The CCCP is a
large observational study of core-collapse SNe. Uniform, high-quality NIR and optical
photometry and multi-epoch optical spectroscopy have been obtained using the
200" Hale and robotic 60" telescopes at Palomar, for a sample of 50 nearby core-collapse
SNe. The combination of both well-sampled optical light curves and multiepoch
spectroscopy will allow to disentangle spectroscopically and photometrically
based subtype definitions. Multi-epoch spectroscopy is crucial to identify transition
events that evolve among subtypes with time (e.g., SNe IIb, initially similar to H-rich
SNe II, but later evolving into H-poor and He-rich SNe Ib - several such events have
been identified among the CCCP sample). The CCCP SN sample includes every corecollapse
SN discovered between July 2004 and September 2005 that was visible from
Palomar, found shortly (< 30 days) after explosion (based on available pre-explosion
photometry), and was closer than ~120 Mpc. This complete sample allows, for the first
time, a study of core-collapse SNe as a population, rather than as individual events.
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Credit: R. Scheps
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