From 54193c01b5c6aabb263a2ee67b81619f8c1ed3e3 Mon Sep 17 00:00:00 2001 From: sfarrens Date: Mon, 12 Jun 2017 17:51:46 +0200 Subject: [PATCH] updated readme --- README.md | 2 ++ 1 file changed, 2 insertions(+) diff --git a/README.md b/README.md index b8989ae..6034abb 100644 --- a/README.md +++ b/README.md @@ -13,6 +13,7 @@ Contents 1. [Introduction](#intro_anchor) 1. [Dependencies](#depend_anchor) 1. [Execution](#exe_anchor) + 1. [Input Format](#in_format) 1. [Running the executable script](#py_ex) 1. [Running the code in a Python session](#py_sesh) 1. [Example](#eg_anchor) @@ -55,6 +56,7 @@ The low-rank approximation method can be run purely in Python. The primary code is an executable script called **sf_deconvolve.py** which is designed to take an observed (*i.e.* with PSF effects and noise) stack of galaxy images and a known PSF, and attempt to reconstruct the original images. The input format are Numpy binary files (.npy) or FITS image files (.fits). + ### Input Format The input files should have the following format: