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 …

2.3. Old Population 2.4. Magnetic Fields of Neutron Stars 2.5. Z and Atoll Classification 3.
Type I X-ray Bursts 3.1. Introduction 3.2. Burst Profiles 3.3. Burst Spectral Analysis 3.4 …

This paper documents the seventeenth data release (DR17) from the Sloan Digital Sky
Surveys; the fifth and final release from the fourth phase (SDSS-IV). DR17 contains the …

The Sloan Digital Sky Surveys (SDSS) have been almost continuously observing the skies
for over 20 yr, since the project began with a first phase in 1998 (SDSS-I; York et al. 2000) …

We present a new model for computing the spectral evolution of stellar populations at ages
between 1× 105 and 2× 1010 yr at a resolution of 3 Å across the whole wavelength range …

We present P 3D, an analysis pipeline based on the FIT3D fitting tool, developed to explore
the properties of the stellar populations and ionized gas of integral field spectroscopy (IFS) …

A new stellar library developed for stellar population synthesis modelling is presented. The
library consists of 985 stars spanning a large range in atmospheric parameters. The spectra …

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

We derive stellar metallicities, light-weighted ages and stellar masses for a magnitude-
limited sample of 175 128 galaxies drawn from the Sloan Digital Sky Survey Data Release …

The construction of detailed models for intermediate and old stellar populations is described.
Input parameters include metallicity (-2 less than (Fe/H) less than 0.5), single-burst age …