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</p>
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<p align="center">
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<a href="https://travis-ci.com/rodluger/everest"><img src="https://travis-ci.com/rodluger/everest.svg?token=jABaFLLgJNHTWSqkT7CM&branch=master"/></a>
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<a href="https://github.com/rodluger/everest/blob/master/paper/tex/k2.pdf"><img src="http://staff.washington.edu/rodluger/paper_badge.svg"/></a>
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<a href="http://arxiv.org/abs/1607.00524"><img src="https://img.shields.io/badge/arXiv-1607.00524-blue.svg?style=flat"/></a>
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<a href="http://dx.doi.org/10.5281/zenodo.56577"><img src="https://zenodo.org/badge/doi/10.5281/zenodo.56577.svg" alt="10.5281/zenodo.56577"></a>
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<a href="https://raw.githubusercontent.com/rodluger/everest/master/LICENSE?token=AI5FKwMJER1BTPmm_2e_4VhVh3x3dfXHks5XfBCiwA%3D%3D"><img src="https://img.shields.io/badge/license-MIT-blue.svg"/></a>
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<b>E</b>PIC <b>V</b>ariability <b>E</b>xtraction and <b>R</b>emoval for <b>E</b>xoplanet <b>S</b>cience <b>T</b>argets: A pipeline for de-trending <b>K2</b> light curves with pixel level decorrelation and Gaussian processes. Here you'll find the Python code used to generate the <b>EVEREST</b> catalog, as well as tools for accessing and interacting with the de-trended light curves.</div>
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<b>Please read <a href="http://staff.washington.edu/rodluger/everest_docs">the documentation</a>! Note that the <a href="https://archive.stsci.edu/prepds/everest/">catalog</a> will be available on July 5, 2016.</b>
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<b>Please read <a href="http://staff.washington.edu/rodluger/everest_docs">the documentation</a>!</b>
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