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GCN Circular 34060

Subject
ZTF23aaoohpy/AT2023lcr: SAO RAS observations
Date
2023-06-22T13:17:37Z (a year ago)
From
Moskvitin Alexander at SAO RAS <mosk@sao.ru>
A. Moskvitin (SAO RAS), O. Spiridonova (SAO RAS), S. Belkin (IKI RAS,
HSE), A. Pozanenko (IKI RAS), report on behalf of a larger
collaboration.

We observed the field of the fast red optical transient
ZTF23aaoohpy/AT2023lcr (Swain et al., GCN 34022) with the 1-m
telescope of SAO RAS Zeiss-1000/CCD-photometer. We obtained 8 x 300
sec images in Rc band on 2023.06.21, 21:06:39--21:52:39 UT, 3.8347
days after GOTO detection (Gompertz et al., GCN 34023) or 3.7432 days
after ZTF detection (Swain et al., GCN 34022).

The OT (Swain et al., GCN 34022; Gompertz et al., GCN 34023; Kumar et
al., GCN 34025; Adami et al., GCN 34030; Perley et al., GCN 34031;
Jiang et al., GCN 34040; Perley et al., GCN 34041; Fulton et al., GCN
34042; Chen et al., GCN 34043, Belkin et al., GCN 34047; Breeveld, GCN
34049; Leonini et al., GCN 34052) is clearly detected in the stacked
frame with the brightness of R = 21.51 +/- 0.09 (based on stars
mentioned in Belkin et al., GCN 34047).


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