[vsnet-grb-info 11582] GRB 120219A: MASTER prompt and early optical limit and OT discussion
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Tue Feb 21 18:04:30 JST 2012
TITLE: GCN CIRCULAR
NUMBER: 12977
SUBJECT: GRB 120219A: MASTER prompt and early optical limit and OT discussion
DATE: 12/02/21 09:04:00 GMT
FROM: Vladimir Lipunov at Moscow State U/Krylov Obs <gcncirc at observ.inetcomm.ru>
E. Gorbovskoy, V. Lipunov, V.Kornilov, D.Kuvshinov, A.Belinski, N.Tyurina,
N.Shatskiy, P.Balanutsa, D.Zimnukhov, A.Kuznetsov, V.V.Chazov,
A.Kuznetsov, A.Sankovich
Sternberg Astronomical Institute, Moscow State University
K.Ivanov, S.Yazev, N.M.Budnev, O.Gres, O.Chuvalaev, V.A.Poleshchuk
Irkutsk State University
V.Krushinski, I.Zalozhnich, A. Popov
Ural State University, Kourovka
V.Yurkov, Yu.Sergienko, D.Varda, E.Sinyakov
Blagoveschensk Educational State University, Blagoveschensk
A. Tlatov, A.V. Parhomenko, D. Dormidontov, V.Sennik
Kislovodsk Solar Station of the Pulkovo Observatory
Hugo Levato and Carlos Saffe
Instituto de Ciencias Astronomicas, de la Tierra y del Espacio (ICATE)
Claudio Mallamaci, Carlos Lopez and Federico Podest
Observatorio Astronomico Felix Aguilar (OAFA)
MASTER II robotic telescope (Global MASTER-Net:
http://observ.pereplet.ru)
located in Tunka and Ural was pointed to the GRB120219A (Swenson et
al., GCN Circ 12964; Ivanov et al., GCN Circ 12965).
One MASTER Very Wide Field Camera located at Tunka
(D=68 mm, 420 square degrees, 11 Mpx) was observed GRB error box
with 5 s exposure before, during and after GRB Trigger Time
without time gap between images.
Our unfiltered images are calibrated relative to Tycho stars (V).
We haven`t found optical transient within enhanced SWIFT XRT error-box
(Goad et al., GCN Circ 12967).
Our results:
T_start-T_trig T_mean-T_trig Limit Coadd Telescope Filter Site
(s) (s)
-9 -6.5 11.5 No VWFC (E) Unfilt Tunka
-4 -1.5 11.5 No VWFC (E) Unfilt Tunka
-9 33.5 13.0 18 VWFC (E) Unfilt Tunka
105 115 17.3 No MASTERII(E) P| Tunka
105 115 17.0 No MASTERII(W) P- Tunka
105 772 19.5 22 MASTERII(E+W)Unfilt Tunka
109 119 17.0 No MASTERII(W) P/ Ural
109 552 19.0 11 MASTERII(W) P/ Ural
There is some marginal object at Xin et al.(GCN 12966) OT candidate
position in Ural and Tunka added images with ~19 and ~20 mag
correspondingly (see images). The some marginal object appear on Very Wide
Field Camera at -1.5 s (mean time) and +3.5s images with 12 mag (pixel is equal 22").
But the signal/noice level is 2-3 sigma and we can not confirm or reject
this candidate.
The images and video are available at
http://master.sai.msu.ru/static/GRB120219A/GRB120219A.html .
The magnitudes in the table are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 0.03 in the direction of the burst
(Schlegel et al. 1998).
The message may be cited.
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