no code implementations • 22 Dec 2020 • Asier Castrillo, Yago Ascasibar, Lluís Galbany, Sebastián F. Sánchez, Carles Badenes, Joseph P. Anderson, Hanindyo Kuncarayakti, Joseph D. Lyman, Angeles I. Díaz
For SNe II and Ib/c, we find a correlation with a Gaussian DTD model with $\sigma = 82^{+129}_{-23}~Myr$ and $\sigma = 56^{+141}_{-9}~Myr$ (50\% C. I.)
Astrophysics of Galaxies High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics