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.
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Updated
Nov 23, 2023 - Jupyter Notebook
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
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).
Pipeline which takes raw VLA data and yields science-ready data products, i.e. star formation rates
collection of analysis tools for accepted paper on streamer (Pineda et al., 2020)
Tool for astronomical data analysis, quantifying the structure of young star clusters using a fractal dimension.
RBH-1 reinterpreted as a gravitational soliton. Explains 650 km/s velocity with cold gas via metric shock, not thermal. Calibrated from GNSS data. Paper 8 of the TEP series.
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
Systematic comparison of galaxies in cosmic voids versus dense "walls" using DESI DR1 data to investigate environmental quenching mechanisms in galaxy evolution.
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
Cecilia Bacchini's website
My PhD thesis titled "Study of the effect of AGN activity on star formation in nearby galaxies using UVIT".
Lecture notes for astrophysics Interstellar Medium course
NEMESIS guided tour of young stellars objects for Stellarium
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