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 …

Observationally, kilonovae are astrophysical transients powered by the radioactive decay of
nuclei heavier than iron, thought to be synthesized in the merger of two compact objects …

Abstract The SUperluminous Supernova Host galaxIES survey aims to provide strong new
constraints on the progenitors of superluminous supernovae (SLSNe) by understanding the …

We present data and initial results from VLT/X-Shooter emission-line spectroscopy of 96
galaxies selected by long γ-ray bursts (GRBs) at 0.1< z< 3.6, the largest sample of GRB host …

We present rest-frame near-IR (NIR) luminosities and stellar masses for a large and
uniformly selected population of gamma-ray burst (GRB) host galaxies using deep Spitzer …

The contemporary discoveries of galaxies and gamma ray bursts (GRBs) at high redshift
have supplied the first direct information on star formation when the universe was only a few …

Superluminous supernovae (SLSNe) are very bright explosions that were only discovered
recently and that show a preference for occurring in faint dwarf galaxies. Understanding why …

We present observations and analysis of the host galaxies of 23 heavily dust-obscured
gamma-ray bursts (GRBs) observed by the Swift satellite during the years 2005–2009 …

We present light curves and spectra of the tidal disruption event (TDE) ASASSN-18pg/AT
2018dyb spanning a period of one year. The event shows a plethora of strong emission …

We present the results of an extensive Hubble Space Telescope imaging study of 105,
mostly Swift, long-duration gamma-ray bursts (LGRBs) spanning $0.03\lesssim z\lesssim …