The Galaxy Cluster ‘Pypeline’ for X-ray Temperature Maps
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Updated
Oct 10, 2023 - Python
The Galaxy Cluster ‘Pypeline’ for X-ray Temperature Maps
X-ray: Generate and Analyse is a module designed to make the analysis of XMM observations simple and efficient. It provides an interface with SAS for the creation of XMM data products, as well as a way to easily perform fits (scalable for multiple observations) and retrieve information about an object, all within a Python package.
Tools for analyzing galaxy clusters.
Python routines for computing Navarro-Frenk-White halo properties
Joint X-ray and SZ data fitting code for galaxy clusters in Python
Pressure Profile Fitter for galaxy clusters in Python
Likelihood Inference Neural Network Accelerator
Codes used in a wide variety of astronomy/astrophysics
Astronomical X-ray sources surface brightness profile fitting package
Friends-of-friends algorithm used to find galaxy clusters.
The Outer Stellar Mass of Massive Galaxies: A SimpleTracer of Halo Mass with Scatter Comparable to Richnessand Reduced Projection Effects
Package to measure and model weak gravitational lensing by sattelite galaxies in galaxy clusters
University of Nottingham 3rd Year Astrophysics Project - Searching for Galaxy Clusters in the Dark Energy Survey
Website do grupo de pesquisa: IAG Machine Learning - Sistemas inteligentes para descoberta em astronomia. Instituto de Astronomia, Geofísica e Ciências Atmosféricas da Universidade de São Paulo - IAG/USP. Para acessar o código fonte do website, acesse: https://github.com/iagml/website. Este repositório possui apenas código gerado.
Code used to galaxy protocluster analysis for Lacaille, K. et al., 2019, MNRAS
My galaxy cluster sample analysis code for temperature, entropy, and metallicity radial profiles from PhD thesis in 2012
Masks a data artefact w.r.t to celestial coords and a Mangle polygon file.
Based on a Fortran code developed by Pier-Stefano Corasaniti (LUTH), the goal of this Python/C code is to provide an efficient yet easy to use library to compute the mass of the most massive galaxy cluster in a given redshift bin.
Study of BCG subtracted images of nearby clusters
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