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most citedMESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models

2.9k citations · 17k across the 123 of their papers we have counts for

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Showing 2019Show all

10 papers · 1 filter

astro-ph.IM2019★ 75 cited

SPECULATOR: Emulating stellar population synthesis for fast and accurate galaxy spectra and photometry

Justin Alsing, Hiranya Peiris, Joel Leja +6

We present SPECULATOR - a fast, accurate, and flexible framework for emulating stellar population synthesis (SPS) models for predicting galaxy spectra and photometry. For emulating…

astro-ph.GA2019★ 135 cited

A New Census of the 0.2 < z < 3.0 Universe, Part I: The Stellar Mass Function

Joel Leja, Joshua S. Speagle, Benjamin D. Johnson +3

There has been a long-standing factor-of-two tension between the observed star formation rate density and the observed stellar mass buildup after . Recently we have propose…

astro-ph.GA2019★ 18 cited

A Lower Limit on the Mass of Our Galaxy from the H3 Survey

Dennis Zaritsky, Charlie Conroy, Huanian Zhang +5

The timing argument provides a lower limit on the mass of the Milky Way. We find, using a sample of 32 stars at kpc drawn from the H3 Spectroscopic Survey and mock catalog…

astro-ph.GA2019★ 119 cited

Resolving the Metallicity Distribution of the Stellar Halo with the H3 Survey

Charlie Conroy, Rohan P. Naidu, Dennis Zaritsky +4

The Galactic stellar halo is predicted to have formed at least partially from the tidal disruption of accreted dwarf galaxies. This assembly history should be detectable in the orb…

astro-ph.GA2019★ 155 cited

Mapping the Stellar Halo with the H3 Spectroscopic Survey

Charlie Conroy, Ana Bonaca, Phillip Cargile +8

Modern theories of galaxy formation predict that the Galactic stellar halo was hierarchically assembled from the accretion and disruption of smaller systems. This hierarchical asse…

astro-ph.SR2019★ 64 cited

MINESweeper: Spectrophotometric Modeling of Stars in the Gaia Era

Phillip A. Cargile, Charlie Conroy, Benjamin D. Johnson +4

We present MINESweeper, a tool to measure stellar parameters by jointly fitting observed spectra and broadband photometry to model isochrones and spectral libraries. This approach…