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cschreib committed Jun 12, 2019
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[![Build Status](https://travis-ci.com/cschreib/fastpp.svg?branch=master)](https://travis-ci.com/cschreib/fastpp)

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- [Description](#description)
- [Install instructions](#install-instructions)
- [Benchmarks](#benchmarks)
- [Hardware/software](#hardwaresoftware)
- [Run 1: a catalog of galaxies with broadband fluxes](#run-1-a-catalog-of-galaxies-with-broadband-fluxes)
- [Parameters](#parameters)
- [Runs](#runs)
- [Recorded times](#recorded-times)
- [Memory consumption](#memory-consumption)
- [Run 2: one galaxy with a high resolution spectrum](#run-2-one-galaxy-with-a-high-resolution-spectrum)
- [Parameters](#parameters-1)
- [Recorded times](#recorded-times-1)
- [Memory consumption](#memory-consumption-1)
- [What is the trick?](#what-is-the-trick)
- [Why is it faster?](#why-is-it-faster)
- [Why does it use so little memory?](#why-does-it-use-so-little-memory)
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- [Confidence intervals from chi2 grid](#confidence-intervals-from-chi2-grid)
- [Controlling the cache](#controlling-the-cache)
- [More output options](#more-output-options)
- [Non-parametric SFH quantities](#non-parametric-sfh-quantities)
- [Custom star formation histories](#custom-star-formation-histories)
- [Non-parametric SFH quantities](#non-parametric-sfh-quantities)
- [Differential attenuation](#differential-attenuation)
- [Using priors on the infrared luminosity](#using-priors-on-the-infrared-luminosity)
- [Better treatment of spectra](#better-treatment-of-spectra)
- [Velocity broadening](#velocity-broadening)
- [Continuum indices](#continuum-indices)
- [Additional documentation](#additional-documentation)
- [Adding new filters](#adding-new-filters)
- [Acknowledgments](#acknowledgments)

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# Description

This is a C++ version of the popular SED fitting code [FAST](http://w.astro.berkeley.edu/~mariska/FAST.html) (Kriek et al. 2009). Below is a list of the main selling points:
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