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

Publikation: Andet › Andet bidrag › Forskning

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GRB 100816 : not optical observations, GRB Coordinates Networks, Circular Service. / Malesani, Daniele; Xu, Dong; Fynbo, Johan Peter Uldall; Jakobsson, P.; Buchhave, Lars C. Astrup.

2010, Observationer. (GRB Corrdinates Network, Circular Services,; Nr. 1, Bind 11120).

Publikation: Andet › Andet bidrag › Forskning

Harvard

Malesani, D, Xu, D, Fynbo, JPU, Jakobsson, P & Buchhave, LCA 2010, GRB 100816: not optical observations, GRB Coordinates Networks, Circular Service..

APA

Malesani, D., Xu, D., Fynbo, J. P. U., Jakobsson, P., & Buchhave, L. C. A. (2010, aug. 17). GRB 100816: not optical observations, GRB Coordinates Networks, Circular Service. GRB Corrdinates Network, Circular Services, Bind 11120 Nr. 1

Vancouver

Malesani D, Xu D, Fynbo JPU, Jakobsson P, Buchhave LCA. GRB 100816: not optical observations, GRB Coordinates Networks, Circular Service. 2010.

Author

Malesani, Daniele ; Xu, Dong ; Fynbo, Johan Peter Uldall ; Jakobsson, P. ; Buchhave, Lars C. Astrup. / GRB 100816 : not optical observations, GRB Coordinates Networks, Circular Service. 2010. (GRB Corrdinates Network, Circular Services,; Nr. 1, Bind 11120).

Bibtex

@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",

}

RIS

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 -

ID: 32931571