activity
20132026
most citedMassive Warm/Hot Galaxy Coronae as Probed by UV/X-ray Oxygen Absorption and Emission: I - Basic Model

149 citations · 375 across the 26 of their papers we have counts for

collaborators

28 papers

astro-ph.GA2026

Highly Ionized Oxygen in the Circumgalactic Medium of TNG100 Galaxies: Distributions, Thermal States, and Ionization Mechanisms

Yossi Oren, Amiel Sternberg, Christopher F. McKee +1

We investigate the origin of the highly ionized oxygen species, O VI, O VII, and O VIII, in the circumgalactic medium (CGM) of galaxies at redshifts , by post-processi…

astro-ph.GA2026

The Halo Gas of Local Spiral Galaxies and the Link to Gaseous Satellites

Yong Zheng, Jingyao Zhu, Ben Wertz +2

Gaseous satellites orbiting massive host galaxies experience gas stripping and may contribute additional gas to the hosts' circumgalactic medium (CGM). We identify a sample of 21 l…

astro-ph.CO2026

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

Pip Petersen, Yakov Faerman, Matthew McQuinn

We explore radio recombination line (RRL) contamination in post-reionization 21 cm intensity mapping observations. We develop a formalism to estimate the contamination of the 21 cm…

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.GA2025★ 3 cited

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.GA2025

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

Mapping Galactic Winds and Small-scale Structure in the Circumgalactic Medium with Habitable Worlds Observatory

Joseph N. Burchett, Deborah M. Lokhorst, Yakov Faerman +4

We present a science case for the Habitable Worlds Observatory (HWO) to map the circumgalactic medium (CGM) in emission by targeting ultraviolet emission lines, which trace the 10^…

astro-ph.GA2025★ 4 cited

Introducing the Descriptive Parametric Model: Gaseous Profiles for Galaxies, Groups, and Clusters

Benjamin D. Oppenheimer, G. Mark Voit, Yannick M. Bahé +14

We develop and present the Descriptive Parametric Model (DPM), a tool for generating profiles of gaseous halos (pressure, electron density, and metallicity) as functions of radius,…

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…

astro-ph.GA2025★ 5 cited

Upper Limits on the Mass of Cool Gas in the Circumgalactic Medium of Dwarf Galaxies

Yakov Faerman, Yong Zheng, Benjamin D. Oppenheimer

We use HI absorption measurements to constrain the amount of cool ( K), photoionized gas in the circumgalactic medium (CGM) of dwarf galaxies with $M_* = 10^{6.5-9.5}…

astro-ph.GA2024

The CIViL* Survey: The Discovery of a C IV Dichotomy in the CGM of L* Galaxies

Samantha L. Garza, Jessica K. Werk, Trystyn A. M. Berg +4

This paper investigates C IV absorption in the circumgalactic medium (CGM) of L* galaxies and its relationship with galaxy star formation rates. We present new observations from th…

astro-ph.SR2024

The Statistics and Environments of Hostless Supernovae

Yu-Jing Qin, Ann Zabludoff, Iair Arcavi +3

Transient surveys routinely detect supernovae (SNe) without obvious host galaxies. To understand the demographics of these "hostless" SNe and to constrain the possible host propert…

astro-ph.GA2024

Comparison of Models for the Warm-Hot Circumgalactic Medium around Milky Way-like Galaxies

Priyanka Singh, Erwin T. Lau, Yakov Faerman +2

A systematic comparison of the models of the circumgalactic medium (CGM) and their observables is crucial to understanding the predictive power of the models and constraining physi…

astro-ph.GA2024★ 1 cited

The signatures of density fluctuations and mixing gas in circumgalactic absorption systems

Yakov Faerman, Daniel R. Piacitelli, Matthew McQuinn +1

We investigate the prospects for detecting and constraining density and temperature inhomogeneities in the circumgalactic medium (CGM) using absorption measurements of metal ions.…

astro-ph.GA2024★ 4 cited

The COS-Holes Survey: Connecting Galaxy Black Hole Mass with the State of the CGM

Samantha L. Garza, Jessica K. Werk, Benjamin D. Oppenheimer +9

We present an analysis of \textit{HST}/COS/G160M observations of CIV in the inner circumgalactic medium (CGM) of a novel sample of eight z0, LL galaxies, p…

astro-ph.GA2024★ 3 cited

Sunyaev-Zeldovich Signals from Galaxies: Observations, Analytics, and Simulations

Yossi Oren, Amiel Sternberg, Christopher F. McKee +2

We analyze measurements of the thermal Sunyaev-Zeldovich (tSZ) effect arising in the circumgalactic medium (CGM) of galaxies, reported by Bregman et al. 2022 and Das et al. 2…

astro-ph.GA2024★ 7 cited

Braving the Storm: Quantifying Disk-wide Ionized Outflows in the Large Magellanic Cloud with ULLYSES

Yong Zheng, Kirill Tchernyshyov, Knut Olsen +11

The Large Magellanic Cloud (LMC) is home to many HII regions, which may lead to significant outflows. We examine the LMC's multiphase gas ( K) in HI, SII, SiIV, and…

astro-ph.GA2023

The Halo21 Absorption Modeling Challenge: Lessons From "Observing" Synthetic Circumgalactic Absorption Spectra

Zachary Hafen, Sameer, Cameron Hummels +7

In the Halo21 absorption modeling challenge we generated synthetic absorption spectra of the circumgalactic medium (CGM), and attempted to estimate the metallicity, temperature, an…

astro-ph.GA2023★ 2 cited

The cool circumgalactic medium of low-redshift star-forming galaxies: I -- Empirical model and mean properties

Yakov Faerman, Jessica K. Werk

We present an analytic model for the cool, K, circumgalactic medium (CGM), describing the gas distribution, thermal and ionization state. Our model assumes (total)…

astro-ph.GA2023

A Comprehensive Investigation of Metals in the Circumgalactic Medium of Nearby Dwarf Galaxies

Yong Zheng, Yakov Faerman, Benjamin D. Oppenheimer +7

Dwarf galaxies are found to have lost most of their metals via feedback processes; however, there still lacks consistent assessment on the retention rate of metals in their circumg…

astro-ph.GA2022★ 9 cited

Absorption-based Circumgalactic Medium Line Emission Estimates

Daniel R. Piacitelli, Erik Solhaug, Yakov Faerman +1

Motivated by integral field units (IFUs) on large ground telescopes and proposals for ultraviolet-sensitive space telescopes to probe circumgalactic medium (CGM) emission, we surve…

astro-ph.GA2021★ 23 cited

Exploring the Milky Way Circumgalactic Medium in a Cosmological Context with a Semi-Analytic Model

Yakov Faerman, Viraj Pandya, Rachel S. Somerville +1

We combine the Santa-Cruz Semi-Analytic Model (SAM) for galaxy formation and evolution with the circumgalactic medium (CGM) model presented in Faerman et al. (2020) to explore the…

astro-ph.GA2019★ 71 cited

Massive Warm/Hot Galaxy Coronae: II. Isentropic Model

Yakov Faerman, Amiel Sternberg, Christopher F. McKee

We construct a new analytic phenomenological model for the extended circumgalactic material (CGM) of galaxies. Our model reproduces the OVII/OVIII absorption observations of…