The spectral energy distributions (SEDs) of galaxies are shaped by nearly every physical
property of the system, including the star-formation history, metal content, abundance …

Inference of the physical properties of stellar populations from observed photometry and
spectroscopy is a key goal in the study of galaxy evolution. In recent years, the quality and …

The stellar masses, mean ages, metallicities, and star formation histories of galaxies are
now commonly estimated via stellar population synthesis (SPS) techniques. SPS relies on …

Evolutionary population synthesis models for a wide range of metallicities, ages, star
formation histories, initial mass functions and horizontal branch morphologies, including …

ABSTRACT We present a 0.8–5 μm spectral library of 210 cool stars observed at a resolving
power of R≡ λ/Δλ∼ 2000 with the medium-resolution infrared spectrograph, SpeX, at the …

We present a new spectral fitting code, firefly, for deriving the stellar population properties of
stellar systems. firefly is a chi-squared minimization fitting code that fits combinations of …

We have incorporated the latest release of the Padova models into the evolutionary
synthesis code Starburst99. The Padova tracks were extended to include the full asymptotic …

Context. The third Gaia Data Release covers 34 months of data and includes the second
Gaia catalogue of long-period variables (LPVs), with G variability amplitudes larger than 0.1 …

We present the first release of the MaNGA Stellar Library (MaStar), which is a large, well-
calibrated, high-quality empirical library covering the wavelength range 3622–10354 Å at a …

We report on an analysis of the gas and dust budget in the interstellar medium (ISM) of the
Large Magellanic Cloud (LMC). Recent observations from the Spitzer Space Telescope …