most citedThe role of galactic dynamics in shaping the physical properties of giant molecular clouds in Milky Way-like galaxies

53 citations · 53 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2025

Glimmers in the Cosmic Dawn. III. On the Photometrically Determined Black Hole Mass to Stellar Mass Relation Across Cosmic Time

Alice R. Young, Matthew J. Hayes, Alberto Saldana-Lopez +7

We present the results from performing spectral energy distribution (SED) fitting on 121 variable active galactic nuclei (AGN) candidates in the Hubble Ultra Deep Field (HUDF) usin…

astro-ph.GA2025

The Emergence and Ionizing Feedback of Pop III.1 Stars as Progenitors for Supermassive Black Holes

Mahsa Sanati, Jonathan C. Tan, Julien Devriendt +9

Recent observations by JWST reveal an unexpectedly abundant population of rapidly growing supermassive black holes (SMBHs) in the early Universe, underscoring the need for improved…

astro-ph.GA2025

Unveiling the drivers of the Baryon Cycles with Interpretable Multi-step Machine Learning and Simulations

Mst Shamima Khanom, Benjamin W. Keller, Javier Ignacio Saavedra Moreno

We present a new approach for understanding how galaxies lose or retain baryons by utilizing a pipeline of two machine learning methods applied the IllustrisTNG100 simulation. We e…

astro-ph.GA2025

Glimmers in the Cosmic Dawn. II. A variability census of supermassive black holes across the Universe

Vieri Cammelli, Jonathan C. Tan, Alice R. Young +7

Understanding the origin and evolution of supermassive black holes (SMBH) stands as one of the most important challenges in astrophysics and cosmology, with little current theoreti…

astro-ph.GA202053 cited

The role of galactic dynamics in shaping the physical properties of giant molecular clouds in Milky Way-like galaxies

Sarah M. R. Jeffreson, J. M. Diederik Kruijssen, Benjamin W. Keller +2

We examine the role of the large-scale galactic-dynamical environment in setting the properties of giant molecular clouds in Milky Way-like galaxies. We perform three high-resoluti…