activity
20112022
most citedFirst Identification of 10-kpc Scale [CII] 158um Halos around Star-Forming Galaxies at z=5-7

144 citations · 1.7k across the 34 of their papers we have counts for

collaborators
Showing 2020Show all

9 papers · 1 filter

astro-ph.CO2020★ 7 cited

A Novel Estimator for the Equation of State of the IGM by Ly Forest Tomography

Hendrik Müller, Christoph Behrens, David James Edward Marsh

We present a novel procedure to estimate the Equation of State of the intergalactic medium in the quasi-linear regime of structure formation based on Ly forest tomography and ap…

astro-ph.GA2020★ 60 cited

Velocity dispersion in the interstellar medium of early galaxies

M. Kohandel, A. Pallottini, A. Ferrara +5

We study the structure of spatially resolved, line-of-sight velocity dispersion for galaxies in the Epoch of Reionization (EoR) traced by [CII] line emission. Our labo…

astro-ph.GA2020★ 19 cited

Early galaxy growth: mergers or gravitational instability?

A. Zanella, A. Pallottini, A. Ferrara +4

We investigate the spatially-resolved morphology of galaxies in the early Universe. We consider a typical redshift z = 6 Lyman Break galaxy, "Althaea" from the SERRA hydrodynamical…

astro-ph.GA2020★ 66 cited

The physical origins and dominant emission mechanisms of Lyman-alpha halos: results from the TNG50 simulation in comparison to MUSE observations

Chris Byrohl, Dylan Nelson, Christoph Behrens +6

Extended Lyman-alpha emission is now commonly detected around high redshift galaxies through stacking and even on individual basis. Despite recent observational advances, the physi…

astro-ph.CO2020★ 91 cited

AxioNyx: Simulating Mixed Fuzzy and Cold Dark Matter

Bodo Schwabe, Mateja Gosenca, Christoph Behrens +2

The distinctive effects of fuzzy dark matter are most visible at non-linear galactic scales. We present the first simulations of mixed fuzzy and cold dark matter, obtained with an…

astro-ph.CO2020★ 4 cited

An Optimized Ly Forest Inversion Tool Based on a Quantitative Comparison of Existing Reconstruction Methods

Hendrik Müller, Christoph Behrens, David James Edward Marsh

We present a same-level comparison of the most prominent inversion methods for the reconstruction of the matter density field in the quasi-linear regime from the Ly forest flux.…

astro-ph.CO2020★ 36 cited

Axion Miniclusters Made Easy

David Ellis, David J. E. Marsh, Christoph Behrens

We use a modified version of the Peak Patch excursion set formalism to compute the mass and size distribution of QCD axion miniclusters from a fully non-Gaussian initial density fi…

physics.atom-ph2020★ 40 cited

Clocking Auger Electrons

D. C. Haynes, M. Wurzer, A. Schletter +34

Intense X-ray free-electron lasers (XFELs) can rapidly excite matter, leaving it in inherently unstable states that decay on femtosecond timescales. As the relaxation occurs primar…

astro-ph.GA2020★ 16 cited

A random-walk model for dark matter halo spins

Andrew Benson, Christoph Behrens, Yu Lu

We extend the random-walk model of Vitvitska et al. for predicting the spins of dark matter halos from their merger histories. Using updated merger rates, orbital parameter distrib…