Tools for analyzing galaxy clusters.
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Updated
Nov 21, 2019 - Jupyter Notebook
Tools for analyzing galaxy clusters.
The Galaxy Cluster ‘Pypeline’ for X-ray Temperature Maps
Python routines for computing Navarro-Frenk-White halo properties
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.
Code used to galaxy protocluster analysis for Lacaille, K. et al., 2019, MNRAS
The Outer Stellar Mass of Massive Galaxies: A SimpleTracer of Halo Mass with Scatter Comparable to Richnessand Reduced Projection Effects
Codes used in a wide variety of astronomy/astrophysics
Analysis of the galaxy clusters in the cosmological simulation - Illustris simulation
Likelihood Inference Neural Network Accelerator
Astronomical X-ray sources surface brightness profile fitting package
Study of BCG subtracted images of nearby clusters
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.
Modelling tool for the rotational kinetic Sunyae-Zel'dovich effect on galaxy clusters and groups.
My galaxy cluster sample analysis code for temperature, entropy, and metallicity radial profiles from PhD thesis in 2012
A Predictive View of Bayesian Clustering
Photometric analysis of galaxy cluster MACSJ0416.1-2403, a project to measure the actual extent of galaxy clusters by means of the properties of their galaxies
Simulation of metal diffusion in the ICM for the Perseus Cluster The aim of the project is to show the possible parameters for efficient metal distribution under reasonable diffusion timescales to reproduce observed abundance profile.
Package to measure and model weak gravitational lensing by sattelite galaxies in galaxy clusters
Repository for suppelementary material from my publications on the entropy core problem
a galaxy cluster catalogue obtained in directions of SZcat by applying deep learning method to ACT+Planck maps
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