Core-collapse supernovae (CCSNe) mark the deaths of stars more massive than about eight
times the mass of the Sun and are intrinsically the most common kind of catastrophic cosmic …

The final fate of massive stars, and the nature of the compact remnants they leave behind
(black holes and neutron stars), are open questions in astrophysics. Many massive stars are …

We present a new compilation of Type Ia supernovae (SNe Ia), a new data set of low-redshift
nearby-Hubble-flow SNe, and new analysis procedures to work with these heterogeneous …

Aims. We present photometric properties and distance measurements of 252high redshift
Type Ia supernovae (0.15< z< 1.1) discovered during the first three years of the Supernova …

Aims. We present an empirical model of type Ia supernovae spectro-photometric evolution
with time. Methods. The model is built using a large data set including light-curves and …

SN 2011fe was the nearest and best-observed type Ia supernova in a generation, and
brought previous incomplete datasets into sharp contrast with the detailed new data. In …

Literature data are collated for 38 stripped-envelope core-collapse supernovae (SE SNe; ie
SNe IIb, Ib, Ic and Ic-BL) that have good light-curve coverage in more than one optical band …

JCW had long wanted to write a new monograph on supernovae. Despite an immense
explosion in the literature and many review articles, there had not been one since that of …

We present an updated version of the multicolor light-curve shape method to measure
distances to Type Ia supernovae (SNe Ia), incorporating new procedures for K-correction …

The most precise local measurements of H 0 rely on observations of Type Ia supernovae
(SNe Ia) coupled with Cepheid distances to SN Ia host galaxies. Recent results have shown …