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User Specified Search Field
You may search on any column listed below. Where reasonable, the table lists the range of valid values or a set of sample values. A description of the column is also given. Note the column "label" is the name displayed on the search forms and in search results. The column "name" is the actual column name in the table and needs to be specified in GET requests.
From a MAST search form, simply select the column "label" in the forms pulldown menu and type in the qualification in the adjacent box. Note that if you specify constraints on the same column in more than one form element, they will all be included in the query and you may not get results you expect. In a HTTP GET request, specify the column "name" in the service request. (See the MAST Services web page for information on sumbitting GET requests.)
| Column Name | Column Label | Description | Examples/Valid Values | Data Type |
|---|---|---|---|---|
| masterID | Master ID | A unique ID for all targets in table comprised of a catalog-designated name, followed by "-catalog" where catalog is a catalog designation such as "Kepler", "USNOb", or "IRT". | example: 10937527-Kepler, 1267-0342530-USNOb, 44117904398771-IRT | char |
| masterRA | RA (J2000) | Right Ascension (J2000) in decimal degrees for all targets (not just KIC targets). | range: 279.21 to 302.31 degrees | double |
| masterDec | Dec (J2000) | Declination (J2000) in decimal degrees for all targets (not just KIC targets). | range: 36.3 to 52.78 degrees | double |
| kic_kepler_id | Kepler_ID | Unique Kepler ID. Also used in Kepler Target Catalog and in naming data files. Note there are 4,374,730 entries in the KIC_CT joined table | range: 482,490 to 13,129,811 | long |
| twomass_2mass_id | 2MASS ID | 2MASS catalog ID, a sexagesimal, equatorial position-based source name in the form: hhmmssss+ddmmsss[ABC...] (Note this entry was added by MAST, and was not included in the KIC). | example: 19045085+3723043 | char |
| twomass_tmid | 2MASS designation | A unique identification number which was defined during final processing to identify a 2Mass catalog entry. The unique identification number is referred to as pts_key/cntr. See the User's Guide to the 2Mass All Sky Data Release, at http://www.ipac.caltech.edu/2mass/releases/allsky/doc/explsup.html for information on the pts_key/cntr field. | range: 79224945 to 1305757552 | long |
| twomass_conflictflag | twoMass conflict flag | Describes difference (if any) between 2MASS values derived by MAST staff and the original KIC 2MASS entries. (See the KIC table to find the original uncorrected values.) | Conditions currently flagged include: null - KIC '2MASS ID' contained a null entry and MAST could not find a match, 0 - KIC non-null value agreed with value found by MAST, 1 - a new entry replaced a null KIC entry, 2 - a null entry replaced a KIC non-null entry, 3 - a new non-null entry replaced a non-null KIC entry. See the 2mass notes for more information. | char |
| kic_degree_ra | KIC RA (J2000) | Right Ascension (J2000) in decimal degrees from KIC. All but roughly 36,000 photometric standards, are within the Kepler FOV. | range: 279.21 to 302.31 degrees | double |
| kic_dec | KIC Dec (J2000) | Declination (J2000) in decimal degrees from KIC. All but roughly 36,000 photometric standards, are within the Kepler FOV. | range: 36.3 to 52.78 degrees | double |
| kct_avail_flag | Data Availability Flag | Data availability flag. 0 = not observed or planned to be observed, 1 = target is either planned to be observed or has been observed but data has not yet been archived, and 2 = data for the particular target has been archived. The flag values will be updated quarterly. | 0, 1 or 2 | long |
| kct_num_season_onccd | Seasons_on_CCD | Number of seasons a target is on the detector. For targets with a known Kepler magnitude, this represents the number of seasons with a distance of 0 or greater. For KIC targets with unknown Kepler magnitudes and non-KIC targets, this is based on the number of seasons with MAST-derived distances (described below) greater than zero. | range 0 to 4. A 0 value indicates a non-observable target and by default are not displayed from the MAST target search interface. (Note: to see the non-observable entries from the MAST target search page, set "Season's on CCD" to "unspecified".) | long |
| kic_pmra | RA_PM (arcsec/yr) | RA proper motion (KIC targets only) | range: -8.36 to 8.04 arcsec/yr | float |
| kic_pmdec | Dec_PM (arcsec/yr) | Dec proper motion (KIC targets only) | range: -7.2 to 8.848 arcsec/yr | float |
| kic_scpid | SCP_ID | SCP processing ID (KIC targets only) | range: 79226018 to 1305757552 | long |
| kic_altid | Alt_ID | ID from alternate source catalog (see Alt ID Source entry) (KIC targets only) | range: -1224784 to 1065212930 | long |
| kic_altsource | Alt_ID_Source | Source catalog that was used for deriving stellar parameters (KIC targets only) | 0 - null, 1 - Hipparcos catalog ID, 2 - Tycho2 ID, 3 - UCAC2 ID, 4 - General Catalog of Var. Stars ID, 5 - Lepine proper motion catalog star. altid>0 is 2MASS ID, altid< 0 is a pseudo-id generated by SCP processing, 6 - altid contains 2MASS ID coming from Astroseiseismology catalog, 11 - NED ID, 12 - Extended 2MASS ID, 13 - FIRST ID, 14 - NVSS catalog ID, 15 - VLBA catalog ID, 16 - CHANDRA catalog ID | long |
| kic_galaxy | Star/Gal_ID | A flag where 0 = star and 1 = galaxy. The original USNO-B catalog codes these with 11 values, depending on the degree that measured image profile was consistent with a point source. The USNO-B codes were star = 6-11 and galaxy = 0-5. (KIC targets only) | 1? = USNO-B values 0 to 5 (i.e., a galaxy), 0? = values 6 to 11 (i.e., a star). The values 0 - 11 were a measure of the similarity between a given image to a stellar point spread function. 0 is quite dissimilar, 11 means quite similar. | long |
| kic_blend | Isolated/Blend_ID | Isolated/blended indicator (never used) | Not yet (and may never be) determined. All values are null. | long |
| kic_variable | Var._ID | Constant/variable indicator based on data from the General Catalog of Variable Stars. (Additional catalogs will be used in future versions.) (KIC targets only) | 0 - constant, 1 - variable | long |
| kic_teff | Teff | Derived Effective Temperature accurate to 200 K (KIC targets only) | range: 3105 to 19337 degrees K | long |
| kic_logg | Log_G | Derived Log10 surface gravity accurate to 0.5 dex (KIC targets only) | range: -0.44 to 6.16 | float |
| kic_feh | Metallicity (solar=0.0) | Derived Log10 Fe/H metallicity accurate to 0.5 dex. (KIC targets only) | range: -2.59 to 0.62 | float |
| kic_ebminusv | E(B-V) | Derived Excess B-V reddening accurate to 0.1 magnitude (KIC targets only) | range: 0.001 to 0.494 | float |
| kic_av | A_V | Derived A-V extinction (KIC targets only) | range: 0.003 to 1.53 | float |
| kic_radius | Radius (solar=1.0) | Estimated Stellar Radius (solar = 1.0) (KIC targets only) | range: 0.097 to 316.30 | float |
| kic_cq | Kepmag_Source | Source of Kepler-band magnitude. (KIC targets only) | SCP, NOCAL, 2MASS, UNCAL, PHOTO, TYBV SCP - SCP values for sdssg and sdssr were used to compute KEPMAG using equation below . The error for KEPMAG is roughly 0.03 mag., NOCAL - No calibration to optical mag. possible, used for entries from non-optical catalogs. KEPMAG field is null. , 2MASS - Objects found only in 2MASS Catalog with no optical counterpart, KEPMAG is null, UNCAL - KEPMAG copied from a single color of the parent catalog, uncertainty could be 1.0 mag or higher, PHOTO - parent catalog contained a red and blue mag. obtained from Photographic photometry. Values used to compute KEPMAG on the basis of: sdssg=blue sdssr=red color=sdssg-sdssr if (color<=0.8) kepmag = 0.8*sdssr + 0.2*sdssg else kepmag = 0.9*sdssr+0.1*sdssg, internal photographic errors have errors of 0.2 mag suggest KEPMAG errors of 0.03 mag, TYBV - parent catalog is Tycho-2 and this gives B and V magnitudes. KEPMAG value computed from sdssg=0.54*b+0.46*v-0.07 sdssr=-0.44*b+1.44*v+0.12 using same transformation as above to calc. KEPMAG. Errors same as for TYCHO-2 catalog. | char |
