Nbody6++GPU

This is Nbody6++GPU, an N-body star cluster simulation code, maintained by Rainer Spurzem and team.

Code for the ASteCA package.

NBODY6

Search for Binary Supernova Ejected OB-type Runaway Stars from Young Open Clusters | Master Thesis Project

Star Cluster Analysis in nearby Galaxies (Krittika Summer Project 5.0)

SteParKin code determine Galactic-space velocity components (U, V, W), evaluate their membership to young kinematic moving groups and associations and assign their stellar populations.

MASSCLEAN cluster generator.

Brand new graphing tool for Skynet

Package for calculating empirical isochrones for star clusters and agglomorates from purely observational data.

Tool for astronomical data analysis, quantifying the structure of young star clusters using a fractal dimension.

Little pipeline, based on Match program, for matching stars in different catalogues with offset in coordinates

This python script simulates the hierarchical merging of black holes for different star cluster environments: Open, Globular, and Nuclear.

Study of age, metallicity and extra-tidal region of a globular cluster NGC 4147 | Observational Astronomy Lab Project

Data reduction for .fits files using the Astropy module and affiliate modules.

Finding Age, Mass, Extinction of star CLUSTers (astrophysical package written in python and Fortran)

MASSCLEAN cluster generator.

Efficient Likelihood Inference for Stellar Ages

No description provided.

This project from the series of "Statistical and Computational Methods in Physics" is a simple image processing project that uses a “Discrete Fourier transform” (DFT) on a collection of fake simple star-cluster images.

Unsupervised identification of M67 cluster members using Gaia DR3 and pyUPMASK with spatial and kinematic filtering.

nbody

This project from the series of "Statistical and Computational Methods in Physics" is a simple image processing project that uses a maximum likelihood technique on a collection of fake simple star-cluster images.

Final project for the "Laboratory of Computational Physics - mod B" course at Unipd during 2020/2021.

GRoupEd sTar formAtion: converting sink particles to stars that are sampled from observational initial mass function (IMF)

Analysis of NGC-104 globular star cluster.