nudging travis
@@ -22,3 +22,4 @@ The source codes included in this directory can be used to reproduce all benchma
* **cosmolss_cclbenchmarking.tar.gz** : this tarball contains CosmoLSS used for benchmarking the galaxy clustering, galaxy-galaxy lensing, and cosmic shear angular power spectra and correlation functions including intrinsic alignments for all tomograhic bin combinations and both analytic/histogram redshift distributions. It can be downloaded from here: https://github.com/sjoudaki/CosmoLSS_CCLbenchmarking. This includes all 3x2pt terms: galaxy-galaxy (gg), galaxy-shear (gG), galaxy-intrinsic (gI), shear-shear (GG), shear-intrinsic (GI), intrinsic-intrinsic (II), galaxy-total (gG+gI), and total-total (GG+GI+II). Please make sure that you have installed Intel Fortran 14 or higher. To compile the code, enter the directory "cosmolss_cclbenchmarking/source", type "make clean", then "make". Then go back to the main directory (i.e. "cd .."), type "./cosmomc testcclbenchmarking.ini". This will generate all of the benchmark files for the analytic redshift distributions. For the histogram case, enter "cosmolss_cclbenchmarking/source" again, and type "cp CosmoLSS_cclbenchmarking_histo.f90 CosmoLSS.f90". Now, type "make", then go back to the main directory ("cd .."), and type "./cosmomc testcclbenchmarking.ini". This now generates all of the benchmark files for the histogram redshift distributions. For completeness, the downloaded tarball contains all of the benchmark files used in the unit tests and python notebook.
* Additional GGL benchmarks were produced using CosmoLSS. CosmoLSS can be downloaded from github: https://github.com/sjoudaki/cosmolss. To reproduce the benchmarks, go to "your CosmoLSS directory"/source, type make clean, then make. Go back to the main directory, type ./cosmomc cclbenchmarking.ini. The code then produces the benchmark files.
* **ggl_benchmarks.zip** : this zip file contains a python executable myggl.py that can be run to generate additional galaxy-galaxy lensing benchmarks for the bin combination 1-2, including the angular power spectra and correlation function.
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