most citedThe Lyman-alpha and Continuum Origins Survey. I. Survey description and Ly imaging

7 citations · 20 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

Specific Star Formation Rate Enhancement across the Galaxy Merger Sequence: Insights from Citizen Science Classifications

Jacob Lee, Alexandra Le Reste, Claudia Scarlata +1

We present an analysis of specific star formation rates (sSFR) across the galaxy merger sequence using visual classifications from the Zooniverse citizen science project "Cosmic Di…

astro-ph.GA2025★ 4 cited

The Ly and Continuum Origins Survey. III. Investigating the Link between Galaxy Morphology, Merger Properties and LyC Escape

Alexandra Le Reste, Anne E. Jaskot, Jordanne Brazie +20

Characterizing the mechanisms and galaxy properties conducive to the emission and escape of ionizing (LyC) emission is necessary to accurately model the Epoch of Reionization, and…

astro-ph.GA2025★ 6 cited

The Lyman-alpha and Continuum Origins Survey II: the connection between the escape of ionizing radiation and Lyman-alpha halos in star-forming galaxies

A. Saldana-Lopez, M. J. Hayes, A. Le Reste +24

One of the current challenges in galaxy evolution studies is to establish the mechanisms that govern the escape of ionizing radiation from galaxies. Here, we investigate the connec…

astro-ph.GA2025★ 7 cited

The Lyman-alpha and Continuum Origins Survey. I. Survey description and Ly imaging

Alexandra Le Reste, Claudia Scarlata, Matthew Hayes +25

Understanding the mechanisms driving the escape of ionizing or Lyman continuum (LyC) emission from the interstellar medium of galaxies is necessary to constrain the evolution of re…

astro-ph.GA2025★ 3 cited

Forming the local starburst galaxy Haro 11 through hydrodynamical merger simulations

Timmy Ejdetjärn, Oscar Agertz, Florent Renaud +3

Haro 11 is a metal-poor, starburst galaxy believed to be the result of an ongoing merger, which is shaping the properties of the galaxy. In this study, we carry out a large suite o…