[vsnet-grb-info 19026] GRB 170130A: POLAR Observation
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Wed Feb 1 17:44:05 JST 2017
TITLE: GCN CIRCULAR
NUMBER: 20568
SUBJECT: GRB 170130A: POLAR Observation
DATE: 17/02/01 08:43:20 GMT
FROM: Radek Marcinkowski at PSI/POLAR <radoslaw.marcinkowski at psi.ch>
R. Marcinkowski (PSI), H.L. Xiao (PSI) and W. Hajdas (PSI) report on behalf
of the POLAR collaboration:
At 2017-01-30 07:14:45 UT(T0), during a routine on-ground search of data,
POLAR detected GRB 170130A, which was also observed by Fermi GBM
(trigger # 507453289). Significant detection was recorded in 9 of 25 POLAR
modules.
The POLAR light curve consists of multi peak structure with duration (T90)
of 35.0 +/- 1.0 s measured from T0 and is compatible with Fermi GBM light curve.
The 1.0 s peak flux at T0 + 30.5 s is equal to 480 +/- 80 counts/sec. POLAR
recorded about 5300 events from the burst.
Above measurements are in the energy range of about 20 - 500 keV and bases
on data from 9 modules.
LC_URL: http://polar.psi.ch/triggers/GRB_170130A_raw_9of25.png
or http://polar.psi.ch/pub/lc.php?event=GRB+170130A
Using the best location from Fermi GBM, which is (J2000):
RA : 271.1 [deg]
Dec: -29.1 [deg]
Err: 5.5 [deg]
the incident angle in the POLAR coordinate at T0 is:
Theta: 56.2 [deg]
Phi: 230.9 [deg]
The analysis results presented above are preliminary. Calibration of the
instrument is ongoing. POLAR is a dedicated Gamma-Ray Burst polarimeter
which was launched on-board the Chinese space laboratory Tiangong-2 (TG-2)
on Sep 15, 2016. The energy detection range of POLAR is ~ 50-500 keV.
More information about POLAR can be found at http://polar.psi.ch/pub ,
http://polar.ihep.ac.cn/en/ and http://isdc.unige.ch/polar/ .
This message is quotable in publications.
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