zdm
zdm is a Python package for Fast Radio Burst (FRB) redshift-dispersion measure (z-DM) calculations. It provides tools for statistical modeling of FRB populations, computing likelihoods, and constraining cosmological and FRB population parameters.
The package implements the theoretical framework for relating observed FRB dispersion measures to their redshifts, accounting for contributions from the Milky Way, host galaxies, and the intergalactic medium.
Key Features
Cosmological Modeling: Lambda-CDM cosmology with configurable parameters
z-DM Grids: Efficient computation of probability distributions over redshift and dispersion measure
Survey Support: Built-in support for CHIME, ASKAP, Parkes and other FRB surveys
Likelihood Analysis: Compute likelihoods for FRB populations given survey data
MCMC Parameter Estimation: Integration with emcee for Bayesian parameter inference
Repeater Modeling: Support for repeating FRB population models
Getting Started
User Guide
Development
Citation
If you use zdm in your research, please cite:
@article{james2022,
author = {James, Clancy W. and others},
title = {A measurement of Hubble's Constant using Fast Radio Bursts},
journal = {MNRAS},
year = {2022}
}
License
zdm is licensed under a 3-clause BSD style license. See the LICENSE file
in the repository for details.