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Generating SZ Profiles
jacksonodonnell edited this page Sep 25, 2019
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3 revisions
By Jackson O'Donnell
The core of the Y3 clusters analysis uses weak lensing profiles to calibrate cluster masses. We can also, however, cross-correlate with the signal cluster imprint on the CMB through the Sunyzev-Zeldovich effect.
Inside the docker image (or on your machine if you're running locally),
# Install colossus - needed to convert between cluster mass definitions
$ pip install colossus==1.2.11
$ pushd /tmp
# Install JOD's of cluster_toolkit - contains pressure profiles
$ git clone https://github.com/jhod0/cluster_toolkit
$ pushd cluster_toolkit
$ git checkout pressure-profiles
$ python setup.py install
$ pushd $COSMOSIS_SRC_DIR/cosmosis-standard-library/
# Now install the clustef_toolkit cosmosis wrapper into a directory called "cluster-sz"
$ git clone https://github.com/jhod0/cosmosis-cluster-sz cluster-sz
$ popd; popd; popd