GCN Circular 31389

R. Strausbaugh (U. of the Virgin Islands), A. Cucchiara (College of Marin) report on behalf of a larger collaboration:

We observed Swift GRB 220101A (Tohuvavohu, et al., GCN 31347
Not found
 
 
) for a third time with the LCO 1-m Sinistro instrument at the Teide Observatory, Tenerife site, on January 4, from 21:35 to 22:02 UT (corresponding to 88.43 to 88.88 hours from the GRB trigger time) with the Bessel R and I filters.

We performed a series of 2x500s exposures in R and I bands. We still detect the source at the UVOT detection coordinates and other optical observations (Tohuvavohu et al., GCN 31347
Not found
 
 
; Kuin & Tohuvavohu, GCN 31351
Not found
 
 
; Fu et al., GCN 31353
Not found
 
 
; Hentunen et al., GCN 31356
Not found
 
 
;
Perley et al., GCN 31357
Not found
 
 
; de Ugarte Postigo et al., GCN 31358
Not found
 
 
; Fynbo et al., GCN 31359
Not found
 
 
; Vinko et al., GCN 31361
Not found
 
 
; Tomasella et al., GCN 31363
Not found
 
 
; Mao et al., GCN 31364
Not found
 
 
; Noschese et al., GCN 31366
Not found
 
 
; Mao et al., GCN 31368
Not found
 
 
; Guelbenzu, et al., GCN 31370
Not found
 
 
; Strausbaugh et al., GCN 31371
Not found
 
 
, D'Avanzo et al., GCN 31373
Not found
 
 
; Strausbaugh et al., GCN 31383
Not found
 
 
; Dimple et al., GCN 31384
Not found
 
 
; Romanov, GCN 31387
Not found
 
 
; Caballero-Garcia, GCN 31388
Not found
 
 
) in both bands. The following magnitudes are calculated using the USNO-B.1 catalog as reference:

R=21.31+/-0.18
I=20.43+/-0.12

These magnitudes are not corrected for galactic extinction.

R.S. is funded by NSF AST grant #1831682