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
A Python‐based data manager for working with tabulated data from publications of observational surveys of cosmic magnetic fields.
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 runaway black hole as Temporal Topology soliton candidate. Explains 650 km/s velocity discontinuity with cold gas via metric shock. TEP calibration: R_×ばつ107 km from GNSS. Alternative to shock physics cooling problem
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.
My code for the Synthetic HR diagram project as a part of the VICO computational astrophysics research group
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).
Systematic comparison of galaxies in cosmic voids versus dense "walls" using DESI DR1 data to investigate environmental quenching mechanisms in galaxy evolution.
Quantifying the recoverable variance in star formation rate from 1.4 GHz radio continuum emission using VLA-COSMOS and MeerKAT data.
Lecture notes for astrophysics Interstellar Medium course
NEMESIS guided tour of young stellars objects for Stellarium
Cecilia Bacchini's website
PHP code to calculate the total column density from a molecular rotational transition
Codes from my CASSUM project
Bousso and Leichenauer model of Star Formation
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