activity
20162026
most citedStrong bound on canonical ultra-light axion dark matter from the Lyman-alpha forest

317 citations · 1k across the 31 of their papers we have counts for

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24 papers · 1 filter

astro-ph.CO2026

Dark Matter Constraints from Small-Scale Cosmic Structure

Ethan O. Nadler, Keir K. Rogers, Alex Drlica-Wagner

Small-scale cosmic structure provides a powerful test of the fundamental nature of dark matter (DM). A wide range of DM models impact matter clustering on small scales, including w…

astro-ph.CO2026

Strongest constraints on dark acoustic oscillations from the Lyman-alpha forest

Zhihan Yuan, Caleb Gemmell, Keir K. Rogers +4

We set the first constraints on a small-scale dark acoustic oscillation (DAO) in the linear matter power spectrum arising from dark sector interactions, with a full forward model o…

astro-ph.CO2026

The Atacama Cosmology Telescope: Probing new signatures of ultralight axions with gravitational lensing

Alex Laguë, Keir K. Rogers, Mathew S. Madhavacheril +14

Ultralight axions (ULAs) are well-motivated dark matter particle candidates that arise in many extensions of the Standard Model of particle physics. ULAs with mass $m_\mathrm{a} \l…

astro-ph.CO2025★ 6 cited

Prospects for disentangling dark matter with weak lensing

Calvin Preston, Keir K. Rogers, Alexandra Amon +1

We investigate the degeneracy between the effects of ultra-light axion dark matter and baryonic feedback in suppressing the matter power spectrum. We forecast that galaxy shear dat…

astro-ph.CO2024★ 3 cited

Interference in Fuzzy Dark Matter Filaments: Idealised Models and Statistics

Tim Zimmermann, David J. E. Marsh, Keir K. Rogers +2

Fuzzy (wave) dark matter (FDM), the dynamical model underlying an ultralight bosonic dark matter species, produces a rich set of non-gravitational signatures that distinguishes it…

astro-ph.CO2024★ 2 cited

High-redshift, small-scale tests of ultralight axion dark matter using Hubble and Webb galaxy UV luminosities

Harrison Winch, Keir K. Rogers, Renée Hložek +1

We calculate the abundance of UV-bright galaxies in the presence of ultralight axion (ULA) dark matter (DM), finding that axions suppress their formation with a non-trivial depende…

astro-ph.CO2023

Extreme Axions Unveiled: a Novel Fluid Approach for Cosmological Modeling

Harrison Winch, Renee Hlozek, David J. E. Marsh +2

Axion-like particles (ALPs) are a well-motivated dark matter candidate that solve some of the problems in the clustering of large scale structure in cosmology. ALPs are often descr…

astro-ph.CO2023★ 2 cited

Cosmological simulations of mixed ultralight dark matter

Alex Laguë, Bodo Schwabe, Renée Hložek +2

The era of precision cosmology allows us to test the composition of the dark matter. Mixed ultralight or fuzzy dark matter (FDM) is a cosmological model with dark matter composed o…

astro-ph.CO2023★ 82 cited

Ultra-light axions and the tension: joint constraints from the cosmic microwave background and galaxy clustering

Keir K. Rogers, Renée Hložek, Alex Laguë +5

We search for ultra-light axions as dark matter (DM) and dark energy particle candidates, for axion masses , by…

astro-ph.CO2022★ 22 cited

Non-linearities in the Lyman- forest and in its cross-correlation with dark matter halos

Jahmour J. Givans, Andreu Font-Ribera, Anže Slosar +6

Three-dimensional correlations of the Lyman- (Ly) forest and cross correlations between the Ly forest and quasars have been measured on large scales, allowing a precise me…

astro-ph.CO2021★ 69 cited

New limits on light dark matter - proton cross section from the cosmic large-scale structure

