activity
20162024
most citedIron K line of Kerr black holes with scalar hair

94 citations · 174 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.CO20241 cited

Debiasing with Diffusion: Probabilistic reconstruction of Dark Matter fields from galaxies with CAMELS

Victoria Ono, Core Francisco Park, Nayantara Mudur +3

Galaxies are biased tracers of the underlying cosmic web, which is dominated by dark matter components that cannot be directly observed. Galaxy formation simulations can be used to…

astro-ph.CO20231 cited

Probabilistic reconstruction of Dark Matter fields from biased tracers using diffusion models

Core Francisco Park, Victoria Ono, Nayantara Mudur +2

Galaxies are biased tracers of the underlying cosmic web, which is dominated by dark matter components that cannot be directly observed. The relationship between dark matter densit…

astro-ph.GA2023

Detecting Wandering Intermediate-Mass Black Holes with AXIS in the Milky Way and Local Massive Galaxies

Fabio Pacucci, Bryan Seepaul, Yueying Ni +2

This white paper explores the detectability of intermediate-mass black holes (IMBHs) wandering in the Milky Way (MW) and massive local galaxies, with a particular emphasis on the r…

astro-ph.GA20238 cited

Extreme Tidal Stripping May Explain the Overmassive Black Hole in Leo I: a Proof of Concept

Fabio Pacucci, Yueying Ni, Abraham Loeb

A recent study found dynamical evidence of a supermassive black hole of at the center of Leo I, the most distant dwarf spheroidal galaxy of th…

astro-ph.CO20231 cited

Cosmology with multiple galaxies

Chaitanya Chawak, Francisco Villaescusa-Navarro, Nicolas Echeverri Rojas +3

Recent works have discovered a relatively tight correlation between and properties of individual simulated galaxies. Because of this, it has been shown that constraints…

astro-ph.CO20231 cited

Modeling Quasar Proximity Zones in a Realistic Cosmological Environment with a Self-consistent Light Curve

Yihao Zhou, Huanqing Chen, Tiziana Di Matteo +3

We study quasar proximity zones in a simulation that includes a self-consistent quasar formation model and realistic IGM environments. The quasar host halo is $10^{13}\ M_{\mathrm{…