activity
19972026
most citedA very energetic supernova associated with the gamma-ray burst of 29 March 2003

1.5k citations · 15.4k across the 209 of their papers we have counts for

collaborators

210 papers

astro-ph.CO2026

Follow-up of SN 2025wny IV: Photometric Time-delay Measurements of a Strongly Lensed Superluminous Supernova

Alice Townsend, Suhail Dhawan, Erin E. Hayes +34

We present photometric time-delay measurements of SN 2025wny, the first strongly lensed Type I superluminous supernova (SLSN-I), discovered at . Time-delay measurements…

astro-ph.CO2026

Follow-up of SN 2025wny II: Superluminous Supernova Physics at Cosmic Noon

Maggie L. Li, Lin Yan, Anamaria Gkini +46

SN 2025wny is a gravitationally lensed, hydrogen-poor superluminous supernova (SLSN-I) at z = 2.015. To date, it is the most extensively observed high-redshift core-collapse SN and…

astro-ph.HE2024★ 12 cited

GRB 201015A: from seconds to months of optical monitoring and supernova discovery

S. Belkin, A. S. Pozanenko, P. Y. Minaev +21

We present full photometric coverage and spectroscopic data for soft GRB 201015A with a redshift z = 0.426. Our data spans a time range of 85 days following the detection of GRB. T…

astro-ph.HE2023★ 4 cited

A nebular origin for the persistent radio emission of fast radio bursts

Gabriele Bruni, Luigi Piro, Yuan-Pei Yang +12

Fast radio bursts (FRBs) are millisecond-duration, bright (Jy) extragalactic bursts, whose production mechanism is still unclear. Recently, two repeating FRBs were found to h…

astro-ph.GA2023

Comparing emission- and absorption-based gas-phase metallicities in GRB host galaxies at using JWST

P. Schady, R. M. Yates, L. Christensen +34

Much of what is known of the chemical composition of the universe is based on emission line spectra from star forming galaxies. Emission-based inferences are, nevertheless, model-d…

astro-ph.GA2023★ 23 cited

The cosmic build-up of dust and metals. Accurate abundances from GRB-selected star-forming galaxies at

K. E. Heintz, A. De Cia, C. C. Thöne +38

The chemical enrichment of dust and metals in the interstellar medium (ISM) of galaxies throughout cosmic time is one of the key driving processes of galaxy evolution. Here we stud…