{
  "bibcode": "2010GCN.10897....1B",
  "body": "E. Berger, R. Chornock, W. Fong (Harvard), W. Krzeminski (LCO), and G. \nAnglada (Carnegie/DTM) report:\n\n\"We observed the location of the short GRB 100625A (GCN 10884) using the \nPANIC infrared imager on the Magellan/Baade 6.5-m telescope on 2010 June \n27.39 UT (38.9 hours after the burst).  A total of 1.75 hours were \nobtained in J-band in good seeing conditions (0.75 arcsec).  Within the \nrefined XRT error circle (GCN 10886) we detect a single object, \ncoincident with the optical source detected by Levan et al. with Gemini \nabout 12.3 hours after the burst (GCN 10887).  In our combined image the \nobject appears to be mildly extended.  Given the continued detection of \nthe object about 27 hours after the initial Gemini detection (with r~23 \nmag), and its extended nature, we consider this source to be a potential \nhost galaxy.\"",
  "circularId": 10897,
  "createdOn": 1277743279000,
  "email": "eberger@cfa.harvard.edu",
  "subject": "GRB 100625A:  Magellan near-IR Observations",
  "submitter": "Edo Berger at Harvard  <eberger@cfa.harvard.edu>",
  "eventId": "GRB 100625A"
}