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bellalongo/README.md

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  1. spec2flux spec2flux Public

    Given a FITS spectrum file, the script will calculate the star’s doppler shift, and fit a Voigt profile and continuum to each emission line, which is used for calculating the flux.

    Python 1

  2. libra libra Public

    Finding the orbital periods and transits of white dwarf-main sequence binaries with TESS.

    Jupyter Notebook

  3. eider eider Public

    Empirically Informed Differential emission measure models for EUV Reconstruction (2)

  4. godwit-migrations godwit-migrations Public

    Through the use of the K Means algorithm, I prove that Marbled Godwits are among the many in the long list of animals affected by climate change by determining the minimum nighttime temperature nee…

    Jupyter Notebook