ASASSN-17bn: Discovery of A Probable Supernova in 2MASX J08592386-0952291
ATel #10030; J. Brimacombe (Coral Towers Observatory), R. S. Post (Post Astronomy), 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), 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), R. A. Koff (Antelope Hills Observatory), G. Krannich (Roof Observatory Kaufering), G. Masi (Virtual Telescope Project, Ceccano, Italy), B. Nicholls (Mt. Vernon Obs., New Zealand), G. Stone (Sierra Remote Observatories)
on 31 Jan 2017; 20:10 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Jonathan Brown (brown@astronomy.ohio-state.edu)
Subjects: Optical, Supernovae, Transient
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 2MASX J08592386-0952291.
ASASSN-17bn (AT 2017vu) was discovered in images obtained on UT 2017-01-21.43 at V~17.6 mag. We also detect the object in images obtained on UT 2017-01-31.48 (V~17.2), UT 2017-01-28.49 (V~17.5), and UT 2017-01-25.310 (V~17.8). We do not detect (V>17.9) the object in images taken on UT 2017-01-18.14 and before. An image obtained on 2016-01-29 by R. Post confirms the discovery of the transient. This figure shows the archival Pan-STARRS (Chambers et al. 2016, arXiv:1612.05560) g-band image of the host (left) and the R. Post confirmation image (right). The red circle has a radius of 5" and is centered on the position of the transient in the R. Post image.
The position of ASASSN-17bn is approximately 0.1" North and 0.6" East from the center of the galaxy 2MASX J08592386-0952291 (z=0.044507, d=194 Mpc, via NED), giving an absolute V-band magnitude of approximately -18.8 (m-M=36.34, A_V=0.101). 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-17bn 08:59:23.92 -09:52:29.32 2017-01-21.43 17.6 -18.8 0.61
Obs. UT Date V mag
2017-01-18.14 >17.9
2017-01-21.43 17.6
2017-01-25.31 17.8
2017-01-28.49 17.5
2017-01-31.48 17.2
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 Center for Cosmology and AstroParticle Physics (CCAPP) at OSU, the Chinese Academy of Sciences South America Center for Astronomy (CASSACA), and the Mt. Cuba Astronomical Foundation. For more information about the ASAS-SN project, see the ASAS-SN Homepage and the list of all ASAS-SN transients.
