ASASSN-17fr: Discovery of A Probable Supernova in IC 4296
ATel #10339; B. Nicholls (Mt. Vernon Obs., New Zealand), J. S. Brown, K. Z. Stanek, T. W.-S. Holoien, C. S. Kochanek, J. Shields, T. A. Thompson (Ohio State), B. J. Shappee (Hubble Fellow, Carnegie Observatories), J. L. Prieto (Diego Portales; MAS), D. Bersier (LJMU), Subo Dong, S. Bose, Ping Chen (KIAA-PKU), J. Brimacombe (Coral Towers Observatory), R. S. Post (Post Astronomy), G. Stone (Sierra Remote Observatories)
on 1 May 2017; 23:52 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Jonathan Brown (email@example.com)
Subjects: Optical, Supernovae, Transient
Referred to by ATel #: 10344
During the ongoing All Sky Automated Survey for SuperNovae (ASAS-SN, Shappee et al. 2014), 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 IC 4296.
ASASSN-17fr (AT 2017dps) was discovered in images obtained on UT 2017-05-01.28 at V~15.4 mag. We also detect the object in images obtained on UT 2017-04-28.13 (V~16.7). We do not detect (V>17.8) the object in images taken on UT 2017-04-27.14 and before. An image obtained on 2017-05-01 by B. Nicholls confirms the discovery of the transient. This figure shows the archival DSS image of the host (left) and the B. Nicholls confirmation image (right). The red circle has a radius of 5" and is centered on the position of the transient in the B. Nicholls image.
The position of ASASSN-17fr is approximately 4.1" South and 12.1" East from the center of the galaxy IC 4296 (z=0.012465, d=55.5 Mpc, via NED), giving an absolute V-band magnitude of approximately -18.5 (m-M=33.69, A_V=0.175). 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-17fr 13:36:40.000 -33:58:01.12 2017-05-01.28 15.4 -18.5 12.78
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-17xx 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-17xx (AT 2017xyz) to preserve, rather than anonymize, the origin of the transient.
We thank Las Cumbres Observatory and its staff for their continued support of ASAS-SN. ASAS-SN is funded in part by the Gordon and Betty Moore Foundation through grant GBMF5490 to the Ohio State University, NSF grant AST-1515927, the Mt. Cuba Astronomical Foundation, the Center for Cosmology and AstroParticle Physics (CCAPP) at OSU, and the Chinese Academy of Sciences South America Center for Astronomy (CASSACA). For more information about the ASAS-SN project, see the ASAS-SN Homepage and the list of all ASAS-SN transients.