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    "info": {
        "author": "Moises Castillo",
        "author_email": "castillo.moises11@gmail.com",
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        "description": "[![Documentation Status](https://readthedocs.org/projects/lightcurator/badge/?version=latest)](https://lightcurator.readthedocs.io/en/latest/?badge=latest)\n[![DOI](https://zenodo.org/badge/124146048.svg)](https://zenodo.org/badge/latestdoi/124146048)\n\n\n# LightCurve\n\nLightCurve is a module that creates light curves of a similar field of stars.\nThis is useful in time domain astronomy in search of transient events\nand studies of variable stars, i.e. eclipsing binaries.\n\n\n# Table of Contents\n\n# Installation\n\n# Usage\n\n```\nfrom lightcurator import lightcurves as lc\n\nobject_table = lc.makelist('')\n\n# parallelized alignment\nobject_table = lc.paralign(object_table)\n\n# or serial alignment\nobject_table = lc.align(object_table)\n\n# All-in-one\nobject_table = lc.do_lightcurve(object_table)\n```\n\nThe process follows:\n1. Take image list\n2. Align images\n3. Create a deepsky image\n4. Plate solve deepsky using `astrometery`\n5. Sorce extraction from deepsky image\n6. Create **reference image** with all candidate sources circled\n7. Match sources between aligned images\n8. Cross match sources from aligned images with sources from deepsky image\n9. Create Timeseries **plot** of different sources\n10. Cross match sources with catalogs like VSX and GCVS \n\n\n# Credits\n\n# License\n\n\n\n",
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        "license": "MIT License",
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        "name": "lightcurator",
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        "summary": "Creates a lightcurve database of series of images.",
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