Skip to main content
Due to the lapse in federal government funding, NASA is not updating this website. See the Operations FAQ for GCN impacts.
New! Super-Kamiokande JSON Notices and Schema v4.5.0. See news and announcements

GCN Circular 33607

Subject
GRB 230409B: OHP/T193 optical upper limit
Date
2023-04-12T13:30:17Z (2 years ago)
Edited On
2024-11-16T16:18:19Z (a year ago)
From
Benjamin Schneider at MIT <bschn@mit.edu>
Edited By
Judith Racusin at NASA/GSFC <judith.racusin@nasa.gov> on behalf of Leo P. Singer at NASA/GSFC <leo.p.singer@nasa.gov>
C. Adami (LAM), B. Schneider (MIT), S. Basa (LAM), 
E. Le Floc'h, D. Turpin, D. Götz (CEA Paris-Saclay), 
S. D. Vergani (GEPI, Obs. de Paris), report on behalf 
of a larger collaboration:

We observed the field of GRB 230409B (Beardmore et al., GCN 33592) 
using the T193cm telescope at Observatoire de Haute-Provence (France) 
equipped with the MISTRAL spectro-imager. Four exposures were obtained 
in the i-band (2x300s + 2x600s) from 2023 10 April 03:03:03 UT to 
2023 10 April 03:44:17 UT (mid time ~22.3h after trigger). In the combined 
frame, we do not detect any source at the position reported by Evans et al., 
GCN 33594 and Kuin et al., GCN 33595 down to the following 3-sigma limit:

i > 20.6 mag (AB)

The photometric calibration was performed using nearby stars from 
the PanSTARRS catalog and the magnitude is not corrected for Galactic 
extinction.

We acknowledge the excellent support from Observatoire de Haute-Provence, 
in particular Jean-Pierre Troncin.
Looking for U.S. government information and services? Visit USA.gov