activity
20162023
most citedA gravitational-wave standard siren measurement of the Hubble constant

1.2k citations · 1.7k across the 21 of their papers we have counts for

collaborators

15 papers

astro-ph.IM20235 cited

The Dark Energy Survey Six-Year Calibration Star Catalog

E. S. Rykoff, D. L. Tucker, D. L. Burke +64

This Technical Note presents a catalog of calibrated reference stars that was generated by the Forward Calibration Method (FGCM) pipeline (arXiv:1706.01542) as part of the FGCM pho…

astro-ph.CO202312 cited

The Dark Energy Survey Supernova Program: Corrections on photometry due to wavelength-dependent atmospheric effects

J. Lee, M. Acevedo, M. Sako +64

Wavelength-dependent atmospheric effects impact photometric supernova flux measurements for ground-based observations. We present corrections on supernova flux measurements from th…

astro-ph.SR202310 cited

Ultracool dwarfs candidates based on six years of the Dark Energy Survey data

M. dal Ponte, B. Santiago, A. Carnero Rosell +57

We present a sample of 19,583 ultracool dwarf candidates brighter than z selected from the Dark Energy Survey DR2 coadd data matched to VHS DR6, VIKING DR5 and AllWISE co…

astro-ph.EP2023

Synchronous rotation in the (136199) Eris-Dysnomia system

G. M. Bernstein, B. J. Holler, R. Navarro-Escamilla +47

We combine photometry of Eris from a 6-month campaign on the Palomar 60-inch telescope in 2015, a 1-month Hubble Space Telescope WFC3 campaign in 2018, and Dark Energy Survey data…

astro-ph.GA202211 cited

Lessons Learned from the Two Largest Galaxy Morphological Classification Catalogues built by Convolutional Neural Networks

Ting-Yun Cheng, H. Domínguez Sánchez, J. Vega-Ferrero +54

We compare the two largest galaxy morphology catalogues, which separate early and late type galaxies at intermediate redshift. The two catalogues were built by applying supervised…

astro-ph.GA202241 cited

A galaxy-driven model of type Ia supernova luminosity variations

P. Wiseman, M. Vincenzi, M. Sullivan +59

Type Ia supernovae (SNe Ia) are used as standardisable candles to measure cosmological distances, but differences remain in their corrected luminosities which display a magnitude s…