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GCN Circular 44304

Subject
GOTO26djh/AT2026jpw transient: SAO RAS optical observations
Date
2026-04-16T00:39:58Z (5 days ago)
From
Alexander Moskvitin at SAO RAS <mosk@sao.ru>
Via
Web form
A. S. Moskvitin and O. I. Spiridonova (SAO RAS)
report on behalf of GRB follow-up team.

We observed the field of the fast-fading transient GOTO26djh/AT2026jpw
(O'Neill et al., GCN 44301) with the Zeiss-1000 1m telescope
of the SAO RAS on April 15/16 night. We obtained two series of images
in Rc band.

The OT (O'Neill et al., GCN 44301; Corcoran et al., GCN 44303) is clearly
detected in the stacked images with the following brightness.

Date        UT start t-T0       Exp.   Filter  OT        Err.  UL      
                     (mid,days) (n*s)                         (3sigma)
                     
2026-04-15T19:30:44  1.87945    8*300  Rc      21.6 +/- 0.1  23.3  
2026-04-15T22:01:13  1.97747   13*300  Rc      22.0 +/- 0.1  23.8

This preliminary photometry is based on nearby stars from the USNO-B1
catalogue (R2 magnitudes) and is not corrected for the Galactic
extinction.
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