The optically dim GRB 030115
Optical follow-up observations at OSN and BOOTES
The reddened object close to the GRB 030115 error box (GCN Circ. 1805)
and unrelated to the GRB (GCN Circ. 1807), based on the 300-s R-band
image obtained at the 1.5-m telescope at Observatorio de Sierra Nevada
in Granada. The field of view is 7' x 7'. North is up and east to
the left. No counterpart within the HETE-2 error box is seen down to
R = 20 in the co-added image.
TITLE: GCN GRB OBSERVATION REPORT
NUMBER: 1805
SUBJECT: GRB 030115, optical candidate
DATE: 03/01/15 06:01:20 GMT
FROM: Alberto Castro-Tirado at Inst. de Astrofísica de Andalucía
GRB 030115, optical candidate
--------------------------------------
Alberto Castro-Tirado, J. Gorosabel, V. Casanova
and Enrique García-Lobo, IAA-CSIC (Granada)
José María Castro Cerón, ROA (San Fernando)
and A. de Ugarte (Oss. Astron. di Brera)
report:
"Following the detection of GRB 030115 by HETE, we have
obtained BVRI images at the 1.5-m telescope at IAA's
Observatorio de Sierra Nevada in Granada, starting on Jan
15.220 UT. An optical source with R about 18 which is not
in the DDS-2 (R) is seen at coordinates AR (2000) =
11 18 23.8 Dec (2000) = + 15 05 10 (preliminary). Further
observations are urged in order to confirm whether this is
the optical counterpart of GRB 030115."
TITLE: GCN GRB OBSERVATION REPORT
NUMBER: 1807
SUBJECT: GRB 030115, no optical candidate
DATE: 03/01/15 08:28:03 GMT
FROM: Alberto Castro-Tirado at Inst. de Astrofísica de Andalucía
GRB 030115, no optical candidate
--------------------------------------
Alberto Castro-Tirado, J. Gorosabel, V. Casanova
and Enrique García-Lobo, IAA-CSIC (Granada)
José María Castro Cerón, ROA (San Fernando)
A. de Ugarte (Oss. Astron. di Brera)
J. Fynbo (Univ. of Aarhus)
and E. Rol (Univ. of Amsterdam)
report:
"Further analysis of the 1.5-m OSN B-band images
obtained covering the GRB 030115 error box, suggests
that the optical candidate previously reported (GCN
Circ. 1805) seems to be a reddened object that is also
present in the DDS-2 (R and B). Taking into account
that there is no other obvious optical counterpart within
the HETE-2 error box down to R about 20 on Jan 15.220
UT (i.e 1h 55m after the trigger), this GRB would be a
good candidate for an optically dim/dark burst. Deeper
optical and IR observations are encouraged."
TITLE: GCN GRB OBSERVATION REPORT
NUMBER: 1826
SUBJECT: GRB 030115, simultaneous observations by BOOTES-1
DATE: 03/01/17 14:00:03 GMT
FROM: Alberto Castro-Tirado at Inst. de Astrofísica de Andalucía
GRB 030115, simultaneous observatios by BOOTES-1
-------------------------------------------------
Alberto Castro-Tirado (IAA-CSIC Granada and LAEFF-INTA, Madrid)
T. J. Mateo Sanguino (CEDEA-INTA, Huelva)
,
A. de Ugarte Postigo (Oss. Astron. di Brera)
,
M. Jélinek, P. Kubánek, R. Hudec (ASU-CAS, Ondrejov)
,
S. Vitek, P. Páta (FEL-CVUT)
and J. Á. Berná (Univ. de Alicante)
on behalf of the BOOTES team,
report:
"We have obtained several unfiltred exposures (45-s each)
under good metereological conditions covering the 20-s long
GRB 030115 HETE-2 error box (Kawai et al. GCN 1816). The
images covered the period 03:22:35 - 03:24:52 UT 15 Jan 2003
(i.e. between 1 and 138-s after the trigger) with the very
wide-field camera of BOOTES-1 (http://www.laeff.esa.es/BOOTES).
After a visual inspection of the HETE-2 error box in the frames,
we do not find evidence of optical emission, in particular
simultaneously to the burst itself, for which we have an image
covering the time interval 03:22:35-03:23:20 UT. Therefore we
derive an upper limit of R = 10 for any optical emission
simultaneous to this long/soft GRB."