{
  "subject": "Correction: Chandra X-ray observations of GW170817 at 1 year post-merger: increasingly rapid fading",
  "version": 2,
  "bibcode": "2018GCN.23140....1H",
  "email": "daryl.haggard@mcgill.ca",
  "eventId": "GW170817",
  "createdOn": 1534261323000,
  "editedBy": "Judith Racusin at NASA/GSFC <judith.racusin@nasa.gov>",
  "circularId": 23140,
  "body": "Daryl Haggard, Melania Nynka, and J. J. Ruan (McGill/MSI) write:\n\nWe correct a typo in GCN 23137: The 0.5-8 keV count rate measured in the \n10 August 2018 Chandra observation of GW170817 should have read 4.9 \n(+0.9/-0.9) e-04 ct/s. All fluxes, photon indices, luminosities, light \ncurve slopes, etc., reported in GCN 23137 are correct, and were derived \nfrom this correct count rate.\n\nGCN OPS NOTE(28aug18):  Per author's request, the Subject-line\nwas corrected with the proper referencing Subject-line.]",
  "editedOn": 1777052902501,
  "submitter": "Daryl Haggard at McGill U  <daryl.haggard@mcgill.ca>"
}