GRB 190615A
GCN Circular 24839
Subject
GRB 190615A: Fermi GBM Final Real-time Localization
Date
2019-06-15T15:28:10Z (6 years ago)
From
Fermi GBM Team at MSFC/Fermi-GBM <do_not_reply@GIOC.nsstc.nasa.gov>
The Fermi GBM team reports the detection of a likely LONG GRB
At 15:16:27 UT on 15 Jun 2019, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 190615A (trigger 582304592.372344 / 190615636).
The on-ground calculated location, using the Fermi GBM trigger data, is RA = 191.4, Dec = 49.4 (J2000 degrees, equivalent to J2000 12h 45m, 49d 23'), with a statistical uncertainty of 2.3 degrees.
The angle from the Fermi LAT boresight is 122.0 degrees.
The skymap can be found here:
http://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2019/bn190615636/quicklook/glg_skymap_all_bn190615636.png
The HEALPix FITS file, including the estimated localization systematic, can be found here:
http://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2019/bn190615636/quicklook/glg_healpix_all_bn190615636.fit
The GBM light curve can be found here:
http://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2019/bn190615636/quicklook/glg_lc_medres34_bn190615636.gif
GCN Circular 24842
Subject
GRB 190615A: Insight-HXMT/HE detection
Date
2019-06-17T05:36:47Z (6 years ago)
From
Qi Luo at IHEP <luoqi@ihep.ac.cn>
Q. Luo, S. Xiao, C. Cai, Q. B. Yi, C. K. Li,
X. B. Li, G. Li, J. Y. Liao, S. L. Xiong,
C. Z. Liu, X. F. Li, Z. W. Li, Z. Chang, X. F. Lu,
A. M. Zhang, Y. F. Zhang, C. L. Zou (IHEP), Y. J. Jin,
Z. Zhang (THU), T. P. Li (IHEP/THU), F. J. Lu, L. M. Song,
M. Wu, Y. P. Xu, S. N. Zhang (IHEP),
report on behalf of the Insight-HXMT team:
At 2019-06-15T15:16:27.00 (T0), Insight-HXMT/HE detected
GRB 190615A (trigger ID: HEB190615636) in a routine search of the data,
which was also triggered by Fermi/GBM (GCN #24839).
The Insight-HXMT/HE light curve mainly consists of a single
pulse with a duration (T90) of 16.33 s measured from T0-1.65 s.
The 1-ms peak rate, measured from T0+7.80 s, is 606 cnts/sec.
The total counts from this burst is 4626 counts.
URL_LC: http://www.hxmt.org/images/GRB/HEB190615636_lc.jpg
All measurements above are made with the CsI detectors operating in the
regular mode with the energy range of about 80-800 keV (deposited energy).
Only gamma-rays with energy greater than about 200 keV can penetrate
the spacecraft and leave signals in the CsI detectors installed inside
of the telescope.
Insight-HXMT is the first Chinese space X-ray telescope, which was
funded jointly by the China National Space Administration (CNSA) and
the Chinese Academy of Sciences (CAS).
More information about it could be found at:
http://www.hxmt.org.