We present a detailed report of the connection between long‐duration gamma‐ray bursts
(GRBs) and their accompanying supernovae (SNe). The discussion presented here places …

Gamma-ray bursts (GRBs) are divided into two populations,; long GRBs that derive from the
core collapse of massive stars (for example, ref.) and short GRBs that form in the merger of …

We review our current understanding of the progenitors of both long and short duration
gamma-ray bursts (GRBs). Constraints can be derived from multiple directions, and we use …

Abstract We present the Open Supernova Catalog, an online collection of observations and
metadata for presently 36,000+ supernovae and related candidates. The catalog is freely …

A new class of ultra-long-duration (more than 10,000 seconds) γ-ray bursts has recently
been suggested,,. They may originate in the explosion of stars with much larger radii than …

We present the most extensive sample of 45 type I (short) and 275 type II (long) gamma-ray
bursts (GRBs) with known redshift to investigate the correlation between the rest-frame peak …

The optical and optical/near-infrared pseudo-bolometric light curves of 85 stripped-envelope
supernovae (SNe) are constructed using a consistent method and a standard cosmology …

We study 34 Type Ic supernovae that have broad spectral features (SNe Ic-BL). This is the
only SN type found in association with long-duration gamma-ray bursts (GRBs). We …

We present a model of the short gamma-ray burst (SGRB) population under a 'quasi-
universal jet'scenario in which jets can differ somewhat in their on-axis peak prompt …

Gamma-ray Burst (GRB) collimation has been inferred with the observations of achromatic
steepening in GRB light curves, known as jet breaks. Identifying a jet break from a GRB …