A. Y. Lien (GSFC/UMBC), J. A. Kennea (PSU),
H. A. Krimm (CRESST/GSFC/USRA), C. B. Markwardt (NASA/GSFC),
F. E. Marshall (NASA/GSFC), C. Pagani (U Leicester) and
D. M. Palmer (LANL) report on behalf of the Swift Team:
At 03:50:43 UT, the Swift Burst Alert Telescope (BAT) triggered and
located GRB 141121A (trigger=619182). Swift slewed immediately to the burst.
The BAT on-board calculated location is
RA, Dec 122.668, +22.225 which is
RA(J2000) = 08h 10m 40s
Dec(J2000) = +22d 13' 31"
with an uncertainty of 3 arcmin (radius, 90% containment, including
systematic uncertainty). The BAT light curve shows no significant structure,
as usual for an image trigger.
The XRT began observing the field at 03:56:45.6 UT, 362.4 seconds after
the BAT trigger. XRT found a bright, uncatalogued X-ray source located
at RA, Dec 122.6700, 22.2177 which is equivalent to:
RA(J2000) = +08h 10m 40.80s
Dec(J2000) = +22d 13' 03.7"
with an uncertainty of 4.8 arcseconds (radius, 90% containment). This
location is 27 arcseconds from the BAT onboard position, within the BAT
error circle. No event data are yet available to determine the column
density using X-ray spectroscopy.
The initial flux in the 2.5 s image was 6.07e-09 erg cm^-2 s^-1 (0.2-10
UVOT took a finding chart exposure of 150 seconds with the White filter
starting 370 seconds after the BAT trigger. No credible afterglow candidate has
been found in the initial data products. The 2.7'x2.7' sub-image covers 100% of
the XRT error circle. The typical 3-sigma upper limit has been about 19.6 mag.
The 8'x8' region for the list of sources generated on-board covers 100% of the
XRT error circle. The list of sources is typically complete to about 18 mag. No
correction has been made for the expected extinction corresponding to E(B-V) of
Burst Advocate for this burst is A. Y. Lien (amy.y.lien AT nasa.gov).
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.)