Fitting the spectral energy distributions of galaxies
See this webpage for a full listing of stellar libraries
The series of stellar absorption lines and features used to characterise the age and metallicity of stellar clusters and galaxies
Stellar population models
Publicly Available SED models
A bag of Stellar Tracks and Isochrones
Binary Population and Spectral Synthesis
SSPs, Template Galaxy Models and more
Spectral models for Solar scaled and α-enhanced stellar populations
Flexible Stellar Population Synthesis by Conroy et al.
The Padova GALaxies AnD single stellaR populatIon modELs
The Bruzual and Charlot Stellar Population Synthesis models
GALaxy EVolutionary Synthesis models by Kotulla et al.,
includes the spectral and chemical evolution of galaxies
Models for both evolution of Balmer Absorption lines, and high
spectral resolution stellar libraries
Lick indices with individual element abundance variations
The Maraston et al. ‘fuel-consumption’ stellar population synthesis
The stellar population synthesis models for old and intermediate age
stellar populations by Vazdekis et al.
“Projet d’Etude des GALaxies par Synthese Evolutive” code by
Rocca-Volmerange et al., includes high-res SSPs based on ELODIE
Evolutionary Synthesis Models by Garcia-Vargas, Bressan, Molla
Stochastically Lighting Up Galaxies
Stellar Population Tools
Stellar population code designed to model spectrophotometric and
related properties of young galaxies
Spectral models for the first galaxies, including nebular continuum
and emission lines
Dust emission models
Library of 105 template SEDs sorted by IR luminosity
Library of IR templates sorted by α, where α is the index of the dust
mass distribution over heating intensity U; dM=U^-α dU
Code for determining IR SED given a range of heating and dust
parameter as well as the library from Draine & Li (2007)
SED fitting of sub-millimeter galaxies
Consistent UV to FIR models
Physically motivated, fast UV-FIR model based on a discrete
set of emission components
Code Investigating GALaxy Emission using Bayesian or MCMC
fitting and able to create ad-hoc models
Efstathiou+Rowan-Robinson Starburst SEDs
The Starburst SEDs of Efstathiou, Rowan-Robinson, & Siebenmorgen
(2000) based on radiative transfer.
Radiative transfer model that takes into account stellar population
synthesis as well as the effects of dust in a galaxy, Silva et al.
Starburst UV-IR SEDs described in Groves et al. (2008)
MappingsIII (also available here) code
“Modelling And Prediction in Photo-Ionized Nebulae and
Gasdynamical Shocks” photoionization radiative transfer code that
includes both line processes and dust emission.
Siebenmorgen+Kruegel Starburst SEDs
Starburst SEDs from the Siebenmorgen & Krügel (2007) model
based on radiative transfer.
Spectral modelling tool for Galaxies in Python
Stellar libraries and spectra