activity
20042026
most citedAstro2020 Science White Paper: The Next Decade of Astroinformatics and Astrostatistics

1 citations · 1 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2026

Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos

Yikun Wang, Idit Zehavi, Sergio Contreras +3

Baryonic physics is anticipated to be a major source of systematic uncertainty in current and future large-scale cosmological surveys. We investigate how baryonic effects on halo d…

astro-ph.CO2026

Cosmological constraints from the small scale clustering of Emission Line Galaxies

Sara Ortega-Martinez, Raul E. Angulo, Sergio Contreras +7

Spectroscopic surveys such as the Dark Energy Spectroscopic Instrument (DESI) and Euclid are mapping the spatial distribution of millions of galaxies, with Emission Line Galaxies (…

astro-ph.CO2026

Correlated residuals in Tully-Fisher and Fundamental Plane relations and their impact on peculiar velocity measurements

Tyann Dumerchat, Raul E. Angulo, Julian Bautista +3

The Tully-Fisher (TF) and Fundamental Plane (FP) relations are widely used to infer extragalactic distances and peculiar velocities, enabling measurements of large-scale velocity s…

astro-ph.GA2026

Implications of the nanoHertz Gravitational-Wave Background for Galactic Feedback and Massive Black Hole Growth

Megan Taylor Tillman, Blakesley Burkhart, Chiara M. F. Mingarelli +5

We investigate how pulsar timing array (PTA) measurements of the nanoHertz gravitational-wave background (GWB) can constrain models for the growth history of supermassive black hol…

astro-ph.CO2025

Estimating the triaxiality of massive clusters from 2D observables in MillenniumTNG with machine learning

Ana Maria Delgado, Michelle Ntampaka, Sownak Bose +7

Properties of massive galaxy clusters, such as mass abundance and concentration, are sensitive to cosmology, making cluster statistics a powerful tool for cosmological studies. How…

astro-ph.GA2025

Development of Turbulence in Post-shock Regions

Michael M. Foley, Philip Mocz, Blakesley Burkhart +2

Supersonic isothermal turbulence is ubiquitous in the interstellar medium. This work presents high-resolution AREPO hydrodynamical simulations of isolated shocks moving through sup…

astro-ph.CO2025

Infalling ultra-faint dwarfs as emissaries of the Axiverse

A. Pozo, T. Broadhurst, H. N. Luu +8

Recent discoveries of ultra-faint dwarf galaxies (UFDs) infalling onto the Milky Way, namely Leo K \& M at kpc, considerably strengthens the case that UFDs constitute…

astro-ph.IM2019★ 1 cited

Astro2020 Science White Paper: The Next Decade of Astroinformatics and Astrostatistics

A. Siemiginowska, G. Eadie, I. Czekala +49

Over the past century, major advances in astronomy and astrophysics have been largely driven by improvements in instrumentation and data collection. With the amassing of high quali…

astro-ph2004

Massive galaxies at redshift 2 in cosmological hydrodynamic simulations

Kentaro Nagamine, Renyue Cen, Lars Hernquist +2

We study the properties of galaxies at z=2 in a Lambda cold dark matter universe, using two different types of hydrodynamic simulation methods -- Eulerian TVD and smoothed particle…