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.

Codes used in a wide variety of astronomy/astrophysics

Pipeline which takes raw VLA data and yields science-ready data products, i.e. star formation rates

CARPP: Core Analysis via Radiative transfer and Profile Parameters! A 3D radiative transfer molecular core analyzing tool through multi-wavelength dust continuum data. It retrieves density profile and helps distinguishing hydrostatic equilibrium (Bonnor-Ebert spheres) from collapsing cores (power-law regimes).

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

A Python‑based data manager for working with tabulated data from publications of observational surveys of cosmic magnetic fields.

Code used to galaxy protocluster analysis for Lacaille, K. et al., 2019, MNRAS

Analytic 1-D radiative transfer model of blue-asymmetric spectral line profiles from infalling molecular clouds. The model is presented in the paper, "Molecular Line Profile Fitting with Analytic Radiative Transfer Models" by De Vries & Myers (2005).

Set of scripts to calculate proper motions of for astronomical masers detected with VLBI.

My code for the Synthetic HR diagram project as a part of the VICO computational astrophysics research group

collection of analysis tools for accepted paper on streamer (Pineda et al., 2020)

Codes from my CASSUM project

Cecilia Bacchini's website

This a repo for the Bousso and Leichenauer model of Star Formation

Radio data and its analytical scripts for authored works studying radio emission from the ionised jets of young stellar objects

PHP code to calculate the total column density from a molecular rotational transition

Fit a modified black body (grey body) to mid-infrared astronomical data

Radiative transfer and synthetic radio imaging of ionised jets from young forming stars

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

Code to calculate the total column density from a molecular rotational transition