8. Output

This section describes the output produced by Nemo, and the main files of interest.

8.1. Directory Structure

The main Nemo script (launched with the nemo command) creates a folder (by default sharing the name of the configuration file, but with .yml removed) in the current working directory under which it stores all of its output. We will refer to this as the output directory hereafter.

After nemo has run, within the output directory, you will find the following:

output/
    diagnostics/
    filteredMaps/
    mocks/
    selFn/
    output_optimalCatalog.csv
    output_optimalCatalog.fits

diagnostics/

This directory contains output that is useful for debugging (mainly plots in .pdf and .png format, but the filter kernels are also cached here).

filteredMaps/

This directory contains the filtered maps, named according to the filter definitions given in the configuration file. For more on the maps themselves, see Filtered Maps below.

mocks/

If you run the nemoMock script, numbered mock catalogs will be written into this directory (otherwise it will be empty).

selFn/

This directory contains all the necessary information for calculating the completeness of the survey, given a model for the relationship between the SZ signal and mass, and an assumed halo mass function. For more information, see Tutorial: Using the Selection Function for Cluster Cosmology and/or Selection Function below.

8.2. Catalogs

And region files. M500 too.

8.3. Filtered Maps

8.4. Selection Function

8.5. Diagnostics