The First Systematic Study of Type Ibc Supernova Multi-band Light Curves

• Published in: The Astrophysical journal Vol. 741; no. 2; pp. 97 - jQuery1323901833426='48'
• Main Authors: Drout, Maria R, Soderberg, Alicia M, Gal-Yam, Avishay, Cenko, S. Bradley, Fox, Derek B, Leonard, Douglas C, Sand, David J, Moon, Dae-Sik, Arcavi, Iair, Green, Yoav
• Format: Journal Article
• Language: English
• Published: Bristol IOP Publishing 10-11-2011; IOP
• Subjects: Astronomy; Color; Earth, ocean, space; Exact sciences and technology; Explosions; Extinction; Galaxies; Photometry; Samples; Statistical analysis; Statistical methods; gamma-ray burst: general; Galaxies; Cosmic gamma sources; Supernovae; Color; Light curves; Absolute magnitude; Luminosity; Probability; Gamma ray burst; supernovae: general; Models; Extinction curve; Kinetic energy; Photometry
• ISSN: 0004-637X; 1538-4357
• DOI: 10.1088/0004-637X/741/2/97

We present detailed optical photometry for 25 Type Ibc supernovae (SNe Ibc) within d 150 Mpc obtained with the robotic Palomar 60 inch telescope in 2004-2007. This study represents the first uniform, systematic, and statistical sample of multi-band SNe Ibc light curves available to date. We correct the light curves for host galaxy extinction using a new technique based on the photometric color evolution, namely, we show that the (V -- R) color of extinction-corrected SNe Ibc at Delta *Dt 10 days after V-band maximum is tightly distributed, (V -- R) V10 = 0.26 ? 0.06 mag. Using this technique, we find that SNe Ibc typically suffer from significant host galaxy extinction, E(B -- V) 0.4 mag. A comparison of the extinction-corrected light curves for helium-rich (Type Ib) and helium-poor (Type Ic) SNe reveals that they are statistically indistinguishable, both in luminosity and decline rate. We report peak absolute magnitudes of MR = --17.9 ? 0.9 mag and MR = --18.3 ? 0.6 mag for SNe Ib and Ic, respectively. Focusing on the broad-lined (BL) SNe Ic, we find that they are more luminous than the normal SNe Ibc sample, MR = --19.0 ? 1.1 mag, with a probability of only 1.6% that they are drawn from the same population of explosions. By comparing the peak absolute magnitudes of SNe Ic-BL with those inferred for local engine-driven explosions (GRB-SN 1998bw, XRF-SN 2006aj, and SN 2009bb) we find a 25% probability that relativistic SNe are drawn from the overall SNe Ic-BL population. Finally, we fit analytic models to the light curves to derive typical 56Ni masses of M Ni 0.2 and 0.5 M for SNe Ibc and SNe Ic-BL, respectively. With reasonable assumptions for the photospheric velocities, we further extract kinetic energy and ejecta mass values of M ej 2 M and EK 1051 erg for SNe Ibc, while for SNe Ic-BL we find higher values, M ej 5 M and EK 1052 erg. We discuss the implications for the progenitors of SNe Ibc and their relation to those of engine-driven explosions.