Code to estimate the Gravitational Wave Background sourced by extragalactic coalescing White Dwarf binaries.
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Updated
Jun 24, 2025 - Jupyter Notebook
Code to estimate the Gravitational Wave Background sourced by extragalactic coalescing White Dwarf binaries.
Newtonian and relativistic asteroseismology code for simple models of stars.
This repository contains excerpts from the programs made during the FRI summer fellowship and fall research in the “White Dwarfs” stream. “Kick_survial_final” and “WD_mass_loss” are our respective final programs, while the rest are functions and separate code snapshots that I contributed to or created.
A work on the Lane-Endem equation for stars applied to non-relativistic white dwarfs of polytropic index n=3/2.
Kinematical studies of white dwarfs populations
Bachelor in Science major project on astrophysics: analysis of properties of dust structure around WD
The term project of the Computational Physics (PHYS514) course. -- Koc University
Python numerical solvers for macroscopic anisotropic and microscopic Landau-quantized Super-Chandrasekhar white dwarfs.
Data and analysis pipeline for Chickles et al. 2026, ApJ — eclipsing 8.56-min mass-transferring binary.
ZTF white-dwarf photometry through the panelcast hierarchical panel-forecasting pipeline — an astronomy port with zero source changes
Finite temperature FMT EoS + TOV solver for single and multiple component white dwarfs
In-browser white-dwarf population simulator (Pyodide): interactive Gaia HR-diagram, no backend.
Injection-recovery audit of a Gaia XP white dwarf plus main-sequence binary catalog: does the BP-band calibration residual manufacture spurious binaries? Code for arXiv:2607.08856.
Some examples and notes on GWFish from LGWA Workshop
Equinox 2020 astrophysics project archive covering dark matter, pulsars and white dwarfs, with team reports, presentations and Jupyter-based data analysis collected as an early multi-topic astronomy research project.
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