| kic_pq | Photometry_Qual | Photometry quality indicator. (KIC targets only) | range: Integer from 0 to 8 which is the count of non-null entries in USNO-B1.0 (O,E,J,F,N), UCAC-2 (R), TYcho-2 (B,V). In general the more colors the more likely the star is real. For NOCAL and 2MASS entries, this value = 0. Stars with low values (e.g., < 3) may not be real and should be verified by other means. | long |
| kic_aq | Astrophysics_Qual | Astrophysics quality indicator. Placeholder for SCP values not yet determined. (KIC targets only) | range: currently 0 to 6 which is the count of all non-null entries in Teff, logG, FeH, AV, E(B-V), and Radius. | long |
| kic_catkey | Catalog_key | Unique integer key to CATKEY database table (not currently available). (KIC targets only) | range: 311150 to 12958186 | long |
| kic_scpkey | Scp_Key | Unique integer key to SCPKEY database table (not currently available). (KIC targets only) | range: 262005541 to 1305757193 | long |
| kic_parallax | Parallax (arcsec) | Parallax in arcsec (KIC targets only) | range: -0.0297 to 0.028 arcsec | float |
| kic_glon | Gal_Lon (deg) | Galactic Longitude (KIC targets only) | range: 67.76 to 84.85 degrees | float |
| kic_glat | Gal_Lat (deg) | Galactic Latitude (KIC targets only) | range: 5.17 to 21.75 degrees | float |
| kic_pmtotal | Total_PM (arcsec/yr) | Total proper motion accurate to 20 mas/yr (KIC targets only) | range: 0.0 to 9.30 arcsec/yr | float |
| kic_ra | RA_hours (J2000) | Right Ascension (J2000) in decimal hours (KIC targets only) | range: 18.61 to 20.15 hours | float |
| u | u | u-band Sloan magnitude from the Kepler Input Catalog accurate to 0.04 magnitude | range: 10.23 to 20.96 | float |
| g | g | g-band Sloan magnitude from the Kepler Input Catalog | range: 4.84 to 23.73 | float |
| r | r | r-band Sloan magnitude from the Kepler Input Catalog | range: 4.50 to 24.99 | float |
| i | i | i-band Sloan magnitude from the Kepler Input Catalog | range: 5.66 to 25.18 | float |
| z | z | z-band Sloan magnitude accurate to 0.03 magnitude from the Kepler Input Catalog | range: 5.31 to 19.42 | float |
| gred | gred | GRed-band Sloan magnitude from the Kepler Input Catalog | range: 8.52 to 19.01 | float |
| d51mag | d51mag | D51 magnitude from the Kepler Input Catalog | range: 7.02 to 19.85 | float |
| J | J | 2MASS J-band magnitude. . In some cases KIC values were replaced with values based on cross-correlations performed by MAST. (See 2mass_conflict_flag). | range: 1.07 to 19.87 | float |
| H | H | 2MASS H-band magnitude. In some cases KIC values were replaced with values based on cross-correlations performed by MAST. (See 2mass_conflict_flag). | range: 0.01 to 20.52 | float |
| K | K | 2MASS K-band magnitude. In some cases KIC values were replaced with values based on cross-correlations performed by MAST. (See 2mass_conflict_flag). | range: 0.001 to 18.59. | float |
| kepmag | kepmag | A magnitude computed according to a hierarchical scheme and depends on what pre-existing catalog source is available, SCP, Tycho 2, or photographic photometry, in order of preferred selection. For SCP stars the magnitude is synthesized from the Sloan-like g and r magnitudes according to the following prescription: if one defines 'color' as g - r, then for color less than or equal to 0.8 kepmag = 0.8r + 0.2g, while for color greater than 0.8 kepmag = 0.9r + 0.1g. Empirical measurements for presumed constant stars suggest that the r.m.s. for this quantity is slightly larger 0.02 mags. except for very faint and bright stars. | range: 4.49 to 24.99 | float |
| FUV | GALEX FUV | Galex Far-UV magnitude. | range: 11.2 to 24.9 | float |
| NUV | GALEX NUV | Galex Near-UV magnitude. | range: 11.85 to 26.30 | float |
| ID_USNO | ID_USNO | USNO ID | example: 1368-0331648 | char |
