spacer link to MAST page spacer logo image spacer
MAST STScI
Tools
Tutorial Site Search

FAQ
Kepler Science Resource
Search & Retrieval
Documentation
Data Release Notes
Data Reduction &   Analysis
Related Sites
Publications/News
MAST Services
Images
Data Use Policy
Acknowledgments
 
link to STScI page


MAST/Kepler Condition Flag


The condition flag is a single, semi-colon separated string of phrases, in alphabetical order, describing various target categories and conditions known about a particular Kepler target. The table below provides information on each of the currently flagged conditions. Note that the table lists the total number of flagged targets on the detector, not the number of observations.

Searching on Condition Flags

The default form entry for the "Condition Flag" form element is "All Targets", which implies all entries will be returned including those with no listed condition (it is equivalent to ignoring the condition flag in the search query.) Selecting a specific condition from the form pull-down menu will return all entries containing that condition in the string, including those with multiple conditions.

You can also use the "user-specified field" form element to try more advanced condition flag searches. Note that if you use the user-specified field be sure the Condition Flag box entry is set to "All Targets", otherwise any other selected value will be included in the search.

  • To search for targets with condition "a" OR condition "b", use a comma to separate the conditions. For example, to retrieve targets which are false positives and targets which have Exoplanets, enter "False*,Exo*". (Note this technique works with all MAST search forms.)

  • To search for targets with condition "a" AND condition "b", use wildcard characters. For example, to search for targets which are flagged as both Eclipsing Binaries and having Exoplanets, enter "*Eclipsing*Exoplanet*. Although changes may occur in the future, the current list of multiple conditions includes:
    • Eclipsing_binary; Exoplanet
    • Eclipsing_binary; False_Positive
    • Eclipsing_binary; Possible_artifact
    • Eclipsing_binary; Red_giant
    • Eclipsing_binary; Planetary_candidate
    • Exoplanet; Planetary_candidate


Condition Definitions

Condition Flag # of Flagged Targets Description
 
Eclipsing_binary 2166 Target is listed in the Kepler eclipsing binary catalog v2.0, published on Oct 12, 2011 and derived from Kepler quarters 0-3. See the Eclipsing Binaries table for more information.
False_positive 492 Targets showing planetary transit-like features but which further analysis concluded was not attributable to a planet. The false positives are also shown in a separate table here.
Planetary_candidate 1790 A target exhibiting photometric features consistent with a transiting planet (but not necessarily confirmed), and published in Batalha et al., 2012. See the planetary candidates table for more information.
Exoplanet 29 A target confirmed to have 1 or more orbiting exoplanets based on information from the Kepler Discoveries web page. Note: this list may (temporarily) become out-of-date as new planets are discovered.
Red_giant 14,000 A possible red giant star for which data is now public. See the Red Giant Release page for more information.
Possible_artifact 36,000 A target believed to be flagged by the Kepler project as a possible artifact. These targets were identified by having row and column positions indicating they are on the detector, but the project did not provide distance to edge values. The distance values shown were added by MAST. They differ from the project-defined distances in that they represent the minimum distance from the detector edge to the target not (more accurately) from the detector edge to the edge of the photometric aperture. Note no targets considered "off" the detector were flagged as possible artifacts.
Null_kepmag 120,000 A target known to be on the detector but without a value for the Kepler magnitude. These were originally included in the target search interface, were later removed (July, 2011) by the Kepler project, then re-added by MAST with MAST-defined distance to edge values. As for the "possible_artifact" case, the MAST-defined distances describe the distance from the detector edge to the target, not from the detector edge to the edge of the photometric aperture. Most galaxies are included in this group.


Last Modified: Mar 08, 2012 11:31