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 …

Fitting the spectral energy distributions (SEDs) of galaxies is an almost universally used
technique that has matured significantly in the last decade. Model predictions and fitting …

BANYAN Σ is a new Bayesian algorithm to identify members of young stellar associations
within 150 pc of the Sun. It includes 27 young associations with ages in the range∼ 1–800 …

We describe the survey design, calibration, commissioning, and emission-line detection
algorithms for the Hobby–Eberly Telescope Dark Energy Experiment (HETDEX). The goal of …

The relation between galaxy stellar mass and gas-phase metallicity is a sensitive diagnostic
of the main processes that drive galaxy evolution, namely cosmological gas inflow, metal …

Stellar population synthesis (SPS) provides the link between the stellar and dust content of
galaxies and their observed spectral energy distributions. In the present work, we perform a …

We have carried out a survey of the north and south ecliptic poles, EP-N and EP-S,
respectively, with the Spitzer Space Telescope and the Wide-field Infrared Survey Explorer …

We present synthetic spectral energy distributions (SEDs) for single-age, single-metallicity
stellar populations (SSPs) covering the full optical spectral range at moderately high …

According to the Λ cold dark matter (ΛCDM) cosmology, present-day galaxies with stellar
masses M⋆> 10 11 M⊙ should contain a sizable fraction of dark matter within their stellar …

Aims. We present a number of improvements to the MILES library and stellar population
models. We correct some small errors in the radial velocities of the stars, measure the …