/2/L122; eprintid: arXiv:0901.3453
Language English
Published at https://doi.org/10.1088/0004-637X/693/2/L122
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