Keir K. Rogers, Cora Dvorkin, Hiranya V. Peiris

We set the strongest limits to-date on the velocity-independent dark matter (DM) - proton cross section for DM masses to , using large…

astro-ph.CO2021★ 60 cited

Fuzzy Dark Matter and the Dark Energy Survey Year 1 Data

Mona Dentler, David J. E. Marsh, Renée Hložek +3

Gravitational weak lensing by dark matter halos leads to a measurable imprint in the shear correlation function of galaxies. Fuzzy dark matter (FDM), composed of ultralight axion-l…

astro-ph.CO2021★ 4 cited

Constraining Ultralight Axions with Galaxy Surveys

Alex Laguë, J. Richard Bond, Renée Hložek +3

Ultralight axions and other bosons are dark matter candidates present in many high energy physics theories beyond the Standard Model. In particular, the string axiverse postulates…

astro-ph.CO2020★ 48 cited

An emulator for the Lyman- forest in beyond-CDM cosmologies

Christian Pedersen, Andreu Font-Ribera, Keir K. Rogers +4

Interpreting observations of the Lyman- forest flux power spectrum requires interpolation between a small number of expensive simulations. We present a Gaussian process emulator…

astro-ph.CO2020★ 42 cited

General framework for cosmological dark matter bounds using -body simulations

Keir K. Rogers, Hiranya V. Peiris

We present a general framework for obtaining robust bounds on the nature of dark matter using cosmological -body simulations and Lyman-alpha forest data. We construct an emulato…

astro-ph.CO2020★ 317 cited

Strong bound on canonical ultra-light axion dark matter from the Lyman-alpha forest

Keir K. Rogers, Hiranya V. Peiris

We present a new bound on the ultra-light axion (ULA) dark matter mass , using the Lyman-alpha forest to look for suppressed cosmic structure growth: a 95% lower limit…

astro-ph.CO2019★ 20 cited

Massive neutrinos and degeneracies in Lyman-alpha forest simulations

Christian Pedersen, Andreu Font-Ribera, Thomas D. Kitching +5

Using a suite of hydrodynamical simulations with cold dark matter, baryons, and neutrinos, we present a detailed study of the effect of massive neutrinos on the 1-D and 3-D flux po…

astro-ph.CO2018★ 59 cited

An Emulator for the Lyman-alpha Forest

Simeon Bird, Keir K. Rogers, Hiranya V. Peiris +3

We present methods for interpolating between the 1-D flux power spectrum of the Lyman- forest, as output by cosmological hydrodynamic simulations. Interpolation is necessary for…

astro-ph.CO2018★ 68 cited

Bayesian emulator optimisation for cosmology: application to the Lyman-alpha forest

Keir K. Rogers, Hiranya V. Peiris, Andrew Pontzen +3

The Lyman-alpha forest provides strong constraints on both cosmological parameters and intergalactic medium astrophysics, which are forecast to improve further with the next genera…

astro-ph.CO2018★ 2 cited

Cosmological Hydrodynamic Simulations with Suppressed Variance in the Lyman- Forest Power Spectrum

Lauren Anderson, Andrew Pontzen, Andreu Font-Ribera +3

We test a method to reduce unwanted sample variance when predicting Lyman- (ly) forest power spectra from cosmological hydrodynamical simulations. Sample variance arises due…

astro-ph.CO2017★ 34 cited

Correlations in the three-dimensional Lyman-alpha forest contaminated by high column density absorbers

Keir K. Rogers, Simeon Bird, Hiranya V. Peiris +3

Correlations measured in three dimensions in the Lyman-alpha forest are contaminated by the presence of the damping wings of high column density (HCD) absorbing systems of neutral…

astro-ph.CO2017★ 42 cited

Simulating the effect of high column density absorbers on the one-dimensional Lyman-alpha forest flux power spectrum

Keir K. Rogers, Simeon Bird, Hiranya V. Peiris +3

We measure the effect of high column density absorbing systems of neutral hydrogen (HI) on the one-dimensional (1D) Lyman-alpha forest flux power spectrum using cosmological hydrod…

astro-ph.CO2016★ 17 cited

Spin-SILC: CMB polarisation component separation with spin wavelets

Keir K. Rogers, Hiranya V. Peiris, Boris Leistedt +2

We present Spin-SILC, a new foreground component separation method that accurately extracts the cosmic microwave background (CMB) polarisation and modes from raw multifrequ…

astro-ph.CO2016★ 21 cited

SILC: a new Planck Internal Linear Combination CMB temperature map using directional wavelets

Keir K. Rogers, Hiranya V. Peiris, Boris Leistedt +2

We present new clean maps of the CMB temperature anisotropies (as measured by Planck) constructed with a novel internal linear combination (ILC) algorithm using directional, scale-…