activity
20082026
most citedCMB-S4 Science Case, Reference Design, and Project Plan

443 citations · 4.9k across the 139 of their papers we have counts for

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Showing 2022Show all

15 papers · 1 filter

astro-ph.SR2022

Hyperion: The origin of the stars A far-UV space telescope for high-resolution spectroscopy over wide fields

Erika Hamden, David Schiminovich, Shouleh Nikzad +30

We present Hyperion, a mission concept recently proposed to the December 2021 NASA Medium Explorer announcement of opportunity. Hyperion explores the formation and destruction of m…

astro-ph.GA2022★ 16 cited

CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A

Hideaki Takemura, Fumitaka Nakamura, Héctor G. Arce +15

The mass distribution of dense cores is a potential key to understand the process of star formation. Applying dendrogram analysis to the CARMA-NRO Orion CO (=1--0) data,…

astro-ph.CO2022★ 7 cited

X-ray Absorption Lines in the Warm-Hot Intergalactic Medium: Probing Chandra observations with the CAMEL simulations

Amanda Butler Contreras, Erwin T. Lau, Benjamin D. Oppenheimer +5

Known as the "Missing Baryon Problem", about one-third of baryons in the local universe remain unaccounted for. The missing baryons are thought to reside in the warm-hot intergalac…

astro-ph.GA2022★ 37 cited

Active galactic nucleus jet feedback in hydrostatic halos

Rainer Weinberger, Kung-Yi Su, Kristian Ehlert +8

Feedback driven by jets from active galactic nuclei is believed to be responsible for reducing cooling flows in cool-core galaxy clusters. We use simulations to model feedback from…

astro-ph.GA2022★ 9 cited

The Supersonic Project: The eccentricity and rotational support of SIGOs and DM GHOSts

Claire E. Williams, Smadar Naoz, William Lake +7

A supersonic relative velocity between dark matter (DM) and baryons (the stream velocity) at the time of recombination induces the formation of low mass objects with anomalous prop…

astro-ph.GA2022★ 21 cited

Efficient long-range AGN feedback affects the low redshift Lyman- forest

Megan Taylor Tillman, Blakesley Burkhart, Stephanie Tonnesen +5

Active galactic nuclei (AGN) feedback models are generally calibrated to reproduce galaxy observables such as the stellar mass function and the bimodality in galaxy colors. We use…

astro-ph.GA2022★ 25 cited

Spiral Arms are Metal Freeways: Azimuthal Gas-Phase Metallicity Variations in Simulated Cosmological Zoom-in Flocculent Disks

Matthew E. Orr, Blakesley Burkhart, Andrew Wetzel +7

We examine the azimuthal variations in gas-phase metallicity profiles in simulated Milky Way mass disk galaxies from the Feedback in Realistic Environments (FIRE-2) cosmological zo…

astro-ph.GA2022★ 37 cited

Code Comparison in Galaxy Scale Simulations with Resolved Supernova Feedback: Lagrangian vs. Eulerian Methods

Chia-Yu Hu, Matthew C. Smith, Romain Teyssier +8

We present a suite of high-resolution simulations of an isolated dwarf galaxy using four different hydrodynamical codes: {\sc Gizmo}, {\sc Arepo}, {\sc Gadget}, and {\sc Ramses}. A…

astro-ph.GA2022★ 9 cited

The Supersonic Project: The Early Evolutionary Path of SIGOs

William Lake, Smadar Naoz, Blakesley Burkhart +7

Supersonically Induced Gas Objects (SIGOs) are a class of early Universe objects that have gained attention as a potential formation route for globular clusters. SIGOs have only re…

astro-ph.GA2022★ 2 cited

On the impact of runaway stars on dwarf galaxies with resolved interstellar medium

Ulrich P. Steinwandel, Greg L. Bryan, Rachel S. Somerville +2

About ten to 20 percent of massive stars may be kicked out of their natal clusters before exploding as supernovae. These "runaway stars" might play a crucial role in driving galact…

astro-ph.GA2022★ 13 cited

Spatially Resolved Gas-phase Metallicity in FIRE-2 Dwarfs: Late-Time Evolution of Metallicity Relations in Simulations with Feedback and Mergers

Lori E. Porter, Matthew E. Orr, Blakesley Burkhart +4

We present an analysis of spatially resolved gas-phase metallicity relations in five dwarf galaxies (, …

astro-ph.GA2022★ 29 cited

Gas Accretion Can Drive Turbulence in Galaxies

John C. Forbes, Razieh Emami, Rachel S. Somerville +11

The driving of turbulence in galaxies is deeply connected with the physics of feedback, star formation, outflows, accretion, and radial transport in disks. The velocity dispersion…

astro-ph.GA2022★ 19 cited

The low redshift Lyman- Forest as a constraint for models of AGN feedback

Blakesley Burkhart, Megan Tillman, Alexander B. Gurvich +5

We study the sensitivity of the Lyman- Forest observables, such as the column density distribution function (CDD), flux PDF, flux power spectrum, and line width distribu…

astro-ph.GA2022★ 4 cited

Studying Interstellar Turbulence Driving Scales using the Bispectrum

Michael J. O'Brien, Blakesley Burkhart, Michael J. Shelley

We demonstrate the utility of the bispectrum, the Fourier three-point correlation function, for studying driving scales of magnetohydrodynamic (MHD) turbulence in the interstellar…

astro-ph.CO2022★ 67 cited

The CAMELS project: public data release

Francisco Villaescusa-Navarro, Shy Genel, Daniel Anglés-Alcázar +44

The Cosmology and Astrophysics with MachinE Learning Simulations (CAMELS) project was developed to combine cosmology with astrophysics through thousands of cosmological hydrodynami…