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![]() TITLE: GCN GRB OBSERVATION REPORT NUMBER: 1046 SUBJECT: Chandra Observations of SGR 1900+14 DATE: 01/04/24 00:00:36 GMT FROM: Chryssa Kouveliotou at MSFC <kouveliotou@eagles.msfc.nasa.gov> C. Kouveliotou, A. F. Tennant, and M. C. Weisskopf (NASA/MSFC), report on behalf of a large SGR collaboration: Chandra observed the newly active (GCN 1041) Soft Gamma Repeater, SGR 1900+14, on April 22, 2001 starting at 4:45 UT, for 20000 seconds. The ACIS S3 observation mode was Continuous Clocking (CC). We have fitted a spectrum to the whole data set; we find the best fit to be a single power law with spectral (photon) index of 2.9 +/- 0.1 and a hydrogen column density (NH) of (3.4 +/- 0.1)x10^22 cm^-2. We detect no black body contribution in the spectrum. The source (unabsorbed) flux is 1.1E-11 ergs/cm^2 s (2-10 keV), nearly identical to the quiescent source flux level. The pulse period is 5.1725 s (barycenter corrected); the pulse profile appears sinusoidal. More detailed analysis and comparison with RXTE simultaneous observations is underway. Cited by 4 messages X-Ray Observations
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Database maintained by Robert Quimby, Erin McMahon, and Jeremy Murphy Information displayed on this site is compiled from GCN Circulars and other sources as indicated. |
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