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20202026
most citedResolved star formation in TNG100 central and satellite galaxies

8 citations · 15 across the 16 of their papers we have counts for

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15 papers · 1 filter

astro-ph.GA2026

A High-Mass Size Deficit for Void Galaxies in the Complete SDSS DR7

Olivia Curtis, Bryanne McDonough, Tereasa G. Brainerd

We characterize how environment shapes the sizes, luminosity functions, and mass functions of galaxies in large-scale underdensities by comparing the NSA catalog of the Sloan Digit…

astro-ph.GA2026

Population III Host Candidates at : Strong He II and Absent UV Metal Lines in HETDEX Ly Emitters

Mahan Mirza Khanlari, Dustin Davis, Karl Gebhardt +15

Population III (Pop III) stars are expected to produce extremely hard ionizing spectra, yet direct evidence for their signature--strong narrow He II emission with wea…

astro-ph.GA2026

A Spectral Framework for Testing the Quasi-Star Hypothesis in Little Red Dots I: Weighing LRDs by Their Super-Eddington Luminosity Ratios---No Signs of Overmassive Black Holes

Olivia Curtis, Nikko J. Cleri, Jakob M. Helton +2

We present a spectral test of the quasi-star hypothesis for Little Red Dots (LRDs) whereby a black hole grows inside a stellar-like envelope. We use Prospector to fit host galaxies…

astro-ph.GA2026

The Ĝ Infrared Search for Extraterrestrial Civilizations with Large Energy Supplies. V. When Galaxies Glow with Industry

Olivia Curtis, Aidan J. Rowland, Jason T. Wright +3

We present the most robust stellar population synthesis (SPS)-based search for galaxy-spanning technological waste heat to date, applied to 129 nearby galaxies spanning a wide rang…

astro-ph.GA2026

Project Hephaistos -- IV. James Webb Space Telescope Observations of Two Dyson Sphere Candidates

Erik Zackrisson, Arjan Bik, Anita Ali Asgar +11

We report on JWST/MIRI imaging and spectroscopy of two M-dwarf stars previously singled out by project Hephaistos as potential Dyson-sphere candidates (their candidates D and E) du…

astro-ph.GA2026★ 1 cited

HETDEX Public Data Release 1: Source Catalog 2 and Data Cubes from ~90 sq deg of Integral-Field Optical Spectroscopy

Erin Mentuch Cooper, Karl Gebhardt, Dustin Davis +36

The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) is a wide-field, integral-field spectroscopic survey designed to map the large-scale distribution of Lyman-alpha emitting…

astro-ph.GA2026

RUBIES: The Evolution of the Ionization Parameter from 0 < z < 9

Nikko J. Cleri, Zach J. Lewis, Joel Leja +10

The dimensionless ionization parameter, U=q/c, where q is the ratio of the local ionizing photon flux to the local hydrogen density, is a key metric to parameterize nebular conditi…

astro-ph.GA2026

The Dyson Minds 2025 Workshop: SETI around Black Holes

Olivia Curtis, Van Hunter Adams, Daniel Angerhausen +9

The Dyson Minds 2025 Workshop, held at the Center for Brains, Minds & Machines at MIT and organized by Penn State, MIT, and The Ultraintelligence Foundation, brought together resea…

astro-ph.GA2026

It's More Complicated Than You Think: A Forward Model to Infer the Recent Star Formation History, Bursty or Not, of Galaxy Populations

Emilie Burnham, Bingjie Wang, Joel Leja +14

Observations of the early Universe (z > 4) with the James Webb Space Telescope reveal galaxy populations with a wide range of intrinsic luminosities and colors. Bursty star formati…

astro-ph.GA2025

Void Galaxies and AGN Activity in ZOBOV-identified TNG300 Voids Out to z=3.0

Olivia Curtis, Bryanne McDonough, Tereasa Brainerd

We study void galaxies in the TNG300 simulation between redshifts and . Cosmic void catalogs were constructed using a watershed-based void-finding algorithm, and we defi…

astro-ph.GA2025

Density Profiles of TNG300 Voids across Cosmic Time

Olivia Curtis, Bryanne McDonough, Tereasa Brainerd

We present radial density profiles, as traced by luminous galaxies and dark matter particles, for voids in eleven snapshots of the \texttt{TNG300} simulation. The snapshots span 11…

astro-ph.GA2025

Measuring Scaling Relationships: Fitting Technique Matters

Bryanne McDonough, Olivia Curtis, Tereasa Brainerd

Scaling relationships, both integrated and spatially resolved, arise due to the physical processes that govern galaxy evolution and are frequently measured in both observed and sim…

astro-ph.GA2024★ 3 cited

Intrinsic and Environmental Effects on the Distribution of Star Formation in TNG100 Galaxies

Bryanne McDonough, Olivia Curtis, Tereasa Brainerd

We present radial profiles of luminosity-weighted age, , and for various populations of high- and low- mass central and satellite galaxies in the TNG100 cosmologi…

astro-ph.GA2024

Properties of Voids and Void Galaxies in the TNG300 Simulation

Olivia Curtis, Bryanne McDonough, Tereasa G. Brainerd

We investigate the properties of voids and void galaxies in the \texttt{TNG300} simulation. Using a luminous galaxy catalog and a spherical void finding algorithm, we identify 5,07…

astro-ph.GA2023★ 8 cited

Resolved star formation in TNG100 central and satellite galaxies

Bryanne McDonough, Olivia Curtis, Tereasa Brainerd

Recent cosmological hydrodynamical simulations have produced populations of numerical galaxies whose global star-forming properties are in good agreement with those of observed gal…