Skip to main content
Testing. You are viewing the public testing version of GCN. For the production version, go to https://gcn.nasa.gov.
New Announcement Feature, Code of Conduct, Circular Revisions. See news and announcements

GCN Circular 12737

Subject
GRB 111228A: Swift detection of a burst with an optical counterpart
Date
2011-12-28T16:00:13Z (12 years ago)
From
David Burrows at PSU/Swift <burrows@astro.psu.edu>
T. N. Ukwatta (MSU), W. H. Baumgartner (GSFC/UMBC),
D. N. Burrows (PSU), S. Campana (INAF-OAB), P. D'Avanzo (INAF-OAB),
B. Gendre (ASDC), C. Guidorzi (U Ferrara),
S. T. Holland (CRESST/USRA/GSFC), E. A. Hoversten (PSU),
H. A. Krimm (CRESST/GSFC/USRA), A. Y. Lien (NASA/GSFC/ORAU),
C. B. Markwardt (NASA/GSFC), A. Melandri (INAF-OAB),
J. P. Osborne (U Leicester), B. Sbarufatti (INAF-OAB/PSU),
M. H. Siegel (PSU), E. Sonbas (NASA/GSFC/Adiyaman Univ.) and
E. Troja (NASA/GSFC/ORAU) report on behalf of the Swift Team:

At 15:44:43 UT, the Swift Burst Alert Telescope (BAT) triggered and
located GRB 111228A (trigger=510649).  Swift slewed immediately to the burst. 
The BAT on-board calculated location is 
RA, Dec 150.079, +18.293 which is 
   RA(J2000) = 10h 00m 19s
   Dec(J2000) = +18d 17' 35"
with an uncertainty of 3 arcmin (radius, 90% containment, including 
systematic uncertainty).  The BAT light curve showed a strong triple-peaked
structure with a duration of about 100 sec.  The peak count rate
was ~5000 counts/sec (15-350 keV), at ~93 sec after the trigger. 

The XRT began observing the field at 15:47:08.6 UT, 145.1 seconds after
the BAT trigger. Using promptly downlinked data we find a bright,
uncatalogued X-ray source located at RA, Dec 150.06478, 18.29912 which
is equivalent to:
   RA(J2000)  = 10h 00m 15.55s
   Dec(J2000) = +18d 17' 56.8"
with an uncertainty of 4.2 arcseconds (radius, 90% containment). This
location is 53 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.  We
cannot determine whether the source is fading at the present time. 

A power-law fit to a spectrum formed from promptly downlinked event
data gives a column density in excess of the Galactic value (2.95 x
10^20 cm^-2, Kalberla et al. 2005), with an excess column of 2.4
(+2.09/-1.76) x 10^21 cm^-2 (90% confidence). 

The initial flux in the 0.1 s image was 8.82e-09 erg cm^-2 s^-1 (0.2-10
keV). 

UVOT took a finding chart exposure of 150 seconds with the White filter
starting 155 seconds after the BAT trigger. There is a candidate afterglow in
the rapidly available 2.7'x2.7' sub-image at
  RA(J2000)  =	10:00:16.01 = 150.06669
  DEC(J2000) = +18:17:51.8  =  18.29773
with a 90%-confidence error radius of about 0.75 arc sec. This position is 8.3
arc sec. from the center of the XRT error circle. The estimated magnitude is
17.19 with a 1-sigma error of about  0.14. No correction has been made for the
expected extinction corresponding to E(B-V) of 0.03. 

Burst Advocate for this burst is T. N. Ukwatta (tilan.ukwatta 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.)
Looking for U.S. government information and services? Visit USA.gov