activity
20232026
most citedApplying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation

3 citations · 4 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2026

GalSyn I: A Forward-Modeling Code for Synthetic Galaxy Observations from Hydrodynamical Simulations and First Data Release from IllustrisTNG

Abdurro'uf, Henry C. Ferguson, Samir Salim +9

We present GalSyn (Galaxy Synthesizer), a modular and flexible Python package for generating synthetic observations from hydrodynamical galaxy simulations. GalSyn generates synthet…

astro-ph.CO2025

Towards Reconciling Reionization with JWST: The Role of Bright Galaxies and Strong Feedback

Ankita Bera, Sultan Hassan, Robert Feldmann +2

The elevated UV luminosity functions (UVLF) from recent James Webb Space Telescope (JWST) have challenged the viability of existing theoretical models. To address this, we use a se…

astro-ph.GA2025

How does feedback affect the star formation histories of galaxies?

Kartheik G. Iyer, Tjitske K. Starkenburg, Greg L. Bryan +20

Star formation in galaxies is regulated by the interplay of a range of processes that shape the multiphase gas in the interstellar and circumgalactic media. Using the CAMELS suite…

astro-ph.GA2025★ 3 cited

Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation

Jan D. Burger, Volker Springel, Eve C. Ostriker +11

Modern high-resolution simulations of the interstellar medium (ISM) have shown that key factors in governing star formation are the competing influences of radiative dissipation, p…

astro-ph.GA2024

Towards Implementation of the Pressure-Regulated, Feedback-Modulated Model of Star Formation in Cosmological Simulations: Methods and Application to TNG

Sultan Hassan, Eve C. Ostriker, Chang-Goo Kim +12

Traditional star formation subgrid models implemented in cosmological galaxy formation simulations, such as that of Springel & Hernquist (2003, hereafter SH03), employ adjustable p…

astro-ph.GA2024

Learning the Universe: GalactISM simulations of resolved star formation and galactic outflows across main sequence and quenched galactic environments

Sarah M. R. Jeffreson, Eve C. Ostriker, Chang-Goo Kim +5

We present a suite of six high-resolution chemo-dynamical simulations of isolated galaxies, spanning observed disk-dominated environments on the star-forming main sequence, as well…

astro-ph.GA2024★ 1 cited

Metallicity Dependence of Pressure-Regulated Feedback-Modulated Star Formation in the TIGRESS-NCR Simulation Suite

Chang-Goo Kim, Eve C. Ostriker, Jeong-Gyu Kim +8

We present a new simulation suite for the star-forming interstellar medium (ISM) in galactic disks using the TIGRESS-NCR framework. Distinctive aspects of our simulation suite are:…

astro-ph.GA2023

Deep Learning Voigt Profiles I. Single-Cloud Doublets

Bryson Stemock, Christopher W. Churchill, Avery Lee +3

Voigt profile (VP) decomposition of quasar absorption lines is key to studying intergalactic gas and the baryon cycle governing the formation and evolution of galaxies. The VP velo…