GRB 100816: not optical observations, GRB Coordinates Networks, Circular Service

Daniele Malesani; Dong Xu; Johan Peter Uldall Fynbo; P. Jakobsson; Lars C. Astrup Buchhave

GRB 100816: not optical observations, GRB Coordinates Networks, Circular Service

Daniele Malesani, Dong Xu, Johan Peter Uldall Fynbo, P. Jakobsson, Lars C. Astrup Buchhave

Abstract

We observed the field of GRB 100816A (Oates et al., GCN 11102) with the
NOT equipped with ALFOSC. Observations were carried out in the R band.
The mid point of the observation is August 17.04 UT (24.3 hr after the GRB).

We clearly detect both the optical afterglow (Oates et al., GCN 11102)
and the putative host galaxy (Im et al., GCN 11108; Tanvir et al., GCN
11109). We find magnitudes of R = 23.0 +- 0.1 and R = 21.65 +- 0.05 for
the two objects, respectively, assuming R=17.06 for the nearby USNO star
1165-0595190. We caution that accurate photometry will have to await for
late-time templates to isolate the contribution of both objects

Originalsprog	Engelsk
Publikationsdato	17 aug. 2010
Status	Udgivet - 17 aug. 2010

Navn	GRB Corrdinates Network, Circular Services,
Nummer	1
Vol/bind	11120

Citationsformater

@misc{a87b24d965034ff89781acd51de308d1,

title = "GRB 100816: not optical observations, GRB Coordinates Networks, Circular Service",

abstract = "We observed the field of GRB 100816A (Oates et al., GCN 11102) with the NOT equipped with ALFOSC. Observations were carried out in the R band. The mid point of the observation is August 17.04 UT (24.3 hr after the GRB). We clearly detect both the optical afterglow (Oates et al., GCN 11102) and the putative host galaxy (Im et al., GCN 11108; Tanvir et al., GCN 11109). We find magnitudes of R = 23.0 +- 0.1 and R = 21.65 +- 0.05 for the two objects, respectively, assuming R=17.06 for the nearby USNO star 1165-0595190. We caution that accurate photometry will have to await for late-time templates to isolate the contribution of both objects ",

author = "Daniele Malesani and Dong Xu and Fynbo, {Johan Peter Uldall} and P. Jakobsson and Buchhave, {Lars C. Astrup}",

year = "2010",

month = aug,

day = "17",

language = "English",

series = "GRB Corrdinates Network, Circular Services,",

number = "1",

type = "Other",

}

TY - GEN

T1 - GRB 100816

T2 - not optical observations, GRB Coordinates Networks, Circular Service

AU - Malesani, Daniele

AU - Xu, Dong

AU - Fynbo, Johan Peter Uldall

AU - Jakobsson, P.

AU - Buchhave, Lars C. Astrup

PY - 2010/8/17

Y1 - 2010/8/17

N2 - We observed the field of GRB 100816A (Oates et al., GCN 11102) with the NOT equipped with ALFOSC. Observations were carried out in the R band. The mid point of the observation is August 17.04 UT (24.3 hr after the GRB). We clearly detect both the optical afterglow (Oates et al., GCN 11102) and the putative host galaxy (Im et al., GCN 11108; Tanvir et al., GCN 11109). We find magnitudes of R = 23.0 +- 0.1 and R = 21.65 +- 0.05 for the two objects, respectively, assuming R=17.06 for the nearby USNO star 1165-0595190. We caution that accurate photometry will have to await for late-time templates to isolate the contribution of both objects

AB - We observed the field of GRB 100816A (Oates et al., GCN 11102) with the NOT equipped with ALFOSC. Observations were carried out in the R band. The mid point of the observation is August 17.04 UT (24.3 hr after the GRB). We clearly detect both the optical afterglow (Oates et al., GCN 11102) and the putative host galaxy (Im et al., GCN 11108; Tanvir et al., GCN 11109). We find magnitudes of R = 23.0 +- 0.1 and R = 21.65 +- 0.05 for the two objects, respectively, assuming R=17.06 for the nearby USNO star 1165-0595190. We caution that accurate photometry will have to await for late-time templates to isolate the contribution of both objects

M3 - Other contribution

T3 - GRB Corrdinates Network, Circular Services,

ER -