Discovery of 11 ASAS-SN Supernovae
ATel #11653; J. Brimacombe (Coral Towers Observatory), P. Cacella (DogsHeaven Observatory), G. Stone (Sierra Remote Observatories), J. M. Fernandez (Observatory Inmaculada del Molino), P. Vallely, K. Z. Stanek, C. S. Kochanek, J. S. Brown, J. Shields, 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, S. Bose, Ping Chen (KIAA-PKU), M. Stritzinger, S. Holmbo (Aarhus), B. Nicholls (Mt. Vernon Obs., New Zealand), R. S. Post (Post Astronomy)
on 18 May 2018; 21:40 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 14-cm telescopes in Hawaii, Texas, South Africa, and 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. V mag Approx. Abs. Mag Offset from Host (")
ASASSN-18kh (AT 2018bsh) 14:39:30.178 -35:11:21.12 Unk 2018-05-15.97 ~17.9 --- ---
ASASSN-18ke (AT 2018bsg) 10:10:28.160 +02:13:48.76 0.021686 2018-05-15.75 ~17.9 -17.2 8.35
ASASSN-18kd (AT 2018brz) 08:33:22.280 -76:37:39.86 Unk 2018-05-15.07 ~16.5 --- 3.99
ASASSN-18jv (AT 2018bkw) 10:22:52.670 -19:40:14.02 0.021512 2018-05-13.04 ~17.3 -17.8 2.24
ASASSN-18jp (AT 2018bfr) 11:04:47.468 -15:37:59.20 0.071746 2018-05-04.74 ~17.9 -19.7 9.74
ASASSN-18jo (AT 2018bfq) 09:38:14.907 -08:47:17.70 Unk 2018-05-05.72 ~17.7 --- 0.42
ASASSN-18jn (AT 2018bfh) 10:22:41.126 +15:56:21.49 0.044541 2018-05-06.16 ~17.0 -19.6 0.41
ASASSN-18jm (AT 2018bfg) 11:41:01.786 -33:40:47.32 Unk 2018-05-05.84 ~17.6 --- ---
ASASSN-18jl (AT 2018bfc) 23:22:58.447 -01:01:39.18 0.034266 2018-05-05.41 ~17.0 -18.9 2.55
ASASSN-18jk (AT 2018bfa) 10:15:30.230 -72:42:37.01 Unk 2018-05-05.04 ~16.8 --- ---
ASASSN-18ji (AT 2018beh) 09:31:23.028 +17:48:27.90 Unk 2018-05-04.04 ~17.4 --- 0.91
Follow-up observations are encouraged.
While we are participating in the TNS system to minimize potential confusion, ASAS-SN will continue using ASASSN-18xx transient names as our primary nomenclature, and we encourage others to do the same. We prefer merging the names as ASASSN-18xx (AT 2018xyz) 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 grant GBMF5490 to the Ohio State University, NSF grant AST-1515927, 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.
