The Subluminous Supernova 2007qd: A Missing Link in a Family of Low-Luminosity Type Ia Supernovae
Colin M. McClelland, Peter M. Garnavich, Llu\'is Galbany, Ramon, Miquel, Ryan J. Foley, Alexei V. Filippenko, Bruce Bassett, J. Craig Wheeler,, Ariel Goobar, Saurabh W. Jha, Masao Sako, Joshua A. Frieman, Jesper, Sollerman, Jozsef Vinko, and Donald P. Schneider

TL;DR
SN 2007qd is a highly subluminous Type Ia supernova with intermediate properties, providing insights into the diversity of SN Ia explosions and their connection to other peculiar and low-luminosity events.
Contribution
This paper reports detailed photometric and spectroscopic observations of SN 2007qd, highlighting its unique properties and suggesting it as a missing link within the SN 2002cx-like supernova family.
Findings
SN 2007qd had an extremely fast rise time of <= 10 days.
It reached a peak absolute B magnitude of -15.4, making it one of the most subluminous SN Ia.
Its photospheric velocity was only 2800 km/s near maximum brightness.
Abstract
We present multi-band photometry and multi-epoch spectroscopy of the peculiar Type Ia supernova (SN Ia) 2007qd, discovered by the SDSS-II Supernova Survey. It possesses physical properties intermediate to those of the peculiar SN 2002cx and the extremely low-luminosity SN 2008ha. Optical photometry indicates that it had an extraordinarily fast rise time of <= 10 days and a peak absolute B magnitude of -15.4 +/- 0.2 at most, making it one of the most subluminous SN Ia ever observed. Follow-up spectroscopy of SN 2007qd near maximum brightness unambiguously shows the presence of intermediate-mass elements which are likely caused by carbon/oxygen nuclear burning. Near maximum brightness, SN 2007qd had a photospheric velocity of only 2800 km/s, similar to that of SN 2008ha but about 4000 and 7000 km/s less than that of SN 2002cx and normal SN Ia, respectively. We show that the peak…
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