CSP classifications of optical transients
ATel #6510; N. Morrell, C. Contreras, C. Gonzalez, M. M. Phillips (Las Campanas Observatory), E. Y. Hsiao, M. Stritzinger, C. Gall, S. Holmbo (Aarhus University), Stu Parker, Peter Marples, Greg Bock, Colin Drescher, Patrick Pearl (BOSS), Paula Sanchez, Paulina Lira (Universidad de Chile), T. W.-S. Holoien, K. Z. Stanek, C. S. Kochanek, A. B. Davis, U. Basu, J. F. Beacom (Ohio State), B. J. Shappee (Hubble Fellow, Carnegie Observatories), J. L. Prieto (Diego Portales, MAS), D. Bersier (LJMU), J. Brimacombe (Coral Towers Observatory), D. Szczygiel, G. Pojmanski (Warsaw University Observatory)
on 28 Sep 2014; 17:09 UT
Distributed as an Instant Email Notice Supernovae
Credential Certification: Eric Hsiao (hsiao@lco.cl)
Subjects: Optical, Supernovae
Carnegie Supernova Project reports the optical spectroscopic classifications of five transients. The spectra were obtained on Sep 28 UT with the Las Campanas 2.5-m du Pont telescope (+ WFCCD).
Name | Source | RA | Dec | z | Type | Phase | Notes
------------------------|--------|-------------|--------------|----------|-------------|-------|------
ASASSN-14hu | ASASSN | 01:50:41.27 | -14:31:04.75 | 0.015 | Ia | -5 | 1
PSN J04175427-5636452 | BOSS | 04:17:54.27 | -56:36:45.2 | 0.022189 | Ia-pec | +3 | 2
MLS140923:021229+111718 | CRTS | 02:12:29.14 | +11:17:18.1 | 0.045 | Ia | +30 | 3
Notes
1) The discovery was reported in ATel #6505. The redshift is derived from the SN spectrum.
2) The spectrum is similar to that of SN1999by at 3 days past maximum.
3) The redshift is derived from the SN spectrum.
