.. include:: references.txt ******************************************************************** Cross-correlation analysis of high resolution spectroscopy (`Tayph`) ******************************************************************** Welcome to Tayph ================== The objective of **Tayph** is to provide a flexible, transparent tool for the analysis of high-resolution spectroscopic time-series observations of close-in exoplanets, using a cross-correlation technique similar to what was first implemented by `Snellen et al. (2010) `_, but translated to python and expanded upon over the course of multiple papers. (`Hoeijmakers et al. 2018 `_, `2019 `_, `2020 `_). The software is designed to be applied to transit observations of hot Jupiters made with echelle spectrographs at optical wavelengths. In particular, it can be applied to pipeline-reduced observations by HARPS, HARPS-N, ESPRESSO, CARMENES and to a certain extent UVES, with minimal interaction required. The software can also work on observations made with other instruments, provided that the user provides these according to a specific format (described below). Another feature is that the software can be used in conjunction with `Molecfit`_ (`Smette et al., 2015 `_) provided that the latter is properly installed. The software is presented as a Python 3 package, following the `Astropy`_ template. It is named Tayph, which is Arabic for Spectrum, and carries additional meanings of phantom, shining and glint or glimmer. This documentation is made using the `Astroplan`_ documentation as a template. Links ===== * `Source code `_ * `Docs `_ * `Issues `_ License: BSD-3 .. _tayph_docs: General Documentation ===================== .. toctree:: :maxdepth: 2 getting_started introduction workflow api .. _tayph_authors: Authors ======= Maintainers ----------- * Jens Hoeijmakers * Bibiana Prinoth Contributors ------------ * Jens Hoeijmakers * Bibiana Prinoth * Brett Morris * Nicholas Borsato * Brian Thorsbro