activity
20102026
most citedThe impact of an evolving stellar initial mass function on early galaxies and reionisation

56 citations · 119 across the 15 of their papers we have counts for

collaborators

17 papers

astro-ph.GA2026

Stability of rotation axis of galactic disks in HESTIA suite

Naira R. Arakelyan, Sergey V. Pilipenko, Stefan Gottlöber +3

We have found that in approximately 1/4 of Milky Way or M31 analogues in the HESTIA suite of simulations there is a significant, , change in the axis of rotation orienta…

astro-ph.GA2026

Enabling Cosmic Web Analysis at Gigaparsec Scales: A Multi Block Approach for DisPerSE

Ankit Singh, Frazer Pearce, Meghan Gray +1

Cosmic filaments are the longest structures in the Universe and the dominant element of the cosmic web, channelling matter onto clusters and shaping the environments in which galax…

astro-ph.CO2025

A continuous parameterization of the cosmic web

C. Yamila Yaryura, Mario G. Abadi, Noam I. Libeskind +3

The intrinsic properties of galaxies are influenced by their environments, underscoring the environment's critical role in galaxy formation and evolution. Traditionally, these envi…

astro-ph.IM2025

Ginnungagap -- a massively parallel cosmological initial conditions generator

Sergey Pilipenko, Gustavo Yepes, Stefan Gottlöber +1

Ginnungagap is a fully parallel (MPI+OpenMP) code designed to generate cosmological initial conditions for simulations involving very large numbers of particles. It operates in sev…

astro-ph.GA2025

Machine Learning the Dark Matter Halo Mass of the Milky Way

Elaheh Hayati, Peter Behroozi, Ekta Patel +3

Although numerous dynamical techniques have been developed to estimate the total dark matter halo mass of the Milky Way, it remains poorly constrained, with typical systematic unce…

astro-ph.GA2025

The life and times of dark matter haloes: what will I be when I grow up?

Julian Onions, Frazer Pearce, Alexander Knebe +6

Are the most massive objects in the Universe today the direct descendants of the most massive objects at higher redshift? We address this question by tracing the evolutionary histo…

astro-ph.GA2025★ 2 cited

Line Intensity Mapping Prediction from the Cosmic Dawn (CoDa) III Simulation for H from Galaxies and the Intergalactic Medium during the Epoch of Reionization

Eugene Hyeonmin Lee, Joohyun Lee, Paul R. Shapiro +13

The evolution of large-scale structure, galaxies and the intergalactic medium (IGM) during the Epoch of Reionization (EoR) can be probed by upcoming Line Intensity Mapping (LIM) ex…

astro-ph.CO2024

The Thermal Sunyaev-Zel'dovich Effect from the Epoch of Reionization

Ilian T. Iliev, Azizah R. Hosein, Jens Chluba +11

The thermal Sunyaev-Zel'dovich (tSZ) effect arises from inverse Compton scattering of low energy photons onto thermal electrons, proportional to the integrated electron pressure, a…

astro-ph.GA2024★ 1 cited

Variable gravitational potential of Milky Way analogues in HESTIA suite

Naira R. Arakelyan, Sergey V. Pilipenko, Stefan Gottlöber +3

Investigations of trajectories of various objects orbiting the Milky Way (MW) halo with modern precision, achievable in observations by Gaia, requires sophisticated, non-stationary…

astro-ph.CO2024★ 2 cited

Dispersion Measures of Fast Radio Bursts through the Epoch of Reionization

Joshua J. Ziegler, Paul R. Shapiro, Taha Dawoodbhoy +13

Dispersion measures (DM) of fast radio bursts (FRBs) probe the density of electrons in the intergalactic medium (IGM) along their lines-of-sight, including the average density vers…

astro-ph.CO2024

Constraining Reionization with Lyα Damping-Wing Absorption in Galaxy Spectra: A Machine Learning Model Based on Reionization Simulations

Hyunbae Park, Intae Jung, Hidenobu Yajima +8

Recently, NIRSpec PRISM/CLEAR observations by JWST have begun providing rest-frame UV continuum measurements of galaxies at , revealing signatures of Ly damping-wing…

astro-ph.GA2024

Astraeus X: Indications of a top-heavy initial mass function in highly star-forming galaxies from JWST observations at z>10

Anne Hutter, Elie R Cueto, Pratika Dayal +3

The James Webb Space Telescope (JWST) has uncovered an abundance of galaxies bright in the ultraviolet (UV) that has challenged traditional theoretical models at high redshi…

astro-ph.GA2024★ 3 cited

Dust-UV offsets in high-redshift galaxies in the Cosmic Dawn III simulation

Pierre Ocvirk, Joseph S. W. Lewis, Luke Conaboy +13

Recent observations have revealed puzzling spatial disparities between ALMA dust continuum and UV emission as seen by HST and JWST in galaxies at (e.g. ALPINE and REBELS su…

astro-ph.GA2023★ 56 cited

The impact of an evolving stellar initial mass function on early galaxies and reionisation

Elie Rasmussen Cueto, Anne Hutter, Pratika Dayal +5

Observations with JWST have revealed an unexpected high abundance of bright z>10 galaxy candidates. We explore whether a stellar initial mass function (IMF) that becomes increasing…

astro-ph.GA2020★ 16 cited

Astraeus III: The environment and physical properties of reionization sources

Anne Hutter, Pratika Dayal, Laurent Legrand +2

In this work, we use the {\sc astraeus} (seminumerical rAdiative tranSfer coupling of galaxy formaTion and Reionization in N-body dArk mattEr simUlationS) framework which couples g…

astro-ph.CO2014★ 8 cited

Universal void density profiles from simulation and SDSS

S. Nadathur, S. Hotchkiss, J. M. Diego +4

We discuss the universality and self-similarity of void density profiles, for voids in realistic mock luminous red galaxy (LRG) catalogues from the Jubilee simulation, as well as i…

astro-ph.CO2010★ 31 cited

The Relation Between Halo Shape, Velocity Dispersion and Formation Time

C. Ragone-Figueroa, M. Plionis, M. Merchan +2

We use dark matter haloes identified in the MareNostrum Universe and galaxy groups identified in the Sloan Data Release 7 galaxy catalogue, to study the relation between halo shape…