ASASSN-16cc: Discovery of A Probable Supernova in NGC 2101
ATel #8736; J. S. Brown (Ohio State), D. Bersier (LJMU), K. Z. Stanek, T. W.-S. Holoien, C. S. Kochanek, D. Godoy-Rivera, U. Basu (Ohio State), B. J. Shappee (Hubble Fellow, Carnegie Observatories), J. L. Prieto (Diego Portales; MAS), Subo Dong, Ping Chen (KIAA-PKU), J. Brimacombe (Coral Towers Observatory), G. Bock (Runaway Bay Observatory, Australia), I. Cruz (Cruz Observatory), J. M. Fernandez (Observatory Inmaculada del Molino), S. Kiyota (Variable Star Observers League in Japan), G. Masi (Virtual Telescope Project, Ceccano, Italy)
on 26 Feb 2016; 12:40 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Jonathan Brown (email@example.com)
Subjects: Optical, Supernovae, Transient
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 NGC 2101.
ASASSN-16cc (AT 2016aqf) was discovered in images obtained on UT 2016-02-26.19 at V~15.8 mag. We do not detect (V>16.8) the object in images taken on UT 2016-02-24.19 and before. This figure shows the ASAS-SN V-band reference image (left), the ASAS-SN discovery image (middle), and the archival DSS image of the host (right). The red circle has a radius of 10" and is centered on the position of the transient in the discovery image.
The position of ASASSN-16cc is approximately 0.2" South and 2.4" West from the center of the galaxy NGC 2101 (z=0.004016, d=17.5 Mpc, via NED), giving an absolute V-band magnitude of approximately -15.6 (m-M=31.22, A_V=0.151). 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-16cc 05:46:23.907 -52:05:18.86 2016-02-26.19 15.8 -15.6 2.41
Obs. UT Date V mag
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 (AT2016yy) 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.