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From the 1 of 10 linked papers with an AI index.

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20242026
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10 papers

astro-ph.CO2026

Radio Recombination Line Contamination in Post-Reionization 21 cm Intensity Mapping

Pip Petersen, Yakov Faerman, Matthew McQuinn

The paper evaluates how radio recombination lines (RRLs) could contaminate post‑reionization 21 cm intensity‑mapping measurements, develops a formalism to predict their impact on t…

astro-ph.IM2026

Revealing Cosmic Ecosystems with the Hubble Space Telescope in 2030s and Beyond

Sanchayeeta Borthakur, Tanmay Singh, David French +22

Ultraviolet spectroscopy with the Hubble Space Telescope (HST) provides the most direct and sensitive probe of the disk-circumgalactic medium (CGM) interface at radii of 20 kpc, wh…

astro-ph.GA2026

High-S/N Quasar Observations with HST/COS: Deep Fields for Spectroscopy

Andrew J. Fox, Jerry Kriss, Philipp Richter +49

Hubble is still in prime observing condition for making transformative discoveries in UV astronomy. In this white paper we describe the science case for a deep (S/N>30) UV spectros…

astro-ph.GA2026

Accretion-Driven Turbulence in the Circumgalactic Medium

Roy Goldner, Jonathan Stern, Drummond Fielding +3

Simulations suggest that turbulence is ubiquitous in the circumgalactic medium (CGM), though the source and properties of CGM turbulence is uncertain. Using analytic considerations…

astro-ph.GA2026

Modeling Emission-Line Surface Brightness in a Multiphase Galactic Wind: An O VI Case Study

Zirui Chen, Zixuan Peng, Kate H. R. Rubin +6

We present a fast and robust analytic framework for predicting surface brightness (SB) of emission lines in galactic winds as a function of radius up to kpc out in the c…

astro-ph.GA2025

Marvelous Metals: Surveying the Circumgalactic Medium of Simulated Dwarf Galaxies

Daniel R. Piacitelli, Alyson M. Brooks, Charlotte Christensen +7

Dwarf galaxies are uniquely sensitive to energetic feedback processes and are known to experience substantial mass and metal loss from their disk. Here, we investigate the circumga…