Erratum to ATel #15175

ATel #15176; M. R. Siebert, R. J. Foley (UC Santa Cruz)
on 22 Jan 2022; 18:08 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Matthew Siebert (msiebert@ucsc.edu)

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In ATel #15175 SN2021aau should be SN2022aau. Below is a corrected version of ATel #15175.

We report the classification of SN 2022aau with the GMOS spectrograph on the Gemini-South Telescope with GMOS on UT 2022 Jan 21. The target was supplied by DLT40. The classification was performed with SNID (Blondin & Tonry, 2007, ApJ, 666, 1024).

 
Name    | IAU Name   | RA (J2000)  | Dec (J2000)  |    z     | Type  |  Phase  | Notes
 
DLT22b  | AT2022aau  | 04:45:41.83 | -59:14:43.87 | 0.004440 |  II   |  peak   | (1) 
 

Notes:
When the redshift is given to 2 decimal places, it is derived from the SN spectrum. Otherwise, the redshift is determined from the host galaxy.

(1) The red spectrum is consistent with a SN II that suffered significant host-galaxy reddening.