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GCN Circular 37280

Subject

GRB 240825A: GMG Optical Observation

Date

2024-08-25T18:13:19Z (22 days ago)

Edited On

2024-08-25T20:36:57Z (22 days ago)

From

Rui-Zhi Li at Yunnan Observatories, CAS <liruizhi@ynao.ac.cn>

Edited By

Vidushi Sharma at NASA GSFC/UMBC <vidushi.sharma@nasa.gov> on behalf of Rui-Zhi Li at Yunnan Observatories, CAS <liruizhi@ynao.ac.cn>

Via

Web form

R.-Z. Li, B.-T. Wang, F.-F. Song, J. Mao, Y.-X. Xin, and J.-M. Bai (YNAO, CAS) report:

We observed the field of GRB 240825A (Gupta et al., GCN 37274Not found
 
 
, T0 at 2024-08-25T15:52:59) using the GMG-2.4m telescope at the Lijiang Observatory. The observation began at 2024-08-25T17:42:38, about 1.83 hours after the trigger.

The optical counterpart of GRB 240825A, not visible in the Pan-STARRS1 r-band image, was clearly detected at the coordinates (J2000):
RA  =  22h58m17.26s
DEC = +01d01'36.7"
, with a positional uncertainty of 0.5" or better. The position is consistent with Swift/UVOT (GCN 37274Not found
 
 
), Nanshan/HMT (GCN 37275Not found
 
 
), Skynet (GCN 37276Not found
 
 
) and AKO (GCN 37277Not found
 
 
).

The preliminary analysis results are shown as follows:
+----------------+------------+----------+--------------+----------------+
|  Tmid-T0 [hr]  |  Exp. [s]  |  Filter  |     Mag      |  5-sigma U.L.  |
+================+============+==========+==============+================+
|      1.91      |    600     |    R     | 18.97 ± 0.04 |       21       |
+----------------+------------+----------+--------------+----------------+ 
The given magnitudes are derived based on calibration against Pan-STARRS1 field stars, and are not corrected for the expected Galactic foreground extinction, corresponding to a reddening of E(B-V) = 0.053 mag in the direction of the optical counterpart (Schlafly & Finkbeiner 2011).

The optical spectroscopic observation is ongoing, but there are thin clouds in the sky.

We acknowledge the staff at the Lijiang Observatory for their efforts in conducting the observation. In particular, we extend our gratitude to the on-duty observers for promptly resolving the instrumental cooling problems with the GMG-2.4m telescope that arose during the night.