{
  "bibcode": "2013GCN.14979....1P",
  "body": "D. A. Perley (Caltech) and M. Kasliwal (Carnegie) report on behalf of a \nlarger collaboration:\n\nWe observed the location of the probable optical counterpart of Fermi \nGRB 130702A (Singer et al., GCN 14967; Cheung et al., GCN 14971; \nCollazzi & Connaughton, GCN 14972) with the Combined Array for Research \nin Millimeter Astronomy (CARMA) on 2013-07-04 between 00:28:21 and \n05:56:31 UT, 2.01-2.24 days after the GBM trigger, at a frequency of 93 \nGHz (3 mm).  Weather conditions were poor initially but improved \nsomewhat over the course of the integration.   In a preliminary \nreduction of the data we detect a millimeter source coincident with the \nlocation of the optical counterpart with a flux of approximately ~2 mJy.\n\nWe thank John Carpenter and the CARMA staff for their support.",
  "circularId": 14979,
  "createdOn": 1372918519000,
  "email": "dperley@astro.caltech.edu",
  "subject": "GRB 130702A: CARMA 3mm detection",
  "submitter": "Daniel Perley at Caltech  <dperley@astro.caltech.edu>",
  "eventId": "GRB 130702A"
}