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

2 citations · 2 across the 4 of their papers we have counts for

collaborators

7 papers

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.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.GA20252 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

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…