{
  "bibcode": "2016GCN.19736....1Y",
  "body": "George Younes (GWU), Chryssa Kouveliotou (GWU), Oliver Roberts (UCD)\nreport on behalf of a larger collaboration:\n\n\"At 13:02:07.91 UT on 27 July 2016, the Fermi Gamma-Ray Burst\nMonitor triggered on an SGR-like burst (trigger 491317331/160727543).\nThe on-ground calculated location, using the Fermi GBM trigger data,\nis RA = 148.4, Dec = -73.3, with a statistical uncertainty of 8.8 degrees.\n\nThe Fermi/GBM location is consistent with the Swift/BAT trigger=706396\nlocation, which is believed to be from the direction of PSR 1119-6127\n(GCN #19735). This would be the second burst from the same source\nand the second high B-field rotation powered pulsar detected emitting\nmagnetar-like bursts.\n\nThe burst has a duration of T90 ~50 ms in the energy range\n10-100 keV. It is well-fit by a two blackbody model with temperatures\nof kT1 = 3.5 +/- 0.8 keV and kT2 = 12.0 +/- 2.0 keV.  The\ncorresponding flux  in the energy range 10-100 keV is (8.0 +/-\n1.0)E-07 erg/s/cm^2. The peak flux integrated over 16 ms is (1.3 +/-\n0.2)E-06 erg/s/cm^2.\n\nThe analysis results presented above are preliminary. Detailed\nanalysis of this burst and any untriggered will be reported elsewhere.\"",
  "circularId": 19736,
  "createdOn": 1469677995000,
  "email": "gyounes@email.gwu.edu",
  "subject": "GBM observation of SGR-like burst from the direction of PSR 1119-6127",
  "submitter": "George A. Younes at George Washington U  <gyounes@email.gwu.edu>"
}