activity
19942022
most citedThe binary progenitor of Tycho Brahe's 1572 supernova

277 citations · 2.9k across the 56 of their papers we have counts for

collaborators

56 papers

astro-ph.HE2022★ 14 cited

MUSSES2020J: The Earliest Discovery of a Fast Blue Ultraluminous Transient at Redshift 1.063

Ji-an Jiang, Naoki Yasuda, Keiichi Maeda +22

In this Letter, we report the discovery of an ultraluminous fast-evolving transient in rest-frame UV wavelengths, MUSSES2020J, soon after its occurrence by using the Hyper Suprime-…

astro-ph.SR2022★ 8 cited

A possible surviving companion of the SN Ia in the Galactic SNR G272.2-3.2

Pilar Ruiz-Lapuente, Jonay I. González Hernández, Régis Cartier +4

We use the {\it Gaia} EDR3 to explore the Galactic supernova remnant SNR G272.2-3.2, produced by the explosion of a Type Ia supernova (SNIa), about 7,500 years ago, to search for a…

astro-ph.CO2021★ 89 cited

The growth of density perturbations in the last 10 billion years from tomographic large-scale structure data

Carlos García-García, Jaime Ruiz Zapatero, David Alonso +5

In order to investigate the origin of the ongoing tension between the amplitude of matter fluctuations measured by weak lensing experiments at low redshifts and the value inferred…

astro-ph.CO2021★ 16 cited

The HST See Change Program: I. Survey Design, Pipeline, and Supernova Discoveries

Brian Hayden, David Rubin, Kyle Boone +53

The See Change survey was designed to make cosmological measurements by efficiently discovering high-redshift Type Ia supernovae (SNe Ia) and improving cluster mass measureme…

astro-ph.GA2020★ 8 cited

See Change: VLT spectroscopy of a sample of high-redshift Type Ia supernova host galaxies

S. C. Williams, I. M. Hook, B. Hayden +9

The Supernova Cosmology Project has conducted the `See Change' programme, aimed at discovering and observing high-redshift (1.13 z 1.75) Type Ia supernovae (SNe Ia).…

astro-ph.HE2019★ 8 cited

Gamma-rays from kilonovae and the cosmic gamma-ray background

Pilar Ruiz-Lapuente, Oleg Korobkin

The recent detection of the gravitational wave event GW170817, produced by the coalescence of two neutron stars, and of its optical-infrared counterpart, powered by the radioactive…