Tenenbaum et al (in prep) uses cuts on several statistics for each TCE, in order to filter out likely false positives. Here are the links to retrieve the final set of 7,959 TCEs that remain after this filtering using API queries:
1. All 7,959 TCEs
Click to run:
http://exoplanetarchive.ipac.caltech.edu/cgi-bin/nstedAPI/nph-nstedAPI?table=q1_q16_tce&format=ipac&where=%28tce_rsnrmes%3E0.6%20or%20tce_rsnrmes%20is%20null%29%20and%20%28tce_rmesmad%3E7.1%20and%20tce_rminmes%3C0.6%292. The 1,243 long-period (> 300 days) TCEs
Click to run:
http://exoplanetarchive.ipac.caltech.edu/cgi-bin/nstedAPI/nph-nstedAPI?table=q1_q16_tce&format=ipac&where=%28tce_rsnrmes%3E0.6%20or%20tce_rsnrmes%20is%20null%29%20and%20%28tce_rmesmad%3E7.1%20and%20tce_rminmes%3C0.6%29%20and%20tce_period%3E300To reproduce the same cuts in the interactive table, follow the instructions below. The criteria in Section 3.1 are to identify the likely false positives, and here we give the instructions to remove those targets from the TCE table. Also note that two different criteria are used for the SNR statistic, so two different stages of filtering are necessary.
This returns 7,566 TCEs.
This returns 393 TCEs.
Together, these two sets make up the 7,959 TCEs that will be examined to identify Kepler Objects of Interest.
Last updated: 31 October 2013