GCN Circular 22190
Subject
GRB 171205A: GOTO detection of the optical counterpart
Event
Date
2017-12-06T16:56:54Z (8 years ago)
From
Rhaana Starling at U of Leicester <rlcs1@leicester.ac.uk>
D.Steeghs, R.Cutter, K.Ulaczyk, D.Pollacco, R.West, A.Levan, J.Lyman, P.Chote, J.McCormac, K.Wiersema (U. Warwick)
G.Ramsay (Armagh O.)
R.Starling, P.O'Brien, R.Eyles (U. Leicester)
D.K.Galloway, E.Rol, E.Thrane, K.Ackley, A.Casey (Monash U.)
V.Dhillon, M.Dyer, S.Littlefair, E.Daw, J.Mullaney, L.Makrygianni, J.Maund (U. Sheffield)
S.Poshyachinda, S.Aukkaravittayapun, U.Sawangwit, S.Awiphan, D.Mkrtichian (NARIT)
report on behalf of the GOTO collaboration:
The Gravitational-wave Optical Transient Observer observed the field of GRB 171205A (trigger=794972, D'Elia et al. GCN Circ. 22177) from Roque de los Muchachos Observatory beginning at 2017-12-06T04:24:31 UT, 21.07 hours since burst, in several wide-band filters.
In a combined L-band image (400-700nm passband), with a total exposure time of 1440s at a mid-time 04:57:38 UT, 21.36 hours since burst, we detect the optical counterpart (Selsing et al. GCN Circ. 22180; Emery & D'Elia GCN Circ. 22181; Butler et al. GCN Circ. 22182; Mao et al. GCN Circ. 22186; Choi & Im GCN Circ. 22188