129 citations · 369 across the 9 of their papers we have counts for
6 papers · 1 filter
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…
On the evolution of the size of Lyman alpha halos across cosmic time: no change in the circumgalactic gas distribution when probed by line emission
Axel Runnholm, Matthew J. Hayes, Yu-Heng Lin +18
Lyman (Ly) is now routinely used as a tool for studying high-redshift galaxies and its resonant nature means it can trace neutral hydrogen around star-forming galaxies. Inte…
The Low-Redshift Lyman Continuum Survey: Optically Thin and Thick Mg II Lines as Probes of Lyman Continuum Escape
Xinfeng Xu, Alaina Henry, Timothy Heckman +14
The Mg II 2796, 2803 doublet has been suggested to be a useful indirect indicator for the escape of Ly-alpha and Lyman continuum (LyC) photons in local star-forming galaxies. Howev…
A First Look at the Abundance Pattern -- O/H, C/O, and Ne/O -- in Galaxies with JWST/NIRSpec
Karla Z. Arellano-Córdova, Danielle A. Berg, John Chisholm +9
We analyze the rest-frame near-UV and optical nebular spectra of three galaxies from the Early Release Observations taken with the Near-Infrared Spectrograph (NIRSpec) on t…
Understanding the spatial variation of \ion{Mg}{II} and ionizing photon escape in a local LyC leaker
Thomas Seive, John Chisholm, Floriane Leclercq +1
Ionizing photons must have escaped from high-redshift galaxies, but the neutral high-redshift intergalactic medium makes it unlikely to directly detect these photons during the Epo…
The MUSE Hubble Ultra Deep Field Survey. XV. The mean rest-UV spectra of Ly-alpha emitters at z>3
Anna Feltre, Michael V. Maseda, Roland Bacon +22
We investigate the ultraviolet (UV) spectral properties of faint Lyman- emitters (LAEs) in the redshift range 2.9<z<4.6 and provide material to prepare future observations of th…