VizieR Online Data Catalog: X-Ray, optical & radio obs. of GRB 160625B (Cunningham+, 2020)

The Neil Gehrels Swift Observatory began observing Gamma-Ray Burst (GRB) 160625B 2.5 hours after the initial Gamma-ray Burst Monitor (GBM) trigger. The X-ray Telescope (XRT) on board Swift observed GRB160625B for 47 days.In addition to the XRT data we include the late-time Chandra observations taken by K20 at 69.8 and 144days after the burst.

We utilized several optical instruments to observe the GRB; the 2m Faulkes Telescope North (FTN) operated by Las Cumbres Observatory (LCO), the 2m Liverpool Telescope (LT) at Roque de los Muchachos Observatory (ORM), and the Low Dispersion Survey Spectrograph 3 (LDSS3) at Magellan, ranging from 0.56 to 37days post-trigger. We also observed the GRB with the Reionization And Transients InfraRed camera (RATIR) beginning 8hr after the trigger until it faded beyond detection at ~50 days and also reported u-band observations taken with the Ultraviolet/Optical Telescope (UVOT) on board Swift. Late-time Hubble Space Telescope (HST) observations were reported by K20 71.5 and 140.2 days post-trigger.

We consolidate previous Karl G. Jansky VLA observations (Program IDs 15A-235 and S81171, PIs: Berger and Cenko, respectively) from 1.37 to 209 days after the burst for the most complete sample of radio data. We obtained additional late-time observations of GRB160625B taken at 6GHz (C band) on 2020 February 4 15:14:24 (1319 days post-burst; Program ID SC1031, PI: Cenko) for an on-source integration time of 1.8hr.

(3 data files).