activity
20172021
most citedDelay Time Distributions of Type Ia Supernovae From Galaxy and Cosmic Star Formation Histories

39 citations · 121 across the 9 of their papers we have counts for

collaborators

20 papers

astro-ph.GA2021

Rates and delay times of type Ia supernovae in the Dark Energy Survey

P. Wiseman, M. Sullivan, M. Smith +87

We use a sample of 809 photometrically classified type Ia supernovae (SNe Ia) discovered by the Dark Energy Survey (DES) along with 40415 field galaxies to calculate the rate of SN…

astro-ph.CO2020

The Dark Energy Survey Supernova Program: Modelling selection efficiency and observed core collapse supernova contamination

M. Vincenzi, M. Sullivan, O. Graur +79

The analysis of current and future cosmological surveys of type Ia supernovae (SNe Ia) at high-redshift depends on the accurate photometric classification of the SN events detected…

astro-ph.HE2020

The Host Galaxies of Tidal Disruption Events

K. Decker French, Thomas Wevers, Jamie Law-Smith +2

Recent studies of Tidal Disruption Events (TDEs) have revealed unexpected correlations between the TDE rate and the large-scale properties of the host galaxies. In this review, we…

astro-ph.GA202039 cited

Delay Time Distributions of Type Ia Supernovae From Galaxy and Cosmic Star Formation Histories

Louis-Gregory Strolger, Steven A. Rodney, Camilla Pacifici +2

We present analytical reconstructions of type Ia supernova (SN Ia) delay time distributions (DTDs) by way of two independent methods: by a Markov chain Monte Carlo best-fit techniq…

astro-ph.GA2020

The BUFFALO HST Survey

Charles L. Steinhardt, Mathilde Jauzac, Ana Acebron +91

The Beyond Ultra-deep Frontier Fields and Legacy Observations (BUFFALO) is a 101 orbit + 101 parallel Cycle 25 Hubble Space Telescope Treasury program taking data from 2018-2020. B…

astro-ph.HE201920 cited

A year-long plateau in the late-time near-infrared light curves of Type Ia supernovae

Or Graur, Kate Maguire, Russell Ryan +6

The light curves of Type Ia supernovae are routinely used to constrain cosmology models. Driven by radioactive decay of 56Ni, the light curves steadily decline over time, but >150…