| ra_USNO | ra_USNO | USNO Right Ascension in decimal degrees | range: 279.62 to 301.84, although values are stored in decimal degrees, valid formats for queries include: "19 28 29.65", "19h28m29s", 292.12354 | float |
| dec_USNO | dec_USNO | USNO Declination in decimal degrees | range: 36.52 to 52.40, stored in decimal degrees but can be queried using values such as: "+37 14 04.5", "37.23458" | float |
| ID_GALEX | ID_GALEX | GALEX ID | example: 6371197300258117766 | char |
| ra_GALEX | ra_GALEX | GALEX Right Ascension in decimal degrees | range: 279.63 to 300.10, although values are stored in decimal degrees, valid formats for queries include: "19 28 29.65", "19h28m29s", 292.12354 | float |
| dec_GALEX | dec_GALEX | GALEX Declination in decimal degrees | range: 36.61 to 51.42, stored in decimal degrees but can be queried using values such as: "+37 14 04.5", "37.23458" | float |
| ra_2M | 2MASS RA (J2000) | Right Ascension (J2000) in decimal degrees from 2MASS. All but roughly 36,000 photometric standards, are within the Kepler FOV. | range: 279.21 to 302.31 degrees | double |
| dec_2M | 2MASS Dec (J2000) | Declination (J2000) in decimal degrees from 2MASS. All but roughly 36,000 photometric standards, are within the Kepler FOV. | range: 36.3 to 52.72 degrees | double |
| ID_IRT | ID_IRT | WFCAM Science Archive designation | range:44117904093025 to 44117921991257 | long |
| ra_IRT | ra_IRT | UKIRT/WFCAM Right Ascension in decimal degrees | range: 279.57 to 301.31, although values are stored in decimal degrees, valid formats for queries include: "19 28 29.65", "19h28m29s", 292.12354 | float |
| dec_IRT | dec_IRT | UKIRT/WFCAM Declination in decimal degrees | range: 36.49 to 52.72, stored in decimal degrees but can be queried using values such as: "+37 14 04.5", "37.23458" | float |
| pStar_IRT | pStar_IRT | image-profile-based probability that the source is a star (where 1.0 = a stellar source). | range: 0.003 to 0.994 | float |
| J_IRT | J_IRT | J band magnitude in a 2 arcsec diameter aperture on the WFCAM MKO (Vega based) system. This is the default UKIRT magnitude to use for stars. The photometric pipeline provides a maximum likelihood estimate in cases where apertures around multiple sources overlap | range: 9.14 to 33.08 | float |
| JErr_IRT | JErr_IRT | Error in J_IRT (in magnitudes?). Anything fainter than J=20 mag is almost certainly bogus. | range: 0.0002 to 59280.9? | float |
| jClass_IRT | jClass_IRT | Discrete Image classification flag. -2 = probably a star (ii.e., 70-90% probability), -1 = star (greater than 90% probability), 0 = noise, +1 = extended source | range: integers from -2 to 1 | long |
| jppErrBits_IRT | jppErrBits_IRT | Error bits information relating to reliability of photometry. The number ranges from 0 to 2**32 -1 The flags are ranked in order of severity and are given in . Our Color Table restricts entries to those with severity flag values less than 256. See http://horus.roe.ac.uk/vsa/www/gloss_j.html | range: 0 to 80 | long |
| Sep_IRT | Sep_IRT | Spatial separation of KIC coordinates from UKIRT/WFCAM coordinates in arcsec. | range: 0 to 1.05 | float |
| gr | gr | kic_gmag - kic_rmag color | range: -10.31 to 10.43 | float |
| gi | gi | kic_gmag - kic_imag color | range: -9.59 to 12.2 | float |
| iz | iz | kic_imag - kic_zmag color | range: -1.60 to 2.35 | float |
| gK | gK | kic_gmag - 2mass_Kmag color | range: -6.67 to 14.85 | float |
| JH | JH | 2mass_jmag - 2mass_hmag color | range: -5.17 to 10.54 | float |
| HK | HK | 2mass_hmag - 2mass_kmag color | range: -8.56 to 7.40 | float |
| JK | JK | 2mass_jmag - 2mass_kmag color | range: -4.24 to 8.21 | float |
| gJ | gJ | kic_gmag - 2mass_jmag color | range: -7.26 to 12.83 | float |
| FUVNUV | GALEX FUVNUV | galexFUV - galexNUV | range: -4.12 to 7.90 | float |
| NUVg | NUVg | galexNUV - kic_gmag color | range: -4.42 to 11.34 | float |
| gJ_KIC_IRT | gJ_KIC_IRT | kic_gmag - IRT_J color | range: -8.71 to 9.46 | float |
