GCN Circular 28639
Subject
GRB 201015A: GOTO confirmation of afterglow detection
Date
2020-10-16T03:18:47Z (5 years ago)
From
Kendall Ackley at Monash University <kendall.ackley@monash.edu>
K. Ackley (1); D. K. Galloway (1); Y-L Mong (1); M. Dyer (2); J. Lyman (3);
K.
Ulaczyk (3); D. Steeghs (3); V. Dhillon (2); P. O'Brien (4); G. Ramsay
(5); S. Poshyachinda (6); R. Kotak (7); L. Nuttall (8); D. Pollacco
(3); R. Breton (9)
((1) Monash University, (2) University of Sheffield, (3) Warwick
University, (4) University of Leicester, (5) Armagh Observatory &
Planetarium, (6) National Astronomical Research Institute of Thailand,
(7) University of Turku, (8) University of Portsmouth, (9) University
of Manchester)
report on behalf of the GOTO collaboration:
We carried out observations with the Gravitational-wave Optical
Transient Observer (GOTO) on La Palma in response to GRB 201015A
(Swift; D'Elia et al; GCN 28632).
We made a series of 4x90 s exposures using our wide L-band filter
(400-700 nm) covering the Swift XRT error box (Swift; Kennea et al.; GCN
28635),
beginning at 51 minutes after trigger, with midtime of the
first observation 23:41:54.25 UT on 15 October 2020.
Using a difference imaging analysis with recent survey observations of
the same pointings as reference, we detect an uncatalogued source
located at (J2000):
RA 23:37:16.42
Dec +53:24:55.89
confirming the OT reported by MASTER (Lupinov et al.; GCN 28633