Supernova 2012ec: identification of the progenitor and early monitoring with PESSTO.
Sollerman, J.; Gal-Yam, A.; Inserra, C.; Smartt, S. J.; Maund, J. R.; Taddia, F.; Fraser, M.; Botticella, M. T.; Pignata, G.; Valenti, S.; Reichart, D.; Tomasella, L.; Barbarino, C.; Yaron, O.; Childress, M.; Schmidt, B.
United Kingdom, Denmark, Italy, Australia, Israel, Chile, United States, Sweden
Abstract
We present the identification of the progenitor of the Type IIP SN 2012ec in archival pre-explosion Hubble Space Telescope Wide Field Planetary Camera 2 (WFPC2) and Advanced Camera for Surveys Wide Field Channel F814W images. The properties of the progenitor are further constrained by non-detections in pre-explosion WFPC2 F450W and F606W images. We report a series of early photometric and spectroscopic observations of SN 2012ec. The r'-band light curve shows a plateau with M_{r^' }}=-17.0. The early spectrum is similar to the Type IIP SN 1999em, with the expansion velocity measured at Hα absorption minimum of -11 700 km s-1 (at 1 d post-discovery). The photometric and spectroscopic evolution of SN 2012ec shows it to be a Type IIP SN, discovered only a few days post-explosion (<6 d). We derive a luminosity for the progenitor, in comparison with MARCS model spectral energy distributions, of log {L/L}_{⊙} = 5.15± 0.19, from which we infer an initial mass range of 14-22 M⊙. This is the first SN with an identified progenitor to be followed by the Public ESO Spectroscopic Survey of Transient Objects (PESSTO).