GCN Circular 14155
Subject
Swift/BAT trigger 547142 is new source Swift J1753.7-2544
Date
2013-01-29T18:40:34Z (12 years ago)
From
Hans Krimm at NASA-GSFC <hans.krimm@nasa.gov>
H. A. Krimm (CRESST/GSFC/USRA), S. D. Barthelmy (GSFC),
W. Baumgartner (CRESST/GSFC/UMBC), J. Cummings (CRESST/GSFC/UMBC),
N. Gehrels (GSFC), C. B. Markwardt (GSFC), D. Palmer (LANL),
T. Sakamoto (AGU), M. Stamatikos (OSU/GSFC), J. Tueller (GSFC),
T. Ukwatta (MSU)
We report a follow-up to Cummings et al, GCN Circ. 14151, which reported
on a possible galactic transient as Swift/BAT trigger 547142. We now know
that this is a new galactic transient source.
The source, to which we give the name Swift J1753.7-2544, was first detected
by the BAT on 2013 January 24 (MJD 56316) and has been mostly brightening
ever since.
The BAT rates in the 15-50 keV band have been
Jan 24: 0.0050 � 0.001 ct/s/cm^2 (23 mCrab)
Jan 25: 0.0074 � 0.001 ct/s/cm^2 (33 mCrab)
Jan 26: 0.014 � 0.002 ct/s/cm^2 (64 mCrab)
Jan 27: 0.0090 � 0.001 ct/s/cm^2 (41 mCrab)
Jan 28: 0.017 � 0.002 ct/s/cm^2 (80 mCrab)
Jan 29: 0.017 � 0.002 ct/s/cm^2 (80 mCrab)
The best BAT position is:
RA(J2000) = 268.429, Dec(J2000) = -25.742
RA = 17h 53m 43s, Dec = -25d 44' 31"
Glon= 3.664, Glat = +0.099
The estimated error (statistical plus systematic) is 3 arc minutes (90%
confidence) This position is derived from the BAT transient monitor.
At 06:16:29 UT on February 28, 2013 (MJD 56320), Swift J1753.7-2544 triggered
BAT in a 1280-second image trigger. On-board software identified it as
a gamma-ray burst, but the Swift team suggested that it is more likely a
galactic transient (Cummings et al, GCN Circ. 14151).
Using the BAT event data set from T+165 to T+963, we report further analysis
of Swift J1753.7-2544 The BAT ground-calculated position from the event data
is RA, Dec = 268.429, -25.745 deg which is within 0.2 arcminutes of the BAT
monitor position. The partial coding was 92%. The mask-weighted light curve
shows no significant structure and an average count rate in the 15-100 keV
band of roughly 0.03 ct/s/cm^2.
The time-averaged spectrum from T+165 to T+963 sec is best fit by a simple
power-law model. The power law index of the time-averaged spectrum is
2.07 +- 0.25. The fluence in the 15-150 keV band is 2.1 +- 0.3 x 10^-6
erg/cm2. (90% confidence level.
Sakamoto et al (GCN Circ. 14153) reported no detection in MAXI (4-10 keV)
during short observations near the time of the BAT trigger.
A Swift target of opportunity observation has been requested. However, due to a
Sun constraint, there will be no Swift XRT or UVOT observations before
Feb. 4, 2013.
The BAT hard X-ray transient monitor light curve for Swift J1753.7-2544 can be
found at
http://swift.gsfc.nasa.gov/docs/swift/results/transients/weak/SWIFTJ1753.7-2544/