| kct_sky_group_id | Skygroup_ID | An integer value from 1 to 84 describing the module/channel where the target falls. It's equivalent to the channel number during season 2. The sky group is an integer that groups stars together on the sky depending on which channel they fall on (or near) during season 2. Due to slight asymmetries in the CCD array layout, positions are not perfectly maintained upon seasonal rotation of the spacecraft. Therefore, there are objects that fall off silicon during season 2 but are on silicon in subsequent seasons. This is especially problematic for Module 13 due to the center gap. Such stars are assigned the sky group corresponding to the other stars that fall on the same channel during other seasons. (KIC targets only) | range: 1 - 84 | long |
| kct_crowding_season_0 | Crowding season 0 | A floating point number between 0 and 1 representing the fraction of light in the aperture due to the target star for season N. A value of 1 means all the light is from the target while a value of 0.5 means half of the light through the aperture is due to the target. (KIC targets only) | range: 8e-05 to 0.999 | float |
| kct_crowding_season_1 | Crowding season 1 | A floating point number between 0 and 1 representing the fraction of light in the aperture due to the target star for season 1. A value of 1 means all the light is from the target while a value of 0.5 means half of the light through the aperture is due to the target. (KIC targets only) | range: 2e-05 to 0.999 | float |
| kct_crowding_season_2 | Crowding season 2 | A floating point number between 0 and 1 representing the fraction of light in the aperture due to the target star for season 2. A value of 1 means all the light is from the target while a value of 0.5 means half of the light through the aperture is due to the target. (KIC targets only) | range: 1e-04 to 0.999 | float |
| kct_crowding_season_3 | Crowding season 3 | A floating point number between 0 and 1 representing the fraction of light in the aperture due to the target star for season 3. A value of 1 means all the light is from the target while a value of 0.5 means half of the light through the aperture is due to the target. (KIC targets only) | range: 8.4e-05 to 0.999 | float |
| kct_contamination_season_0 | Contamination season 0 | Measure of light contamination defined as 1 - crowding value. A value of 0 implies no contamination, 1 implies all background. (KIC targets only) | range 0.001 - 0.999 | float |
| kct_contamination_season_1 | Contamination season 1 | Measure of light contamination defined as 1 - crowding value. A value of 0 implies no contamination, 1 implies all background. (KIC targets only) | range 0.001 - 0.999 | float |
| kct_contamination_season_2 | Contamination season 2 | Measure of light contamination defined as 1 - crowding value. A value of 0 implies no contamination, 1 implies all background. (KIC targets only) | range 0.001 - 0.999 | float |
| kct_contamination_season_3 | Contamination season 3 | Measure of light contamination defined as 1 - crowding value. A value of 0 implies no contamination, 1 implies all background. (KIC targets only) | range 9e-04 - 0.999 | float |
| kct_flux_fraction_in_aperture_season_0 | Flux Fraction season 0 | The fraction of target flux that falls within the photometric aperture. A value of 1 means all the flux from the target falls within the aperture, while a value of 0 means no flux from the target falls within the photometric aperture. (KIC targets only) | range 0.106 - 0.999 | float |
| kct_flux_fraction_in_aperture_season_1 | Flux Fraction season 1 | The fraction of target flux that falls within the photometric aperture. A value of 1 means all the flux from the target falls within the aperture, while a value of 0 means no flux from the target falls within the photometric aperture. (KIC targets only) | range 0.104 to 0.999 | float |
