ASAS-SN Discovery of A Probable Supernova in KUG 1457+066
ATel #8463; S. Kiyota (Variable Star Observers League in Japan), T. W.-S. Holoien, K. Z. Stanek, C. S. Kochanek, J. S. Brown, D. Godoy-Rivera, U. Basu (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), G. Bock (Runaway Bay Observatory, Australia), R. A. Koff (Antelope Hills Observatory), G. Masi (Virtual Telescope Project, Ceccano, Italy), L. A.G. Monard (Klein Karoo Observatory)
on 24 Dec 2015; 18:03 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Thomas Holoien (email@example.com)
Subjects: Optical, Supernovae, Transient
Referred to by ATel #: 8543
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 1457+066.
ASASSN-15ul was discovered in images obtained on UT 2015-12-23.64 at V~16.9 mag. We do not detect (V>15.14) the object in images taken on UT 2015-12-16.67 and before. An image obtained by S. Kiyota on UT 2015-12-24.23 using a 0.43m CDK + STL-11000M at the ITelescope.NET site at Nerpio, Spain confirms the discovery of the transient. This figure shows archival DSS image of the host (left) and the S. Kiyota confirmation image (right). The red circle has a radius of 4" and is centered on the position of the transient in the S. Kiyota image.
The position of ASASSN-15ul is approximately 2.2" North and 1.3" East from the center of the galaxy KUG 1457+066 (z=0.029791, d=128 Mpc, via NED), giving an absolute V-band magnitude of approximately -18.7 (m-M=35.54, A_V=0.089). 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-15ul 15:00:27.68 +06:27:19.31 2015-12-23.64 16.9 -18.7 2.56
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, the Center for Cosmology and AstroParticle Physics (CCAPP) at OSU, 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.