ASASSN-17fs and ASASSN-17fy: Discovery of Two Probable Supernovae
ATel #10358; J. Brimacombe (Coral Towers Observatory), P. Cacella (DogsHeaven Observatory), S. Kiyota (Variable Star Observers League in Japan), 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), R. A. Koff (Antelope Hills Observatory), R. S. Post (Post Astronomy), G. Stone (Sierra Remote Observatories), W. Wiethoff (University of Minnesota, Duluth)
on 8 May 2017; 16:54 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Jonathan Brown (firstname.lastname@example.org)
Subjects: Optical, Supernovae, Transient
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 two new transient sources, most likely supernovae, in the galaxies FAIRALL 0131 and 2MASX J09033237-2120017.
ASASSN-17fs (AT 2017dry) was discovered in images obtained on UT 2017-04-28.40 at V~17.2 mag. We do not detect (V>17.8) the object in images taken on UT 2017-04-25.310 and before. An image obtained on 2017-05-04 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-17fs is approximately 0.4" South and 0.5" West from the center of the galaxy FAIRALL 0131 (z=0.040415, d=169 Mpc, via NED), giving an absolute V-band magnitude of approximately -18.9 (m-M=36.06, A_V=0.063).
ASASSN-17fy (AT 2017dwq) was discovered in images obtained on UT 2017-05-04.05 at V~16.9 mag. We do not detect (V>18.0) the object in images taken on UT 2017-04-24.10 and before. Follow-up images obtained on 2017-05-06 confirm 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 P. Cacella confirmation image (right). The red circle has a radius of 5" and is centered on the position of the transient in the P. Cacella image.
The position of ASASSN-17fy is approximately 1.8" South and 1.7" East from the center of the galaxy 2MASX J09033237-2120017 (z=0.018199, d=80.1 Mpc, via NED), giving an absolute V-band magnitude of approximately -18.0 (m-M=34.48, A_V=0.435). 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-17fs 22:32:44.530 -59:28:18.05 2017-04-28.40 17.2 -18.9 0.64
ASASSN-17fy 09:03:32.468 -21:20:02.73 2017-05-04.05 16.9 -18.0 2.48
Obs. UT Date V mag
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.