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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