ASASSN-17dv and ASASSN-17ed: Discovery of Two Probable Supernovae
ATel #10226; J. Brimacombe (Coral Towers Observatory), R. S. Post (Post Astronomy), 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), G. Masi (Virtual Telescope Project, Ceccano, Italy)
on 29 Mar 2017; 21:32 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 and the 14-cm "Brutus" telescope in Haleakala, Hawaii, we discovered two new transient sources, most likely supernovae, in the galaxies GALEXASC J095231.21-215754.7 and AM 0440-442.
ASASSN-17dv (AT 2017civ) was discovered in images obtained on UT 2017-03-22.34 at V~17.9 mag. We do not detect (V>18.2) the object in images taken on UT 2017-03-19.30 and before. Follow-up images obtained on 2017-03-23 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 S. Kiyota confirmation image (right). The red circle has a radius of 5" and is centered on the position of the transient in the S. Kiyota image.
The position of ASASSN-17dv is approximately 0.2" North and 0.2" East from the center of the galaxy GALEXASC J095231.21-215754.7 (no redshift information available from NED).
ASASSN-17ed (AT 2017cnn) was discovered in images obtained on UT 2017-03-16.06 at V~16.8 mag. We do not detect (V>16.8) the object in images taken on UT 2017-03-15.11 and before. An image obtained on 2017-03-17 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-17ed is approximately 9.9" South and 4.0" West from the center of the galaxy AM 0440-442 (z=0.040308, d=171 Mpc, via NED), giving an absolute V-band magnitude of approximately -19.3 (m-M=36.08, A_V=0.032). Properties of the new sources 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-17dv 09:52:31.221 -21:57:54.59 2017-03-22.34 17.9 N/A 0.28
ASASSN-17ed 04:42:28.250 -44:15:04.43 2017-03-16.06 16.8 -19.3 10.68
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 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.