Astronomical X-ray sources surface brightness profile fitting package
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Updated
Nov 25, 2022 - Jupyter Notebook
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
Masks a data artefact w.r.t to celestial coords and a Mangle polygon file.
University of Nottingham 3rd Year Astrophysics Project - Searching for Galaxy Clusters in the Dark Energy Survey
Repository for suppelementary material from my publication on the rotational kinetic SZ effect in MACSIS
Pressure Profile Fitter for galaxy clusters in Python
Code to analyse data outputs from zoom galaxy cluster simulations investigating the effect of different mass and spatial resolutions.
A Python library to analyse zoom-in hydrodynamic simulations of groups and clusters of galaxies.
Tools to analyze Planck CMB maps with a focus on thermal and kinetic SZ effect. Includes implementation of Internal Linear Combination (ILC) and Wiener filter using NIFTy. Supplementary repo to master thesis
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