activity
20242026
most cited-MC: Self-consistent -enhanced stellar population models covering a wide range of age, metallicity, and wavelength

1 citations · 1 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2026

Twists in the flow: revisiting convective mixing in rotating stellar models. I. Effect on the stellar structure

Poojan Agrawal, Aaron Dotter, Conny Aerts +2

Convection and rotation are both key processes in stellar evolution modelling. While standard mixing-length theory (MLT) provides a widely used modelling of convection, it neglects…

astro-ph.SR2026

MESA Isochrones and Stellar Tracks. II. Models with alpha-enhanced chemical composition

A Dotter, E Bauer, MJ Park +4

We update and expand the MESA Isochrones and Stellar Tracks (MIST) database to include variations in the alpha-capture elements, specifically [alpha/Fe]=-0.2, 0, +0.2, +0.4, and +0…

astro-ph.SR2025

MESA Isochrones and Stellar Tracks (MIST) III. The White Dwarf Cooling Sequence

Evan B. Bauer, Aaron Dotter, Charlie Conroy +3

We present a substantial update to the MESA Isochrones and Stellar Tracks (MIST) library, extending the MIST model grids and isochrones down the white dwarf (WD) cooling sequence w…

astro-ph.SR2025

Deriving Stellar Properties, Distances, and Reddenings using Photometry and Astrometry with BRUTUS

Joshua S. Speagle, Catherine Zucker, Angus Beane +18

We present brutus, an open source Python package for quickly deriving stellar properties, distances, and reddenings to stars based on grids of stellar models constrained by photome…

astro-ph.GA20241 cited

-MC: Self-consistent -enhanced stellar population models covering a wide range of age, metallicity, and wavelength

Minjung Park, Charlie Conroy, Benjamin D. Johnson +3

We present new stellar population models, -MC, self-consistently taking into account non-solar abundances for both isochrones and stellar spectra. The -MC models…