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Discovery of Nine ASAS-SN Supernovae

ATel #10992; J. Brimacombe (Coral Towers Observatory), P. Cacella (DogsHeaven Observatory), J. G. Carballo (Observatorio Cerro del Viento MPC 184), R. G. Farfan (Uraniborg Observatory, Sevilla, Spain), R. A. Koff (Antelope Hills Observatory), B. Nicholls (Mt. Vernon Obs., New Zealand), R. S. Post (Post Astronomy), G. Stone (Sierra Remote Observatories), P. Vallely, K. Z. Stanek, J. S. Brown, C. S. Kochanek, J. V. 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), E. Conseil (Association Francaise des Observateurs d'Etoiles Variables)
on 21 Nov 2017; 21:57 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Krzysztof Stanek (stanek.32@osu.edu)

Subjects: Optical, Supernovae

Referred to by ATel #: 10994

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, 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. V/g mag  Approx. Abs. Mag   Offset from Host (") 
ASASSN-17pl  (AT 2017ijw)  17:08:45.105   42:16:58.60    0.046539     2017-11-17.09       ~18.6          -18.1               0.5 
ASASSN-17pj  (AT 2017iim)  20:40:09.54   -71:06:27.7     0.012619     2017-11-20.08       ~16.6          -17.1              18.1 
ASASSN-17pi  (AT 2017iha)  08:57:28.538   28:37:00.52    0.047931     2017-11-19.43       ~17.5          -19.2               0.1 
ASASSN-17ph  (AT 2017igs)  06:23:38.594  -35:38:23.22    0.030241     2017-11-17.25       ~16.4          -19.3               7.7 
ASASSN-17pg  (SN 2017igf)  17:08:45.105   42:16:58.60    0.005624     2017-11-18.59       ~15.9          -16.1               0.2 
ASASSN-17pe  (AT 2017ige)  17:08:45.105   42:16:58.60    0.024319     2017-11-17.65       ~16.9          -18.2               1.1 
ASASSN-17pa  (AT 2017icv)  23:08:08.423  -37:34:11.53     N/A         2017-11-14.10       ~18.3            N/A               1.3 
ASASSN-17oy  (AT 2017icu)   0:54:44.796  -50:00:35.70    0.048313     2017-11-13.16       ~18.1          -18.5               0.9 
ASASSN-17ox  (AT 2017ict)   0:25:01.794  -37:59:05.33     N/A         2017-11-11.16        ~18.6           N/A              12.2 

Follow-up observations are encouraged.

While we are participating in the TNS system to minimize potential confusion, ASAS-SN will continue using ASASSN-17xx 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-17xx (AT 2017xyz) to preserve, rather than anonymize, the origin of the transient.

We 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, and the Chinese Academy of Sciences South America Center for Astronomy (CASSACA). For more information about the ASAS-SN project, see the ASAS-SN Homepage and the list of all ASAS-SN transients.