[vsnet-grb-info 27432] GRB 210217A: Liverpool Telescope First Hour Observations
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Fri Feb 19 07:18:28 JST 2021
TITLE: GCN CIRCULAR
NUMBER: 29535
SUBJECT: GRB 210217A: Liverpool Telescope First Hour Observations
DATE: 21/02/18 22:17:33 GMT
FROM: Manisha Shrestha at Liverpool John Moores U <m.shrestha at ljmu.ac.uk>
M. Shrestha (Liverpool JMU), R. Smith (LJMU) , A. Melandri (INAF), I.A. Steele (LJMU), S. Kobayashi (LJMU), C. Mundell (Univ. Bath), A. Gomboc (Univ. Nova Gorica), C. Guidorzi (Univ. Ferrara) report on behalf of a wider collaboration:
We observed the field of Swift GRB 210217A (GCN 29521) with the 2.0m Liverpool Telescope (LT), La Palma on 2021 Feb 17 starting at 23:28:51.056 UT
using the IO:O optical camera in the r, i, and z bands. Data were calibrated with respect to nearby APASS secondary standard stars for r and i bands
and SDSS secondary standard stars for z band. We confirm the optical counterpart reported by Swift UVOT and NEXT (GCN 29523).
At T=194 seconds after the BAT trigger time, we measure r = 18.51 +/- 0.3 mag which is close to 18.6 +/- 0.2 mag detected by NEXT team (GCN 29523).
The r band light curve made with IO:O observations show a power law decay over the first hour in flux vs time with alpha = 0.48.
At T = 690 seconds after the BAT trigger time, we measure i = 18.77 +/- 0.1 mag and at T = 868 seconds after the trigger we measure z = 18.67 +/-0.1 mag.
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