ASAS-SN Discovery of A Probable Supernova in ESO 357-G005
ATel #8099; J. Brimacombe (Coral Towers Observatory), P. Marples (Leyburn Observatory, Australia), S. Kiyota (Variable Star Observers League in Japan), G. Bock (Runaway Bay Observatory, Australia), J. S. Brown, K. Z. Stanek, T. W.-S. Holoien, C. S. Kochanek, D. 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), E. Falco (CfA), P. R. Wozniak (LANL), G. Pojmanski (Warsaw University Observatory), I. Cruz (Cruz Observatory), R. A. Koff (Antelope Hills Observatory), J. Nicolas (Groupe SNAUDE, France)
on 27 Sep 2015; 17:31 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Jonathan Brown (email@example.com)
Subjects: Optical, Supernovae, Transient
Referred to by ATel #: 8105
During the ongoing All Sky Automated Survey for SuperNovae (ASAS-SN or "Assassin"), using data from the quadruple 14-cm "Cassius" telescope in Cerro Tololo, Chile, we discovered a new transient source, most likely a supernova, in the galaxy ESO 357-G005.
ASASSN-15pz was discovered in images obtained on UT 2015-09-27.16 at V~16.4 mag. We do not detect (V>16.5) the object in images taken on UT 2015-09-26.16 and before. An image obtained on 2015-09-27 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-15pz is approximately 16.34" North and 14.45" West from the center of the galaxy ESO 357-G005 (z=0.014903, d=60.1 Mpc, via NED), giving an absolute V-band magnitude of approximately -17.5 (m-M=33.90, A_V=0.049). 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-15pz 03:08:48.443 -35:13:50.89 2015-09-27.16 16.4 -17.5 21.81
Obs. UT Date V mag
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 the Center for Cosmology and AstroParticle Physics (CCAPP) at OSU. For more information about the ASAS-SN project, see the ASAS-SN Homepage and the list of all ASAS-SN transients.