We conducted follow-up imaging and spectroscopy of the candidate supernova GSNST-20ca (AT 2020rml; TNS report 80195) using the Liverpool Telescope as part of a live observing session during the Global Relay of Observatories Watching Transients Happen (GROWTH) online astronomy school. We obtained one 180s image in each of the g, r, and i band filters with IO:O between 03:38 and 03:48 UT on 2020-08-19, followed by two spectroscopic exposures of 600 seconds with SPRAT.
Image subtraction of the IO:O images versus Pan-STARRS reference imaging shows no source at the location of the reported transient, to an estimated limiting magnitude of approximately 22. The extracted spectrum shows only host galaxy light at z=0.018, consistent with the catalogued redshift of the host galaxy. We thus cannot confirm the presence of a transient in this galaxy, unless it faded very rapidly from the reported discovery three days prior.
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 | 2020rml [GSNST-20ca] | 01:24:27.398 | +33:47:56.53 | NGC 513 | 0.019544 | Catalog redshift from NED. | 01:24:27.398 | +33:47:56.53 |
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