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20242026
most citedDark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear

4 citations · 9 across the 14 of their papers we have counts for

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astro-ph.CO2024

The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level

Mikhail M. Ivanov, Carolina Cuesta-Lazaro, Andrej Obuljen +8

Cosmological analyses of redshift space clustering data are primarily based on using luminous ``red'' galaxies (LRGs) and ``blue'' emission line galaxies (ELGs) to trace underlying…

astro-ph.GA2024

Signatures of black hole seeding in the local Universe: Predictions from the BRAHMA cosmological simulations

Aklant K Bhowmick, Laura Blecha, Paul Torrey +8

The first "seeds" of supermassive black holes (BHs) continue to be an outstanding puzzle, and it is currently unclear whether the imprints of early seed formation survive today. He…

astro-ph.GA2024

The THESAN project: tracking the expansion and merger histories of ionized bubbles during the Epoch of Reionization

Nathan Jamieson, Aaron Smith, Meredith Neyer +7

The growth of ionized hydrogen bubbles in the intergalactic medium around early luminous objects is a fundamental process during the Epoch of Reionization (EoR). In this study, we…

astro-ph.GA2024

The THESAN project: galaxy sizes during the epoch of reionization

Xuejian Shen, Mark Vogelsberger, Josh Borrow +12

We investigate galaxy sizes at redshift with the cosmological radiation-magneto-hydrodynamic simulation suite THESAN(-HR). These simulations simultaneously capture the…

astro-ph.GA2024

Brightest Cluster Galaxy Offsets in Cold Dark Matter

Cian Roche, Michael McDonald, Josh Borrow +7

The distribution of offsets between the brightest cluster galaxies of galaxy clusters and the centroid of their dark matter distributions is a promising probe of the underlying dar…

astro-ph.CO2024

The boundary of cosmic filaments

Wei Wang, Peng Wang, Hong Guo +12

For decades, the boundary of cosmic filaments have been a subject of debate. In this work, we determine the physically-motivated radii of filaments by constructing stacked galaxy n…