Pressure Profile Fitter for galaxy clusters in Python
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Updated
Sep 5, 2024 - Python
Pressure Profile Fitter for galaxy clusters in Python
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.
a galaxy cluster catalogue obtained in directions of SZcat by applying deep learning method to ACT+Planck maps
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.
Repository for suppelementary material from my publications on the entropy core problem
A Python library to analyse zoom-in hydrodynamic simulations of groups and clusters of galaxies.
Repository for suppelementary material from my publication on the rotational kinetic SZ effect in MACSIS
Code to analyse data outputs from zoom galaxy cluster simulations investigating the effect of different mass and spatial resolutions.
Documentation from my PhD thesis in hydrodynamic cosmological simulations.
The Galaxy Cluster ‘Pypeline’ for X-ray Temperature Maps
A specialized repository for fitting the Vikhlinin model to galaxy cluster density profiles.
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.
Masks a data artefact w.r.t to celestial coords and a Mangle polygon file.
Astronomical X-ray sources surface brightness profile fitting package
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
University based project on simulating and analysing galaxy clustering.
The Outer Stellar Mass of Massive Galaxies: A SimpleTracer of Halo Mass with Scatter Comparable to Richnessand Reduced Projection Effects
Likelihood Inference Neural Network Accelerator
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