activity
20052026
most citedLSST: from Science Drivers to Reference Design and Anticipated Data Products

3.5k citations · 6.2k across the 41 of their papers we have counts for

collaborators

42 papers

astro-ph.IM2026

The Rubin Observatory Target-of-Opportunity System in the First Year of Operations

Sean Patrick MacBride, R. Lynne Jones, Peter Yoachim +41

The NSF/DOE Vera C. Rubin Observatory is a discovery machine, with unprecedented survey speed, which can be used to identify exotic astrophysical transients. In its prime mission,…

astro-ph.IM2026

PSF-like Alpha-Particle Events in LSST Images

Guillem Megias Homar, Craig S. Lage, Pierre-François Léget +6

Rare -particle-induced charge clusters appear in LSST images as compact, PSF-like sources with a median FWHM of and median ellipticity consistent with…

astro-ph.IM2024★ 1 cited

Every Datapoint Counts: Stellar Flares as a Case Study of Atmosphere Aided Studies of Transients in the LSST Era

Riley W. Clarke, James R. A. Davenport, John Gizis +8

Due to their short timescale, stellar flares are a challenging target for the most modern synoptic sky surveys. The upcoming Vera C. Rubin Legacy Survey of Space and Time (LSST), a…

astro-ph.IM2022★ 6 cited

The FHD Polarized Imaging Pipeline: A New Approach to Widefield Interferometric Polarimetry

Ruby Byrne, Miguel F. Morales, Bryna Hazelton +2

We describe a new polarized imaging pipeline implemented in the FHD software package. The pipeline is based on the optimal mapmaking imaging approach and performs horizon-to-horizo…

astro-ph.CO2021★ 26 cited

A Map of Diffuse Radio Emission at 182 MHz to Enhance Epoch of Reionization Observations in the Southern Hemisphere

Ruby Byrne, Miguel F. Morales, Bryna Hazelton +5

We present a broadband map of polarized diffuse emission at 167-198 MHz developed from data from the Murchison Widefield Array (MWA). The map is designed to improve visibility simu…

astro-ph.CO2019★ 98 cited

First Season MWA Phase II EoR Power Spectrum Results at Redshift 7

W. Li, J. C. Pober, N. Barry +44

The compact configuration of Phase II of the Murchison Widefield Array (MWA) consists of both a redundant subarray and pseudo-random baselines, offering unique opportunities to per…