SN 2002gc
The UCB team took a spectrum with Keck-I telescope on Oct. 8, which shows
it was a type Ia SN with some peculiarities, A Si II/Ti II 580-nm absorption
feature (typical for subluminous SN Ia) was prominent, but Ti II 420-nm
absorption (also seen in subluminous SN Ia) was absent. Such characteristics
resembles that of SN Ia 2002eu which had a normal luminosity (vsnet-campaign-sn
483).