activity
20222025
most citedThe Far-Ultraviolet Continuum Slope as a Lyman Continuum Escape Estimator at High-redshift

158 citations · 218 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2025

How Do Ionizing Photons Escape from Star-Forming Galaxies?

Cody Carr, Renyue Cen, Sophia Flury +3

The Epoch of Reionization marks the last major phase transition in the early Universe, during which the majority of neutral hydrogen once filling the intergalactic medium was ioniz…

astro-ph.GA20245 cited

A Simulated Galaxy Laboratory: Exploring the Observational Effects on UV Spectral Absorption Line Measurements

R. Michael Jennings, Alaina Henry, Valentin Mauerhofer +13

Ultraviolet absorption line spectroscopy is a sensitive diagnostic for the properties of interstellar and circumgalactic gas. Down-the-barrel observations, where the absorption is…

astro-ph.GA202441 cited

Ubiquitous broad-line emission and the relation between ionized gas outflows and Lyman continuum escape in Green Pea galaxies

R. O. Amorín, M. Rodríguez-Henríquez, V. Fernández +29

We report observational evidence of highly turbulent ionized gas kinematics in a sample of 20 Lyman continuum (LyC) emitters (LCEs) at low redshift (). Detailed Gaussian…

astro-ph.GA2023

Galactic Outflow Emission Line Profiles: Evidence for Dusty, Radiatively-Driven Ionized Winds in Mrk 462

Sophia R. Flury, Edward C. Moran, Miriam Eleazer

Over the past half century, gas outflows and winds have been observed as asymmetric emission lines in a wide range of astrophysical contexts, including galaxies and early-type star…

astro-ph.GA202314 cited

Chemical abundances in Seyfert galaxies X. Sulphur abundance estimates

O. L. Dors, M. Valerdi, R. A. Riffel +12

For the first time, the sulphur abundance relative to hydrogen (S/H) in the Narrow Line Regions of a sample of Seyfert 2 nuclei (Sy 2s) has been derived via direct estimation of th…

astro-ph.GA2022158 cited

The Far-Ultraviolet Continuum Slope as a Lyman Continuum Escape Estimator at High-redshift

J. Chisholm, A. Saldana-Lopez, S. Flury +25

Most of the hydrogen in the intergalactic medium (IGM) was rapidly ionized at high-redshifts. While observations have established that reionization occurred, observational constrai…