DRAFT
2020-07-31 15:27:40
Type: Object/s-Discovery/Classification
Bibcode: 2020TNSAN.149....1D
Spectroscopic classification of the bright NIR transient PGIR20eid/SN2020qmp as a young Type II supernova in UGC07125
Source Group: Gattini
Abstract:
We report spectroscopic classification of the bright NIR transient PGIR20eid/SN2020qmp as a young Type II supernova in UGC07125.
The bright NIR transient PGIR20eid/AT2020qmp was discovered by the Palomar Gattini-IR survey (De et al. 2020; Moore and Kasliwal 2019) on UT 2020-07-30 and reported as a young supernova candidate in UGC07125 (ATel #13909, Astronote 2020-147). On UT 2020-07-31, we obtained a low resolution optical spectrum of the source with the SED Machine spectrograph (Blagorodnova et al. 2018) on the Palomar 60-inch telescope.
The spectrum shows broad P-Cygni features of the Balmer series and He I. Using SNID (Blondin and Tonry 2007) on the spectrum, we find a best match to the Type IIP SN 1999em at peak light, indicating a young Type II supernova. Further spectroscopic and photometric follow-up of this very nearby supernova is encouraged.
| 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 | 2020qmp [PGIR20eid] | 12:08:44.430 | +36:48:19.36 | SN II | 0.003 | 12:08:44.440 | +36:48:17.28 | SN II | 0.003 |
Comments