DRAFT
2023-08-17 21:03:02
Type: Object/s-Data/Analysis
Bibcode: 2023TNSAN.232....1K
Follow up of Optical Transients
Authors: M. R. Kendurkar (GSNST) and D. D. Balam (Dominion Astrophysical Observatory, National Research Council of Canada)
Source Group: WOTS
Keywords: Photometry, Cataclysmic Variable, Supernova, Optical
Abstract:
Here we present photometric follow up observations of 3 optical transients discovered by GOTO (M. Pursiaine., et al.), GEOTS (B. Kumar) and MASTER (T. Pogrosheva., et al.) using 0.33-m Telescope + KAF-3200E CCD of Western Optical Transient Survey, Canada.
                Name                       UT             CV
              2023pgr           2023-08-15.298       18.86 (0.12)
              2023pfd           2023-08-16.329       18.04 (0.13)
              2023pmd           2023-08-16.295       17.99 (0.12)


secondary standards are as follow; WISEA J234737.50+165910.2, 2MASS J23524766+5144339 and 2MASS J21562421+5704577. 

 

All the secondary standards were used from PS1 Survey DR1 (Chambers+, 2016) to perform differential photometry using Image Reduction and Analysis Facility (IRAF) (Tody, D. 1986, "The IRAF Data Reduction and Analysis System").

 

Show current TNS values
Catalog Name Reported RA Reported DEC Reported Obj-Type Reported Redshift Host Name Host Redshift Remarks TNS RA TNS DEC TNS Obj-Type TNS Redshift
TNS 2023pgr 23:47:33.190 +16:58:17.01 SN 0.08 23:47:33.204 +16:58:16.91 SN 0.08
TNS 2023pfd 23:53:44.406 +51:45:31.99 23:53:44.406 +51:45:31.99
TNS 2023pmd 21:56:26.220 +57:04:57.70 21:56:26.220 +57:04:57.70

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