ZTF processed light curves

<strong><em>ZTF_all.csv</em></strong>: Catalog of the ~ 7 million ZTF periods measured <em>source_id</em>: gaia EDR3 source ID <em>Prot_all</em>: measured period from the entire light curve in days <em>Prot_1</em>: measured period from the first season light curve in days <em>Prot_2</em>: measured period from the second season light curve in days <em>Prot_3</em>: measured period from the third season light curve in days <em>Prot_4</em>: measured period from the fourth season light curve in days <em>maxpower_all</em>: normalized maximum LS power from the entire light curve <em>maxpower_1</em>: normalized maximum LS power from the first season light curve <em>maxpower_2</em>: normalized maximum LS power from the second season light curve <em>maxpower_3</em>: normalized maximum LS power from the third season light curve <em>maxpower_4</em>: normalized maximum LS power from the fourth season light curve <em>ra</em>: right ascension from gaia eDR3 in deg <em>dec</em>: declination from gaia eDR3 in deg <em>bprp</em>: bprp from gaia eDR3 <em>abs_G</em>: absolute magnitude from gaia eDR3 <em>parallax</em>: parallax from gaia eDR3 <em>ruwe</em>: ruwe number from gaia eDR3 <em><strong>source_id.csv</strong></em>: source_id to ztf file name <em>source_id</em>: gaia eDR3 source ID <em>filename</em>: file that contains the light curve associated with the source_id <em><strong>ZTFlc.zip</strong></em>: processed light curves Contain multiple .tgz files with processed light curves with the naming convention of &lt;source_id&gt;.pkl. One can use the source_id.csv file to find the .tgz file that contains the light curve with a specific gaia source_id. For each light curve pickle file, it contains the following columns: <em>lctime</em>: processed light curve times <em>lcmag</em>: processed normalized magnitudes <em>orglctime</em>: original light curve times <em>orglcmag</em>: original light curve magnitudes pandas version used to save the .pkl files: 1.4.2