TITLE: GCN CIRCULAR NUMBER: 14140 SUBJECT: GRB 130122A: Swift detection of a burst with an optical counterpart DATE: 13/01/22 23:57:00 GMT FROM: Scott Barthelmy at NASA/GSFC A. Y. Lien (NASA/GSFC/ORAU), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC), A. P. Beardmore (U Leicester), N. Gehrels (NASA/GSFC), K. L. Page (U Leicester), D. M. Palmer (LANL), T. Sakamoto (AGU), B. Sbarufatti (INAF-OAB/PSU), M. H. Siegel (PSU) and E. Troja (NASA/GSFC/UMCP) report on behalf of the Swift Team: At 23:44:09 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 130122A (trigger=546731). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 194.218, +59.015 which is RA(J2000) = 12h 56m 52s Dec(J2000) = +59d 00' 55" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve shows a single peak with a duration of about 30 sec. The peak count rate was ~1000 counts/sec (15-350 keV), at ~1 sec after the trigger. The XRT began observing the field at 23:46:06.3 UT, 116.9 seconds after the BAT trigger. Using promptly downlinked data we find a fading, uncatalogued X-ray source located at RA, Dec 194.28337, 59.01331 which is equivalent to: RA(J2000) = 12h 57m 08.01s Dec(J2000) = +59d 00' 47.9" with an uncertainty of 3.6 arcseconds (radius, 90% containment). This location is 121 arcseconds from the BAT onboard position, within the BAT error circle. This position may be improved as more data are received; the latest position is available at http://www.swift.ac.uk/sper. A power-law fit to a spectrum formed from promptly downlinked event data gives a column density consistent with the Galactic value of 9.34 x 10^19 cm^-2 (Kalberla et al. 2005). UVOT took a finding chart exposure of 150 seconds with the White filter starting 121 seconds after the BAT trigger. There is a candidate afterglow in the list of sources generated on-board at RA(J2000) = 12:57:08.34 = 194.28476 DEC(J2000) = +59:00:53.9 = 59.01496 with a 90%-confidence error radius of about 1.10 arc sec. This position is 6.2 arc sec. from the center of the XRT error circle. The estimated magnitude is 18.95. No correction has been made for the expected extinction corresponding to E(B-V) of 0.01. Burst Advocate for this burst is A. Y. Lien (yarleen AT gmail.com). Please contact the BA by email if you require additional information regarding Swift followup of this burst. In extremely urgent cases, after trying the Burst Advocate, you can contact the Swift PI by phone (see Swift TOO web site for information: http://www.swift.psu.edu/too.html.)