GCN Circular 28644
Subject
GRB 201014A: Swift/UVOT Upper Limits
Date
2020-10-16T04:29:10Z (4 years ago)
From
Sam LaPorte at PSU <sjl5346@psu.edu>
GRB 201014A: Swift/UVOT Upper Limits
J. D. Gropp (PSU) and E. Ambrosi (INAF-IASFPA)
report on behalf of the Swift/UVOT team:
The Swift/UVOT began settled observations of the field of GRB 201014A
176 s after the BAT trigger (Ambrosi et al., GCN Circ. 28623) .
No optical afterglow consistent with the XRT position
(D'Elia et al., GCN Circ. 28626)
is detected in the initial UVOT exposures.
Preliminary 3-sigma upper limits using the UVOT photometric system
(Breeveld et al. 2011, AIP Conf. Proc. 1358, 373) for the first
finding chart (FC) exposure and subsequent exposures are:
Filter T_start(s) T_stop(s) Exp(s) Mag
b 3291 3483 38 >19.17
uvm2 7457 7657 196 >19.18
u 3035 7877 275 >19.82
v 3365 7452 235 >19.24
uvw1 3414 7862 216 >19.25
uvw2 3514 7248 216 >19.32
white 2876 7042 382 >21.14
The magnitudes in the table are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 0.05 in the direction of the burst
(Schlegel et al. 1998).
<https://www.avast.com/sig-email?utm_medium=email&utm_source=link&utm_campaign=sig-email&utm_content=webmail&utm_term=icon>
Virus-free.
www.avast.com
<https://www.avast.com/sig-email?utm_medium=email&utm_source=link&utm_campaign=sig-email&utm_content=webmail&utm_term=link>
<#DAB4FAD8-2DD7-40BB-A1B8-4E2AA1F9FDF2>