Codes that I use for my astrophysics projects:
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BJDtoMJD: This code converts BJD time to MJD time and is specifically designed for converting TESS time (BJD) to Fermi time (MJD).
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ExploreCleanCorr: This script explores TESS data, especially focusing on weak signals. It cleans the data by removing negative flux values and calculates the correlation between signal data and background data.
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calVar: This code calculates flux variability using a custom-made model.
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fitUL: For a list of sources, this code identifies the best-fit model for estimating upper-limit flux values at different confidence levels.
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analyzeTimebin: Using the FermiPy package, this script models the flux of a source and measures its average flux. The accompanying Jupyter Notebook visualizes the data for a single time bin.
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FluxVariability: This script finds the correlation between flux and variability using data generated by the "analyzetimebin" code.