PI: Benjamin Shappee, U. of Hawaii, email@example.com
Address: Institute for Astronomy, 2680 WOODLAWN DRIVE, HONOLULU, HI 96822 USA
CoI: Juna Kollmeier, Carnegie Institution of Washington
CoI: Subo Dong, Peking University
CoI: Jose Luis Prieto, Universidad Diego Portales
Title: What Are Type-Ia Supernovae?
Abstract: Type Ia supernovae (SN Ia) currently serve as the astrophysical backbone of the cosmic distance scale due to their property as cosmological standardizable candles (Phillips 1993). What is truly remarkable, is that despite their critical use in this capacity, we do not currently know a) what their progenitors are and b) what physical mechanism makes them explode. Here we propose to address this outstanding issue by building a sample of high-signal-to-noise, late-time, nebular-phase spectroscopic LBT/MODS observations of a local sample of Type Ia Supernova. In particular, by measuring the velocities and line profiles of the supernova ejecta we can constrain the kinematic of the explosion and distinguish between progenitor models.
Program Type: Standard/Extragalactic
Run 1 (2018A): LBT-SVC/MODS -- 20hrs
National Optical Astronomy Observatory, 950 North Cherry Avenue, P.O. Box 26732, Tucson, Arizona 85726, Phone: (520) 318-8000, Fax: (520) 318-8360