{
  "bibcode": "2024GCN.37473....1P",
  "createdOn": 1726152279839,
  "body": "Devraj Pawar (R. J. College, Mumbai-86, India) on behalf of a collaboration studying transients.\n\nThe Fermi GBM team reported detection of GRB 240912A in GCN 37465. We analyzed the INTEGRAL SPI ACS data around the given T0 and detected a multi-peak burst. The light curve is given on the following link and further outcomes will be updated on the same page. The SPI ACS is sensitive above 80 keV; the burst peaks at ~4200 counts/s above a steady rate of 3400 counts/s, this may be affected by the instruments orientation with respect to the direction of the source. \n\n[https://docs.google.com/document/d/1e3pSUtLecDZTZkkMOuYGc6L4t64F4V-tjK1KT3_N7GE/edit?usp=sharing]()\n\nThis work is based on observations with INTEGRAL, an ESA project with instruments and a science data center funded by ESA member states (especially the PI countries: Denmark, France, Germany, Italy, Switzerland, Spain), and with the participation of Russia and the USA. The SPI-ACS detector system has been provided by MPE Garching/Germany. ",
  "subject": "GRB 240912A :  INTEGRAL SPI ACS LIGHT CURVE",
  "submitter": "Devraj Pawar at R. J. College, Mumbai - 86, India <devrajdp@gmail.com>",
  "circularId": 37473,
  "format": "text/plain",
  "submittedHow": "web",
  "eventId": "GRB 240912A"
}