The sky-projected distance between the center of the The orbital plane of the planet candidate. For the case of zero orbitalĮccentricity, the distance at mid-transit is the semi-major The distance between the planet and the star at mid-transitĭivided by the stellar radius. The planet radius divided by the stellar radius. The time corresponding to the center of the firstĭetected transit in Barycentric Julian Day (BJD). The time corresponding to the center of the first detected transit inīarycentric Julian Day (BJD) minus a constant offset of 2,454,833.0 days. The interval between consecutive planetary transits. Matrix covariances are adopted as errors to the fit parameters, they therefore ignore the effects of correlation between the fit parameters and are likely Planet-Star Radius Ratio, Planet-Star Separation and mpact Parameter are the free parameters in the fit. Limb darkening coefficients are fixed and pre-calculated from host star properties. Some of the parameters listed below are fit directly, other are derived from theīest-fit parameters. (2002) fit to a multi-quarter Kepler light curve, assuming a linear orbital ephemeris. Transit parameters delivered by the Kepler Project are typically best-fit parameters produced by a Mandel-Agol You must append the following URL to the file name in your wget query: This is the relative path for the data validation report You must append the following URL to the file name in your Use it when retrieving individual reports through the archive'sĪpplication programming interface with wget. This is the relative path for the data validation summary The TCE delivery name from the Kepler project. The intended detection criteria (i.e., tce_rogue_flag = 0)Īre considered for inclusion in the DR25 KOI activity tableĪnd reflected in the DR25 occurrence rate products. These rogue TCEs are excluded fromĪll subsequent analyses, so only the TCEs uniformly meeting 2016) as "rogue" (or unintended) detections In the DR25 pipeline run ( Twicken et al. Uniform manner, we have flagged 1498 of the 34032 TCEs identified To enforce this intended criterion and create valid TCEs in a Signals that fail the "three-transit weight check." In order The intent of the TPS algorithm was to fail "three-transit weight check" (see Section 2 of the DR25 windowįunction documentation, KSCI-19101) to become TCEs. Which inadvertently allowed a subset of signals that fail the This flag addresses a bug in DR25 and earlier versions of TPS, The Kepler ID is unique to a target and there is only one Kepler ID per target. The subset of 4 million targets found upon the Kepler CCDs can be searched via the Kepler Target Search form. Sources can be searched at the MAST archive. The survey's purpose was to identify stars for the Kepler exoplanet survey by magnitude and color. The KIC was derived from a ground-based imaging survey of the Kepler field conducted prior to launch. Target identification number, as listed in the Kepler Input Catalog (KIC). Target Labels and Flags Database Column Name
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