most citedResolving the Unresolved Galactic Winds in Multi-phase Models. I. Methodology and Application

1 citations · 1 across the 8 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026

The LBT Y Project VI: Gas-Phase Chemical Abundance Patterns of Metal-Poor Nebulae

Noah S. J. Rogers, Evan D. Skillman, Richard W. Pogge +7

Through a combined rest-optical and NIR observing campaign, the Large Binocular Telescope Primordial He Abundance () Project has delivered a precision measurement of $Y_…

astro-ph.HE2026

Not So Heavy Metal I: Low Metallicity Enhances the Rate of high-redshift Superluminous Supernovae

Ben Margalit, Allison L. Strom, Cristina Andrade +4

Type-I superluminous supernovae (SLSNe) are extremely luminous stellar explosions originating from the core collapse of massive stars. Unlike normal core-collapse supernovae, howev…

astro-ph.GA2026

The Low-Mass Baryon Cycle in QUEST Dwarf Galaxies I: Sample definition and first results

Ava Polzin, Hsiao-Wen Chen, Zhijie Qu +3

We introduce the QUEST Dwarfs program, which connects low-mass galaxies' stellar populations, interstellar medium, and circumgalactic medium in a large and coherently analyzed samp…

astro-ph.GA2026★ 1 cited

Resolving the Unresolved Galactic Winds in Multi-phase Models. I. Methodology and Application

Xinfeng Xu, Drummond Fielding, Timothy Heckman +12

Galactic winds shape galaxy evolution; however, the outflowing gas is complex: it consists of multiple ionization phases, and its properties vary spatially. Therefore, methods that…

astro-ph.GA2026

The LBT Project II: MODS Spectra, Physical Conditions, and Oxygen Abundances in Local Metal-Poor Nebulae

Noah S. J. Rogers, Evan D. Skillman, Richard W. Pogge +7

Empirically measuring the primordial He mass fraction, , requires a significant number of low-metallicity nebulae with direct constraints on He/H and O/H abundances. Thi…

astro-ph.IM2025

Resolving the Origins and Pathways of Ionizing Radiation Escape with UV Integral Field Spectroscopy

Cody Carr, Renyue Cen, Brian Fleming +4

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.GA2025

CLASSY XIII. Cutting through the Clouds - Comparing Indirect Tracers of Ionizing Photon Escape

Kaelee S. Parker, Danielle A. Berg, John Chisholm +25

The Epoch of Reionization (EoR) provides critical insights into the role of early galaxies in shaping the ionization state of the universe. However, because of the opacity of the i…

astro-ph.GA2025

Spatially Resolving the Fundamental Elements of Reionization in Galaxies

Xinfeng Xu, Stephan McCandliss, Allison Strom +10

Cosmic reionization marks a critical epoch when the first galaxies ionized the intergalactic medium through the escape of Lyman continuum (LyC) radiation. Young, massive star clust…

astro-ph.IM2025

Evolution of the Ionizing Photon Luminosity Function

Stephan R. McCandliss, Swara Ravindranath, Sangeeta Malhotra +6

Counting the number and brightness of ionizing radiation sources out to a redshift of z ~ 1.2 will revolutionize our understanding of how the ionizing background is created and sus…

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…