CLMM

1.12.0

Getting Started

Rapid overview
Installation
Using and citing CLMM

Usage Demos

Generate mock data for a cluster
Measure WL Profiles
Model WL Profiles
Generate mock data for a cluster ensemble
Using the cosmoDC2 catalog

Mass Fitting Examples

Example 1: Ideal data
Example 1b: Impact of miscentering
Example 2: Realistic data and wrong model
Example 3: Account for the n(z) of sources
Example 4: Using a real dataset (HSC)
Example 5: Using a real datasets (DES)

Other

Model WL Profiles (different redshift inputs)
Model WL Profiles (Object Oriented)
Boost factors
Weak lensing weights
Mass conversion between different mass definitions
Generate “realistic” mock data for a cluster ensemble

Reference

API Documentation

CLMM

API Documentation
clmm.cosmology package
clmm.cosmology.numcosmo module
View page source

clmm.cosmology.numcosmo module

@file numcosmo.py Cosmology using NumCosmo

© Copyright 2018-2021, LSST DESC CLMM Contributors.

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