Discovery of 8 ASAS-SN Supernova Candidates
ATel #15396; J. Brimacombe (Coral Towers Observatory), I. Cruz (Cruz Observatory), P. Cacella (DogsHeaven 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)
on 23 May 2022; 20:19 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 "Brutus" telescope in Haleakala, Hawaii, the quadruple 14-cm "Leavitt" telescope in Fort Davis, Texas, the quadruple 14-cm "Payne-Gaposchkin" telescope in Sutherland, South Africa, and the quadruple 14-cm "Cassius" and "Paczynski" telescopes in Cerro Tololo, Chile, we discovered several new transient sources. Properties of the supernovae, 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-22gq (AT 2022jqj) 21:55:22.447 -50:42:53.75 0.060749 2022-05-09.33 ~100.0 62.8 2.93
ASASSN-22gp (AT 2022jqd) 17:28:22.977 -61:08:40.87 Unk 2022-05-09.26 ~16.8 --- 13.56
ASASSN-22gn (AT 2022jmn) 01:23:04.339 -43:54:51.87 0.022185 2022-05-07.42 ~16.2 -18.6 0.81
ASASSN-22ft (AT 2022hod) 21:43:05.121 -17:32:43.75 0.036969 2022-04-14.37 ~17.3 -18.7 6.71
ASASSN-22fn (AT 2022hfo) 18:21:29.614 +17:16:16.07 Unk 2022-04-10.41 ~17.1 --- 18.82
ASASSN-22fm (AT 2022hfn) 22:23:28.214 -55:02:14.87 Unk 2022-04-10.41 ~17.3 --- 1.0
ASASSN-22eq (AT 2022frl) 15:21:33.203 -07:26:51.93 0.006430 2022-04-02.41 ~17.4 -15.2 1.36
ASASSN-22ep (AT 2022fpo) 20:20:49.305 -48:14:26.78 0.010194 2022-04-01.36 ~15.4 -17.8 6.94
Follow-up observations are encouraged.
While we are participating in the TNS system to minimize potential confusion, ASAS-SN will continue using ASASSN-22xx 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-22xx (AT 2022xyz) 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, and also funded in part by the Alfred P. Sloan Foundation grant G-2021-14192. For more information about the ASAS-SN project, see the ASAS-SN Homepage and the list of all ASAS-SN transients.
