{
  "bibcode": "2019GCN.24253....1B",
  "body": "C. D. Bochenek (Caltech), S. R. Kulkarni (Caltech), D. McKenna (Caltech), K. Belov (JPL), V. Ravi (Harvard, Caltech), T. Callister (Caltech)\n\nSTARE2 is an all-sky instrument located at the Owens Valley Radio Observatory (OVRO) and the Goldstone Deep Space Communications Complex designed to search for fast radio transients. STARE2 is sensitive to millisecond duration bursts of radio emission above 157 kJy, for a burst at zenith. STARE2 regularly sees type IIIdm bursts from the Sun.\n\nNo candidate events were found within 3 hours of the LIGO/Virgo S190426c.\n\nObserving frequency: 1280-1530 MHz\nTime resolution: 65.536 microseconds\nMaximum timescale STARE2 is sensitive to: 34 ms\nFrequency resolution: 122.07 kHz\nDispersion measure search range: 5 pc cm^-3 - 3000 pc cm^-3\n\nA map of our upper limit as a function of RA and DEC can be found at: http://www.astro.caltech.edu/~cbochenek/LIGO_VIRGO_S190426c_limits.png\n\n\nThe sky at OVRO at the time of the event contains 76% of the LIGO localization region.",
  "circularId": 24253,
  "createdOn": 1556323671000,
  "email": "cbochenek@astro.caltech.edu",
  "subject": "LIGO/Virgo S190426c: STARE2 simultaneous L-band radio observations",
  "submitter": "Christopher Bochenek at California Institute of Technology  <cbochenek@astro.caltech.edu>",
  "eventId": "LIGO/Virgo S190426c"
}