ASAS-SN Discovery of A Probable Supernova in CGCC 226-005

ATel #8012; G. Masi (Virtual Telescope Project, Ceccano, Italy), J. S. Brown, K. Z. Stanek, T. W.-S. Holoien, C. S. Kochanek, Diego Godoy Rivera, G. Simonian, U. Basu, J. F. Beacom, T. A. Thompson (Ohio State), B. J. Shappee (Hubble Fellow, Carnegie Observatories), J. L. Prieto (Diego Portales; MAS), D. Bersier (LJMU), Subo Dong, Ping Chen (KIAA-PKU), J. Brimacombe (Coral Towers Observatory), E. Falco (CfA), P. R. Wozniak (LANL), G. Pojmanski (Warsaw University Observatory), S. Kiyota (Variable Star Observers League in Japan), B. Nicholls (Mt. Vernon Obs., New Zealand), I. Cruz (Cruz Observatory), E. Conseil (Association Francaise des Observateurs d'Etoiles Variables)
on 7 Sep 2015; 22:56 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 CGCC 226-005.

ASASSN-15pe was discovered in images obtained on UT 2015-09-07.28 at V~16.7 mag. We do not detect (V>17.3) the object in images taken on UT 2015-09-05.31 and before. An image obtained on 2015-09-07 by G. Masi confirms the discovery of the transient. This figure shows the archival SDSS g-band image of the host (left) and the G. Masi confirmation image (right). The red circle has a radius of 3" and is centered on the position of the transient in the G. Masi image.

The position of ASASSN-15pe is approximately 1.7" North and 4.8" West from the center of the galaxy CGCC 226-005 (z=0.037930, d=160 Mpc, via NED), giving an absolute V-band magnitude of approximately -19.4 (m-M=36.02, A_V=0.108). 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-15pe  17:20:15.353    39.15.39.40      2015-09-07.28      16.7          -19.4               5.09 

 
Obs. UT Date         V mag 
2015-09-05.31        >17.3 
2015-09-07.28         16.7 

Follow-up observations are encouraged.

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