Discovery of A Probable Supernova in KUG 1201+220

ATel #9724; J. Brimacombe (Coral Towers Observatory), R. S. Post (Post Astronomy), S. Kiyota (Variable Star Observers League in Japan), G. Stone (Sierra Remote Observatories), J. Shields, K. Z. Stanek, C. S. Kochanek, J. S. Brown, T. W.-S. Holoien (Ohio State), B. J. Shappee (Hubble Fellow, Carnegie Observatories), J. L. Prieto (Diego Portales; MAS), D. Bersier (LJMU), Subo Dong, S. Bose, Ping Chen (KIAA-PKU), G. Masi (Virtual Telescope Project, Ceccano, Italy)
on 7 Nov 2016; 16:51 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Krzysztof Stanek (stanek.32@osu.edu)

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During the ongoing All Sky Automated Survey for SuperNovae (ASAS-SN or "Assassin"), using data from the quadruple 14-cm "Brutus" telescope in Haleakala, Hawaii, we discovered a new transient source, most likely a supernova, in the galaxy KUG 1201+220.

ASASSN-16mz (AT 2016hwn) was discovered in images obtained on UT 2016-11-06.64 at V~17.1 mag. We also detect the object in images obtained on two other epochs. We do not detect (V>16.8) the object in images taken on UT 2016-06-20.2 and before. An image obtained on 2016-11-07 by J. Brimacombe confirms the discovery of the transient. This figure shows the archival DSS image of the host (left) and the J. Brimacombe confirmation image (right). The red circle has a radius of 5" and is centered on the position of the transient in the J. Brimacombe image.

The position of ASASSN-16mz is approximately 9.1" North and 5.8" East from the center of the galaxy KUG 1201+220 (z=0.021451, d=94.1 Mpc, via NED), giving an absolute V-band magnitude of approximately -17.8 (m-M=34.87, A_V=0.063). Properties of the new source and photometry are summarized in the tables below:

 
Object       RA (J2000)     DEC (J2000)     Disc. UT Date   Disc. V mag  Approx. Abs. Mag   Offset from Host (") 
ASASSN-16mz  12:04:16.906   +21:48:03.3     2016-11-06.63      17.1          -17.8               10.8 

 
Obs. UT Date       V mag  mag_err 
2016-06-20.26     >16.83   
2016-11-04.64      16.83  0.15 
2016-11-06.63      17.08  0.18 
2016-11-07.63      16.73  0.13 

Follow-up observations are encouraged.

While we are participating in the TNS system to minimize potential confusion, ASAS-SN will continue using ASASSN-16xx 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-16xx (AT2016xyz) to preserve, rather than anonymize, the origin of the transient.

We thank LCOGT and its staff for their continued support of ASAS-SN. ASAS-SN is supported by NSF grant AST-1515927, the Center for Cosmology and AstroParticle Physics (CCAPP) at OSU, and the Mt. Cuba Astronomical Foundation. For more information about the ASAS-SN project, see the ASAS-SN Homepage and the list of all ASAS-SN transients.