The Spectral Classification of Astronomical Transients (SCAT) survey (ATel #11444) presents the classification of 7 optical transients. We report optical spectroscopy (330-970nm, R~1200) taken with the University of Hawaii 88-inch (UH88) telescope using the SuperNova Integral Field Spectrograph (SNIFS). Transients were classified using the SuperNova IDentification code (SNID, Blondin & Tonry 2007, ApJ, 666, 1024). Additionally, we use photometry from the All-Sky Automated Survey for SuperNovae (ASAS-SN, Shappee et al. 2014, ApJ, 788, 48) to more accurately constrain the phase of each object. Redshifts given to 2 decimal places are derived supernova lines (via SNID), otherwise the redshifts are taken from NED or measured from narrow host galaxy emission lines.
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 | 2019ktf [ATLAS19oqd] | 23:32:29.939 | -29:33:36.66 | SN Ia | 0.05 | 23:32:29.893 | -29:33:37.13 | SN Ia | 0.05 | |||
TNS | 2019kpv [ATLAS19one] | 23:47:05.597 | -34:42:34.78 | SN Ia | 0.0425 | 23:47:05.600 | -34:42:35.06 | SN Ia | 0.0425 | |||
TNS | 2019kcv [ATLAS19ohp] | 14:25:44.579 | -03:13:58.97 | SN Ia | 0.08 | Templates from Ia-norm and Ia-91T SNe provide similar results. | 14:25:44.578 | -03:13:58.89 | SN Ia | 0.073011 | ||
TNS | 2019kaj [ATLAS19ogn] | 23:28:20.334 | +19:33:29.80 | SN IIP | 0.04 | 23:28:20.350 | +19:33:29.70 | SN IIP | 0.04 | |||
TNS | 2019kah [ATLAS19oft] | 00:58:09.796 | -29:19:24.49 | SN IIP | 0.03411 | 00:58:09.796 | -29:19:24.49 | SN IIP | 0.03411 | |||
TNS | 2019jwq [ZTF19abcneik] | 12:55:54.639 | +48:45:04.00 | SN IIP | 0.035 | 12:55:54.630 | +48:45:04.03 | SN II | 0.035 | |||
TNS | 2019jzt [ATLAS19odx] | 00:54:32.221 | +34:22:41.68 | SN Ia-91T-like | 0.08 | SNID also provides several matches to pre-maximum SN Ia-norm templates, however, ATLAS first reported this object over two weeks ago. Considering the discovery date, we consider the post-max Ia-91T results more reasonable. | 00:54:32.212 | +34:22:41.83 | SN Ia-91T-like | 0.08 |
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