Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S295(8), p. 321-321, 2012
DOI: 10.1017/s1743921313005231
Full text: Unavailable
AbstractWe study and compare the stellar populations of host galaxies of different types of supernovae (SNe): SN Ia and core collapse SN (SN II and SN Ibc) at the same time. The 234 sample galaxies are selected by cross-matching the Asiago Supernova Catalogue (ASC) and the SDSS-DR7 main galaxy sample (MGS). The STARLIGHT software is used to analyze their stellar populations by fitting the continua and absorption lines of the hosts.