TITLE: GCN GRB OBSERVATION REPORT NUMBER: 1741 SUBJECT: Chandra observation of the IPN error box of GRB021201 (short/hard) DATE: 02/12/12 21:34:59 GMT FROM: Kevin Hurley at UCBerkeley/SSL K. Hurley, T. Cline, M. Feroci, P. Li, F. Frontera, E. Mazets, S. Golenetskii, I. Mitrofanov, G. Ricker, and J.-L. Atteia, on behalf of the Chandra target of opportunity for IPN short bursts collaboration, report: Chandra observed the error box of the short/hard GRB021201 (GCN 1719) for approximately 21 ks starting at 23:10 on December 9. A very preliminary analysis indicates that about 26 sources are present in the Chandra field. They are listed in the table below. One of these sources (#10) is inside the IPN error box. A map has been posted at ssl.berkeley.edu/ipn3/021201. A second follow-up Chandra observation will take place in several weeks to determine whether this or any other source in the field displays fading behavior. SOURCE # RA(2000) DEC(2000) NET_COUNTS 1 122.0995407104 21.3008174896 26.18750 2 122.0711364746 21.2559471130 39.250 3 122.0690231323 21.1490001678 182.750 4 122.0568161011 21.102066040 1553.06250 5 122.0377426147 21.1755084991 77.68750 6 122.0145645142 21.2685337067 29.8750 7 121.9966888428 21.1383686066 38.750 8 121.9874267578 21.3674888611 28.43750 9 121.9564666748 21.1419563293 139.93750 10 121.9553070068 21.2090072632 105.18750 11 121.9549407959 21.3561420441 50.43750 12 121.9532623291 21.2970886230 40.06250 13 121.9205551147 21.3233127594 29.93750 14* 121.9204101562 21.3241481781 34.8750 15 121.9017181396 21.1891117096 28.750 16* 121.9007949829 21.1885643005 29.50 17 121.8824768066 21.2981529236 54.0 18 121.8699111938 21.1710834503 176.06250 19 121.8655853271 21.2566776276 36.68750 20 121.8629837036 21.2110004425 43.1250 21 121.8587265015 21.1649875641 32.1250 22 121.8439636230 21.1804847717 92.18750 23 121.8304367065 21.3124256134 24.56250 24 121.8092498779 21.2480392456 47.93750 25 121.7484664917 21.2483577728 30.18750 26 121.7267990112 21.1938285828 32.06250 27 121.6778488159 21.4611721039 20.6250 28 121.6126785278 21.2064838409 32.93750 *These are probably duplicate detections of the preceding sources