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Suzaku Observation of the New Soft Gamma Repeater SGR 0501+4516 in Outburst

Authors :
Enoto, T.
Nakagawa, Y. E.
Rea, N.
Esposito, P.
Gotz, D.
Hurley, K.
Israel, G. L.
Kokubun, M.
Makishima, K.
Mereghetti, S.
Murakami, H.
Nakazawa, K.
Sakamoto, T.
Stella, L.
Tiengo, A.
Turolla, R.
Yamada, S.
Yamaoka, K.
Yoshida, A.
Zane, S.
Publication Year :
2009

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 3.8E-11 erg/s/cm2, 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 ~2.1E-7 erg/cm2 and a peak intensity of about 89 Crab. The entire burst fluence is estimated to be ~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.<br />Comment: 4 pages, 4 figures, accepted for publication in ApJL

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.0901.3453
Document Type :
Working Paper
Full Text :
https://doi.org/10.1088/0004-637X/693/2/L122