activity
20092023
most citedGalaxy Formation with BECDM: I. Turbulence and relaxation of idealised haloes

324 citations · 5k across the 89 of their papers we have counts for

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Showing 2022Show all

14 papers · 1 filter

hep-ph2022

Anticipating a New-Physics Signal in Upcoming 21-cm Power Spectrum Observations

Rennan Barkana, Anastasia Fialkov, Hongwan Liu +1

Dark matter-baryon interactions can cool the baryonic fluid, which has been shown to modify the cosmological 21-cm global signal. We show that in a two-component dark sector with a…

astro-ph.CO2022★ 57 cited

Astrophysical Constraints from the SARAS3 non-detection of the Cosmic Dawn Sky-Averaged 21-cm Signal

H. T. J. Bevins, A. Fialkov, E. de Lera Acedo +4

Observations of the redshifted 21-cm line of atomic hydrogen have resulted in several upper limits on the 21-cm power spectrum and a tentative detection of the sky-averaged signal…

astro-ph.CO2022★ 31 cited

The Second Radio Synchrotron Background Workshop: Conference Summary and Report

J. Singal, N. Fornengo, M. Regis +24

We summarize the second radio synchrotron background workshop, which took place June 15-17, 2022 in Barolo, Italy. This meeting was convened because available measurements of the d…

astro-ph.CO2022★ 110 cited

The REACH radiometer for detecting the 21-cm hydrogen signal from redshift 7.5 to 28

E. de Lera Acedo, D. I. L. de Villiers, N. Razavi-Ghods +31

Observations of the 21-cm line from primordial hydrogen promise to be one of the best tools to study the early epochs of the Universe: the Dark Ages, the Cosmic Dawn, and the subse…

astro-ph.CO2022★ 184 cited

Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations

The HERA Collaboration, Zara Abdurashidova, Tyrone Adams +92

We report the most sensitive upper limits to date on the 21 cm epoch of reionization power spectrum using 94 nights of observing with Phase I of the Hydrogen Epoch of Reionization…

astro-ph.CO2022★ 24 cited

On the Cosmic Web Elongation in Fuzzy Dark Matter Cosmologies: Effects on Density Profiles, Shapes and Alignments of Halos

Tibor Dome, Anastasia Fialkov, Philip Mocz +3

The fuzzy dark matter (FDM) scenario has received increased attention in recent years due to the small-scale challenges of the vanilla Lambda cold dark matter (CDM) cosmological…

astro-ph.CO2022★ 6 cited

Relative baryon-dark matter velocities in cosmological zoom simulations

Luke Conaboy, Ilian T. Iliev, Anastasia Fialkov +2

Supersonic relative motion between baryons and dark matter due to the decoupling of baryons from the primordial plasma after recombination affects the growth of the first small-sca…

astro-ph.CO2022★ 9 cited

Marginal Bayesian Statistics Using Masked Autoregressive Flows and Kernel Density Estimators with Examples in Cosmology

Harry Bevins, Will Handley, Pablo Lemos +3

Cosmological experiments often employ Bayesian workflows to derive constraints on cosmological and astrophysical parameters from their data. It has been shown that these constraint…

astro-ph.IM2022★ 32 cited

Antenna beam characterisation for the global 21cm experiment LEDA and its impact on signal model parameter reconstruction

M. Spinelli, G. Kyriakou, G. Bernardi +4

Cosmic Dawn, the onset of star formation in the early universe, can in principle be studied via the 21cm transition of neutral hydrogen, for which a sky-averaged absorption signal,…

astro-ph.IM2022★ 1 cited

Marginal Post Processing of Bayesian Inference Products with Normalizing Flows and Kernel Density Estimators

Harry T. J. Bevins, William J. Handley, Pablo Lemos +4

Bayesian analysis has become an indispensable tool across many different cosmological fields including the study of gravitational waves, the Cosmic Microwave Background and the 21-…

astro-ph.IM2022★ 15 cited

Bayesian Data Analysis for Sky-averaged 21-cm Experiments in the Presence of Ionospheric Effects

Emma Shen, Dominic Anstey, Eloy de Lera Acedo +1

The ionosphere introduces chromatic distortions on low frequency radio waves, and thus poses a hurdle for 21-cm cosmology. In this paper we introduce time-varying chromatic ionosph…

astro-ph.CO2022★ 45 cited

Impact of the Primordial Stellar Initial Mass Function on the 21-cm Signal

T. Gessey-Jones, N. S. Sartorio, A. Fialkov +6

Properties of the first generation of stars (Pop III), such as their initial mass function (IMF), are poorly constrained by observations and have yet to converge between simulation…

astro-ph.CO2022

A Comprehensive Bayesian re-analysis of the SARAS2 data from the Epoch of Reionization

H. T. J. Bevins, E. de Lera Acedo, A. Fialkov +4

We present a Bayesian re-analysis of the sky-averaged 21-cm experimental data from SARAS2 using nested sampling implemented with polychord, spectrally smooth foreground modelling i…

astro-ph.CO2022★ 14 cited

Emulation of the Cosmic Dawn 21-cm Power Spectrum and Classification of Excess Radio Models Using an Artificial Neural Network

Sudipta Sikder, Rennan Barkana, Itamar Reis +1

The cosmic 21-cm line of hydrogen is expected to be measured in detail by the next generation of radio telescopes. The enormous dataset from future 21-cm surveys will revolutionize…