{
  "bibcode": "2020GCN.28822....1G",
  "body": "B. Gompertz (1); A. Levan (2); N. Tanvir (3); A. Fruchter (4); A. \nCucchiara (5); J. Greiner (6); J. Hjorth (7); T. Kangas (4); G. Lamb \n(3); J. Lyman (1); S. Oates (8); P. O'Brien (3); J. Osborne (3); K. Page \n(3); D. Perley (9); E. Pian (10); D. Steeghs (1); K. Wiersema (1); G. \nWynn (3)\n\n((1) University of Warwick, (2) Radboud University, (3) University of \nLeicester, (4) Space Telescope Science Institute, (5) University of the \nVirgin Islands, (6) MPE Garching, (7) University of Copenhagen, (8) \nUniversity of Birmingham, (9) Liverpool John Moores University, (10) \nINAF-OAS)\nreport:\n\nWe observed the position of GRB 201015A (D'Elia et al., GCN 28632) with \nthe Chandra X-ray Observatory with epochs 8.4 and 13.6 days after \ntrigger. The X-ray afterglow is clearly detected with a flux around 100x \nbrighter than expected based on the extrapolation of the early XRT data \ntaken between 0.03 and 0.8 days after burst. The source is seen to fade \nbetween the two Chandra epochs with a power-law index of approximately \n-0.8. A Swift ToO has been approved.",
  "circularId": 28822,
  "createdOn": 1604421905000,
  "email": "b.gompertz@warwick.ac.uk",
  "subject": "GRB 201015A: Late X-ray Detections with Chandra",
  "submitter": "Ben Gompertz at U of Warwick  <b.gompertz@warwick.ac.uk>",
  "eventId": "GRB 201015A"
}