| kct_flux_fraction_in_aperture_season_2 | Flux Fraction season 2 | The fraction of target flux that falls within the photometric aperture. A value of 1 means all the flux from the target falls within the aperture, while a value of 0 means no flux from the target falls within the photometric aperture. (KIC targets only) | range 0.087 to 0.999 | float |
| kct_flux_fraction_in_aperture_season_3 | Flux Fraction season 3 | The fraction of target flux that falls within the photometric aperture. A value of 1 means all the flux from the target falls within the aperture, while a value of 0 means no flux from the target falls within the photometric aperture. (KIC targets only) | range 0.103 to 0.999 | float |
| kct_snr_season_0 | SNR season 0 | The ratio of target flux collected within the photometric aperture to the statistical 1-sigma uncertainty in the collected target flux. (KIC targets only) | range 0.04 to 608602 | float |
| kct_snr_season_1 | SNR season 1 | The ratio of target flux collected within the photometric aperture to the statistical 1-sigma uncertainty in the collected target flux. (KIC targets only) | range 0.03 to 607510 | float |
| kct_snr_season_2 | SNR season 2 | The ratio of target flux collected within the photometric aperture to the statistical 1-sigma uncertainty in the collected target flux. (KIC targets only) | range 0.04 to 607071 | float |
| kct_snr_season_3 | SNR season 3 | The ratio of target flux collected within the photometric aperture to the statistical 1-sigma uncertainty in the collected target flux. (KIC targets only) | range 0.05 to 606119 | float |
| kct_distance_0 | Edge_Distance_0 (px) | The shortest distance from the edge of the CCD to a pixel in the photometric aperture for season 0. Values of 0 or greater are observable. For KIC targets with undefined Kepler magnitudes, the distance represents the distance in pixels from the nearest edge to the target (i.e., not to the photometric aperture). For non-KIC targets, the distance is the closest possible distance from the target to the edge with a maximum absolute uncertainty of 22 pixels (i.e., the target could be up to 22 pixels farther from, but not closer to, the edge). Non-KIC targets calculated to be less than 5 pixels from the edge were excluded. | range 0 to 511 and null | long |
| kct_distance_1 | Edge_Distance_1 (px) | The shortest distance from the edge of the CCD to a pixel in the photometric aperture for season 1. Values of 0 or greater are observable. For targets with undefined Kepler magnitudes, the distance represents the distance in pixels from the nearest edge to the target (i.e., not to the photometric aperture). For non-KIC targets, the distance is the closest possible distance from the target to the edge with a maximum absolute uncertainty of 22 pixels (i.e., the target could be up to 22 pixels farther from, but not closer to, the edge). Non-KIC targets calculated to be less than 5 pixels from the edge were excluded. | range 0 to 511 and null | long |
| kct_distance_2 | Edge_Distance_2 (px) | The shortest distance from the edge of the CCD to a pixel in the photometric aperture for season 2. Values of 0 or greater are observable. For targets with undefined Kepler magnitudes, the distance represents the distance in pixels from the nearest edge to the target (i.e., not to the photometric aperture). For non-KIC targets, the distance is the closest possible distance from the target to the edge with a maximum absolute uncertainty of 22 pixels (i.e., the target could be up to 22 pixels farther from, but not closer to, the edge). Non-KIC targets calculated to be less than 5 pixels from the edge were excluded. | range 0 to 511 and null | long |
| kct_distance_3 | Edge_Distance_3 (px) | The shortest distance from the edge of the CCD to a pixel in the photometric aperture for season 3. Values of 0 or greater are observable. For targets with undefined Kepler magnitudes, the distance represents the distance in pixels from the nearest edge to the target (i.e., not to the photometric aperture). For non-KIC targets, the distance is the closest possible distance from the target to the edge with a maximum absolute uncertainty of 22 pixels (i.e., the target could be up to 22 pixels farther from, but not closer to, the edge). Non-KIC targets calculated to be less than 5 pixels from the edge were excluded. | range 0 to 511 and null | long |
