//////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 20363 SUBJECT: GRB 170102A: POLAR observation DATE: 17/01/04 08:29:33 GMT FROM: Zhao Yi at POLAR Yi Zhao (IHEP), Hancheng Li (IHEP) and Minzi Feng (IHEP) report on behalf of the POLAR collaboration: At 2017-01-02T02:51:18.00 UT (T0), during a routine on-ground search of data, POLAR detected the GRB 170102A, which was also detected by the KONUS-Wind. The POLAR light curve consists of multiple peaks, with a duration (T90) of 40.03 s measured from T0-1.66 s. The 1-s peak rate measured from T0+23.00 s is 335.7 cnts/s. The total counts is about 4727 cnts. The above measurements are in the energy range of about 80-500 keV. LC_URL: http://polar.ihep.ac.cn/grb/2017/01/GRB170102A/lc/POLAR_lc_grb170102A.jpg All analysis results presented above are preliminary. POLAR is a dedicated Gamma-Ray Burst polarimeter (50-500 keV) on-board the Chinese space laboratory Tiangong-2 launched on Sep 15,2016. More information about POLAR can be found at http://polar.ihep.ac.cn/en/, http://isdc.unige.ch/polar/ and http://polar.psi.ch/pub/. //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 20368 SUBJECT: GRB 170102A: Astrosat CZTI detection DATE: 17/01/05 10:51:34 GMT FROM: Vidushi Sharma at IUCAA V. Sharma, V. Bhalerao (IUCAA) and D. Bhattacharya, A. R. Rao (TIFR) and S. Vadawale (PRL) report on behalf of the AstroSat CZTI collaboration: Analysis of AstroSat CZTI data showed weak detection of GRB170102A (POLAR detection: Yi Zhao et al., GCN 20363) in the 40-200 keV energy range. The light curve shows multiple peak structure with stronger peak at 02:51:41 UT, 23 secs after POLAR trigger. The measured peak count rate is 101.98 counts/sec above the background in combined data of four quadrants, with a total of 636.26 counts. The local mean background count rate was 353 counts/sec. CZTI GRB detections are reported regularly on the payload site at http://astrosat.iucaa.in/czti/?q=grb. CZTI is built by a TIFR-led consortium of institutes across India, including VSSC, ISAC, IUCAA, SAC and PRL. The Indian Space Research Organisation funded, managed and facilitated the project.