A Python package for forward asteroseismic modelling of gravity modes
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Updated
May 25, 2024 - Python
A Python package for forward asteroseismic modelling of gravity modes
A Python package for asteroseismic analyses of γ Doradus and Slowly Pulsating B stars.
Controller module for MESA (Modules for Experiments in Stellar Astrophysics). Create, modify and run MESA projects using python. Or even install MESA on Linux and macOS from scratch!
Modelling the imprint of mass transfer on asteroseismic signals in SPB stars - Wagg+2024
Simulate stellar oscillations and granulation with Gaussian processes 🌟
Interactive Python tool for browsing periodograms of g-mode pulsators, finding period-spacing patterns and creating échelle diagrams.
Pick a TIC number and obtain a reduced light curve for all TESS sectors available along with diagnostic plots about the reduction.
Tutorial given at the 2023 MESA Summer School on using MESA and GYRE for asteroseismology of early type star
automated measurements of global asteroseismic parameters
Celery is healthy
Newtonian and relativistic asteroseismology code for simple models of stars.
Add and remove an artificial buoyancy glitch from an existing AMDL stellar model
Public repository for Hall et al. (2019)
Fitting acoustic glitches in solar-like stars with emcee
This is an unofficial backup of SigSpec (abbreviation of `SIGnificance SPECtrum'), which is a program that computes a significance spectrum for a time series, developed by Piet Reegen.
Forward modelling of pulsating stars in binaries
Asteroseismic scaling relations for red giant branch stars
The K2 Halo Campaign Data Release and Paper
Kepler Smear Campaign Paper and Data
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