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Discovery of 10 ASAS-SN Supernova Candidates

ATel #15030; J. Brimacombe (Coral Towers Observatory), B. Nicholls (Mt. Vernon Obs., New Zealand), I. Cruz (Cruz Observatory), P. Vallely, K. Z. Stanek, C. S. Kochanek, C. Christy, M. Rizzo Smith, S. Bose, T. A. Thompson (Ohio State), B. J. Shappee (IfA-Hawaii), T. W.-S. Holoien (Carnegie Observatories), J. L. Prieto (Diego Portales; MAS), D. Bersier (LJMU), Subo Dong (KIAA-PKU), M. Stritzinger (Aarhus), P. Pearl (The Gap Observatory, BOSS)
on 12 Nov 2021; 19:25 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Patrick Vallely (vallely.7@osu.edu)

Subjects: Optical, Supernovae, Transient

During the ongoing All Sky Automated Survey for SuperNovae (ASAS-SN, Shappee et al. 2014), using data from the quadruple 14-cm telescopes "Brutus" in Haleakala, Hawaii, "Leavitt" in Fort Davis, Texas, "Payne-Gaposchkin" in Sutherland, South Africa, and "Cassius" and "Paczynski" in Cerro Tololo, Chile, we discovered several new transient sources. Properties of these sources, as well as associated finding charts showing the archival imaging (left) and the follow-up confirmation image (right) are included in the table below:

 
Object                     RA (J2000)     DEC (J2000)    Redshift     Disc. UT Date   Disc. g mag    Approx. Abs. Mag   Offset from Host (") 
ASASSN-21ul (AT 2021adko)  00:54:17.942   -61:44:47.98   Unk          2021-11-03.04       ~17.3           ---           3.22 
ASASSN-21uk (AT 2021adkn)  07:29:56.439   -66:59:25.67   0.047586     2021-11-04.29       ~17.6          -19.4          0.22 
ASASSN-21uc (AT 2021acwp)  21:04:41.713   -37:47:36.78   0.031112     2021-10-30.15       ~17.8          -17.9          0.14 
ASASSN-21tw (AT 2021acgj)  03:43:16.760   -53:37:31.83   0.054831     2021-10-26.10       ~17.2          -19.7          0.22 
ASASSN-21tu (AT 2021aceu)  01:16:04.117   +37:38:55.62   0.030344     2021-10-25.13       ~17.3          -18.4          1.13 
ASASSN-21ts (AT 2021abyo)  02:34:11.404   -61:36:37.21   0.018950     2021-10-22.22       ~16.5          -18.0          8.33 
ASASSN-21tm (AT 2021abvm)  20:34:21.522   -54:59:20.46   0.040124     2021-10-17.03       ~17.0          -19.3          8.94 
ASASSN-21tk (AT 2021abko)  02:02:07.215   +23:32:59.94   0.015908     2021-10-14.52       ~17.0          -17.3          1.08 
ASASSN-21tf (AT 2021abjr)  10:21:39.266   +06:24:08.75   0.028842     2021-10-13.63       ~16.8          -18.8          0.3 
ASASSN-21td (AT 2021abcw)  10:35:45.302   +21:03:19.11   0.023486     2021-10-11.49       ~17.2          -17.9          25.49 

Follow-up observations are encouraged.

While we are participating in the TNS system to minimize potential confusion, ASAS-SN will continue using ASASSN-21xx transient names as our primary nomenclature (including supernovae, but also other classes of transients), and we encourage others to do the same. We prefer merging the names as ASASSN-21xx (AT 2021xyz) to preserve, rather than anonymize, the origin of the transient.

We would like to thank Las Cumbres Observatory and its staff for their continued support of ASAS-SN. ASAS-SN is funded in part by the Gordon and Betty Moore Foundation through grants GBMF5490 and GBMF10501, NSF grant AST-1908570, the Mt. Cuba Astronomical Foundation, the Center for Cosmology and AstroParticle Physics (CCAPP) at OSU, the Chinese Academy of Sciences South America Center for Astronomy (CASSACA), and the Villum Fonden (Denmark). For more information about the ASAS-SN project, see the ASAS-SN Homepage and the list of all ASAS-SN transients.