Codes used in a wide variety of astronomy/astrophysics
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Updated
Feb 1, 2019 - Python
Codes used in a wide variety of astronomy/astrophysics
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.
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).
Code used to galaxy protocluster analysis for Lacaille, K. et al., 2019, MNRAS
Set of scripts to calculate proper motions of for astronomical masers detected with VLBI.
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).
Tool for astronomical data analysis, quantifying the structure of young star clusters using a fractal dimension.
collection of analysis tools for accepted paper on streamer (Pineda et al., 2020)
Lecture notes for astrophysics Interstellar Medium course
This a repo for the Bousso and Leichenauer model of Star Formation
NEMESIS guided tour of young stellars objects for Stellarium
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)
PHP code to calculate the total column density from a molecular rotational transition
Cecilia Bacchini's website
Radio data and its analytical scripts for authored works studying radio emission from the ionised jets of young stellar objects
Code to calculate the total column density from a molecular rotational transition
Claculates the column density of interstellar molecular gas
Codes from my CASSUM project
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