ASASSN-16hy: Discovery of A Probable Supernova in UGC 09857

ATel #9305; J. Brimacombe (Coral Towers Observatory), J. S. Brown (Ohio State), Subo Dong (KIAA-PKU), T. W.-S. Holoien, K. Z. Stanek, C. S. Kochanek, J. Shields, D. Godoy-Rivera, U. Basu (Ohio State), B. J. Shappee (Hubble Fellow, Carnegie Observatories), J. L. Prieto (Diego Portales; MAS), D. Bersier (LJMU), S. Bose, Ping Chen (KIAA-PKU), G. Masi (Virtual Telescope Project, Ceccano, Italy), R. S. Post (Post Astronomy)
on 3 Aug 2016; 15:38 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Jonathan Brown (brown@astronomy.ohio-state.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 UGC 09857.

ASASSN-16hy (AT 2016enk) was discovered in images obtained on UT 2016-08-03.210 at V~16.5 mag. We also detect the object in images obtained on UT 2016-07-31.27 (V~17.4). We do not detect (V>18.5) the object in images taken on UT 2016-07-27.33 and before. An image obtained on 2016-08-03 by J. Brimacombe confirms the discovery of the transient. This figure shows the archival SDSS g-band 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-16hy is approximately 32.6" North and 20.7" West from the center of the galaxy UGC 09857 (z=0.007799, d=33.5 Mpc, via NED), giving an absolute V-band magnitude of approximately -16.2 (m-M=32.61, A_V=0.068). 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-16hy  15:26:29.523   +41:44:03.32     2016-08-03.210      16.5          -16.2               38.62 

 
Obs. UT Date         V mag 
2016-07-27.33        >18.5 
2016-07-31.27         17.4 
2016-08-03.21         16.5 

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, the Mt. Cuba Astronomical Foundation, George Skestos, and the Robert Martin Ayers Sciences Fund. For more information about the ASAS-SN project, see the ASAS-SN Homepage and the list of all ASAS-SN transients.