diff --git a/README.md b/README.md index a43e4f4..a290692 100644 --- a/README.md +++ b/README.md @@ -2,21 +2,14 @@ [![Build Status](https://travis-ci.com/cschreib/fastpp.svg?branch=master)](https://travis-ci.com/cschreib/fastpp) - + - [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) @@ -35,17 +28,20 @@ - [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) + # 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: