TY - GEN
T1 - GRB 191019A: Zadko Telescope optical observations
AU - Gendre, B.
AU - Crisp, H.
AU - Coward, D.
AU - Zadko, J.
AU - Moore, J. A.
AU - Burrell, A.
AU - Klotz, A.
AU - Thierry, P.
AU - Howell, E. J.
AU - Verveer, A.
AU - Kennewell, J.
PY - 2019/10/1
Y1 - 2019/10/1
N2 - We observed GRB 191019A (Simpson et al., GCN 26031) with the Zadko
Telescope (Coward et al. 2017), starting at 2019 October the 19th at
15:20:23 UT (7 minutes 50 seconds after the trigger) under fair
conditions. The object reported by Reva et al. (GCN 26036) is clearly
visible in our images. However, we measure an R magnitude of 18.92 at
the time reported by the GCN. Observations stopped one hour twenty
three minutes after the burst, and during that time we do not see any
variation on the light curve, similar to other teams (Perley et al.,
GCN 26039; Fynbo et al., GCN 26041; and Zhu et al., GCN 26059). At that
position, the USNO catalog reports a source of magnitude R = 19.0,
consistent with our findings. We conclude that this object is not the
afterglow of GRB 191019A, but the host galaxy, as reported by Perley et
al. (GCN 26062). The Zadko Telescope has been under refurbishment
during the last year, and is still in recommissioning mode. This
message can be cited. -- L'absence de virus dans ce courrier
électronique a été vérifiée par le
logiciel antivirus Avast. https://www.avast.com/antivirus
AB - We observed GRB 191019A (Simpson et al., GCN 26031) with the Zadko
Telescope (Coward et al. 2017), starting at 2019 October the 19th at
15:20:23 UT (7 minutes 50 seconds after the trigger) under fair
conditions. The object reported by Reva et al. (GCN 26036) is clearly
visible in our images. However, we measure an R magnitude of 18.92 at
the time reported by the GCN. Observations stopped one hour twenty
three minutes after the burst, and during that time we do not see any
variation on the light curve, similar to other teams (Perley et al.,
GCN 26039; Fynbo et al., GCN 26041; and Zhu et al., GCN 26059). At that
position, the USNO catalog reports a source of magnitude R = 19.0,
consistent with our findings. We conclude that this object is not the
afterglow of GRB 191019A, but the host galaxy, as reported by Perley et
al. (GCN 26062). The Zadko Telescope has been under refurbishment
during the last year, and is still in recommissioning mode. This
message can be cited. -- L'absence de virus dans ce courrier
électronique a été vérifiée par le
logiciel antivirus Avast. https://www.avast.com/antivirus
M3 - Article in specialist publication
VL - 26098
JO - GRB Coordinates Network, Circular Service
JF - GRB Coordinates Network, Circular Service
ER -