Abstract
We present observational data for a peculiar supernova discovered by the OGLE-IV survey and followed by the Public ESO Spectroscopic Survey for Transient Objects. The inferred redshift of z = 0.07 implies an absolute magnitude in the rest-frame I-band of M-1 similar to -17.6 mag. This places it in the luminosity range between normal Type Ia SNe and novae. Optical and near infrared spectroscopy reveal mostly Ti and Ca lines, and an unusually red color arising from strong depression of flux at rest wavelengths
Original language | English |
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Article number | L2 |
Number of pages | 7 |
Journal | The Astrophysical Journal Letters |
Volume | 799 |
Issue number | 1 |
DOIs | |
Publication status | Published - 09 Jan 2015 |
Keywords
- supernovae: general
- supernovae: individual (OGLE-2013-SN-079)
- surveys
- white dwarfs
- SUB-CHANDRASEKHAR SUPERNOVAE
- WHITE-DWARFS
- IA SUPERNOVAE
- MASS MODELS
- FAINT TYPE
- OBSERVABLES
- TRANSIENTS
- PHOTOMETRY
- EXPLOSION
- IB/C