activity
20242026
most citedMilky Way Mapper decoded abundances -- I. Shared disc enrichment patterns

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

collaborators

9 papers

astro-ph.SR2026

An upper limit on Galactic OB+black hole binaries from SDSS-V

J. Müller-Horn, H. -W. Rix, S. Shahaf +14

Binaries composed of a luminous OB star and a black hole (BH) are a key evolutionary link between massive stellar binaries and merging compact-object binaries, but only a handful a…

astro-ph.GA2026

AGN Feedback Models and AGN Demographics II: Comparing Predictions of Radiative and Total Feedback to Observations

Arjun Suresh, Michael R. Blanton

We evaluate the radiative-mode active galactic nucleus (AGN) feedback models of EAGLE, SIMBA, and TNG100 by comparing their predictions for the AGN-host galaxy relationship to new…

astro-ph.SR2026

BOSS-CLAM: Utilizing a Constrained Linear Absorption Model to Infer Stellar Parameters from BOSS Spectra

Ilija Medan, Andrew R. Casey, Alexander P. Ji +13

Large spectroscopic surveys require robust pipelines capable of inferring stellar parameters over a wide range of the Hertzsprung-Russell (HR) diagram from data of varying quality.…

astro-ph.GA2026

Milky Way Mapper decoded abundances -- II: From patterns to paths

Melissa K. Ness, Sarah Aquilina, Jennifer Mead +15

The element abundances of Milky Way disc stars encode entangled imprints of multiple enrichment processes, making it difficult to uncover the underlying chemical evolution. Here we…

astro-ph.GA2026★ 2 cited

Milky Way Mapper decoded abundances -- I. Shared disc enrichment patterns

Melissa K. Ness, Sarah Aquilina, Jennifer Mead +15

Elemental abundances in the Milky Way disc trace its star-formation and enrichment history, but predicting these abundances from theory is limited by uncertain nucleosynthetic yiel…

astro-ph.GA2025★ 1 cited

The Eddington Ratio Distribution of Narrow Line Active Galactic Nuclei

Michael R. Blanton, Arjun Suresh, Kyle B. Westfall +2

We measure the Eddington ratio distribution of local optical narrow-line active galactic nuclei (AGN) as a function of host galaxy properties, as a potential test of galaxy formati…

astro-ph.GA2025

AGN Feedback Models and AGN Demographics I: Radio-Mode AGN in EAGLE, SIMBA and TNG100 are Inconsistent with Observations

Arjun Suresh, Michael R. Blanton, Douglas Rennehan

We compare predictions of how Active Galactic Nuclei (AGN) populate host galaxies at low redshifts to observations, finding large discrepancies between cosmological simulation pred…

astro-ph.GA2024

Testing the accuracy of SED modeling techniques using the NIHAO-SKIRT-Catalog

Nicholas Faucher, Michael R. Blanton

We use simulated galaxy observations from the NIHAO-SKIRT-Catalog to test the accuracy of Spectral Energy Distribution (SED) modeling techniques. SED modeling is an essential tool…

astro-ph.GA2024

A dust attenuation model inspired by the NIHAO-SKIRT-Catalog

Nicholas Faucher, Michael R. Blanton

We use simulated attenuation curves from the NIHAO-SKIRT-Catalog to test the flexibility of commonly used dust attenuation models in the face of the variations expected from realis…