{
  "eventId": "LIGO/Virgo G298048",
  "editedBy": "Judith Racusin at NASA/GSFC <judith.racusin@nasa.gov>",
  "createdOn": 1506402856000,
  "subject": "LIGO/VIRGO G298048: Latest 3 GHz Detection of Radio Counterpart to SSS17a",
  "bibcode": "2017GCN.21929....1H",
  "submitter": "Gregg Hallinan at Caltech  <gh@astro.caltech.edu>",
  "email": "gh@astro.caltech.edu",
  "body": "G. Hallinan (Caltech), A. Corsi (TTU), K. Mooley (Hintze Fellow, \nOxford), D.A. Frail (NRAO), M.M. Kasliwal (Caltech), report on behalf of \na larger collaboration:\n\nOur collaboration (GROWTH, JAGWAR, Caltech-NRAO, TTU-NRAO) has continued \nto monitor the evolution of the radio counterpart to GW170817/SSS17a \ndiscovered on September 2,3, 2017 with the Jansky VLA (Mooley et al. LVC \nGCN 21814 and Corsi et al. LVC GCN 21815), with ongoing observations at \nfrequencies of 1.4 GHz, 3 GHz and 6 GHz. Responding to a request for \nfurther information to help plan observations at other radio facilities, \nwe are including details on the most recent detection at 3 GHz, wherein \nthe source was detected at a flux density of 34 +/- 3.6 uJy on Sept 17 \n(UT). The full light curves and interpretation have been submitted for \npublication (Hallinan, Corsi et al.).\n\nWe thank the VLA staff for scheduling these observations.",
  "editedOn": 1777052883090,
  "circularId": 21929,
  "version": 2
}