When a Period Is Not a Full Stop: Light Curve Structure Reveals Fundamental Parameters of Cepheid and RR Lyrae Stars
Non Uniform Discrete Fourier Transform applied to OGLE-III Type 1 Cepheid photometry database.
The ResonanceChecker program was written to check for resonances between modal oscillations from linear MESA RSP output up to the ninth overtone. The code is a work in progress as the project is still being worked on. PlotterProgram was written to take "Fig4" output from ResonanceChecker and recreate the plot that can be seen in Figure 4 within …
The Cepheid Bias: Resolving the Hubble Tension — Environment-dependent Cepheid clock bias under TEP. Generative clock-aware model across 37 SH0ES hosts yields H0 = 66.65 ± 1.58 km/s/Mpc, consistent with Planck at 0.45σ. M31 and OGLE-IV differential tests confirm the predicted sign.
GEOS data for the O-C of the Classical Cepheid RT Aur (GEOS CIRCULAR CEP4)
Python project to find pulsation period of a cepheid star
Non Uniform Discrete Fourier Transform applied to OGLE-III Type 1 Cepheid photometry database.
Explore a newly developed methodology that could allow us to determine the pulsation and orbit periods of binary Cepheids without using any prior knowledge.
InstabilityStrip is a C++ program written to analyze linear data from MESA's RSP and study variable star's instability strips. Originally called BlueEdge_Plotter as this was the first function the program was fitted for.
Add a description, image, and links to the cepheids topic page so that developers can more easily learn about it.
To associate your repository with the cepheids topic, visit your repo's landing page and select "manage topics."