| kct_channel_season_0 | Channel_0 | Integer channel number for season 0. There are 21 modules, each with 4 outputs for a total of 84 channels. CHANNEL is an integer ranging from 1 to 84 that uniquely specifies the MODULE/OUTPUT pair. An object can have a non-zero channel number if it is off, but near, a CCD. Such cases can be identified by examining the expected ROW and COLUMN values for a specified season. (KIC targets only) | range: 1 to 84 | long |
| kct_module_season_0 | Module_0 | Integer module number for season 0. A module refers to a pair of CCDs that share a field flattener and are read out simultaneously by the detector electronics. There are 21 modules on the focal plane. MODULE is an integer from the set [2-4,6-20,22-24]. An object can have a non-zero module number if it is off, but near, a CCD. Such cases can be identified by examining the expected ROW and COLUMN values for a specified season. (KIC targets only) | 2-4,6-20,22-24 | long |
| kct_output_season_0 | Output_0 | Each module has four output channels (two per CCD). Each output is read out by a unique analog signal chain (e.g. amplifier). OUTPUT is an integer ranging from 1 to 4. An object can have a non-zero output number if it is off, but near, a CCD. Such cases can be identified by examining the expected ROW and COLUMN values for a specified season. (KIC targets only) | range 1 to 4 | long |
| kct_row_season_0 | Row_0 | Row number for season 0 with values ranging from -232 to 1098. Each channel has 1132 columns and 1070 rows. There are 1024 science rows enumerated as rows 20 through 1043. Collateral data is enumerated as rows 0 through 19 and 1044 through 1069. Values outside 0 through 1069 are enumerated in order to provide information about how far off a target is from the CCD channel. (KIC targets only) | range -227 to 1094 | long |
| kct_column_season_0 | Column_0 | Column number for season 0 defined like the Row values. Each channel has 1132 columns. There are 1100 science channels described as columns 12 - 1111. Collateral values range from 0-11 and 1112-1131. Other values ranging from -205 to -1 describe how far a target is from the CCD channel. (KIC targets only) | range -203 to 1111 | long |
| kct_channel_season_1 | Channel_1 | Integer channel number for season 1. There are 21 modules, each with 4 outputs for a total of 84 channels. CHANNEL is an integer ranging from 1 to 84 that uniquely specifies the MODULE/OUTPUT pair. An object can have a non-zero channel number if it is off, but near, a CCD. Such cases can be identified by examining the expected ROW and COLUMN values for a specified season. (KIC targets only) | range: 1 to 84 | long |
| kct_module_season_1 | Module_1 | Integer module number for season 1. A module refers to a pair of CCDs that share a field flattener and are read out simultaneously by the detector electronics. There are 21 modules on the focal plane. MODULE is an integer from the set [2-4,6-20,22-24]. An object can have a non-zero module number if it is off, but near, a CCD. Such cases can be identified by examining the expected ROW and COLUMN values for a specified season. (KIC targets only) | 2-4,6-20,22-24 | long |
| kct_output_season_1 | Output_1 | Each module has four output channels (two per CCD). Each output is read out by a unique analog signal chain (e.g. amplifier). OUTPUT is an integer ranging from 1 to 4. An object can have a non-zero output number if it is off, but near, a CCD. Such cases can be identified by examining the expected ROW and COLUMN values for a specified season. (KIC targets only) | range 1 to 4 | long |
| kct_row_season_1 | Row_1 | Row number for season 1 with values ranging from -232 to 1098. Each channel has 1132 columns and 1070 rows. There are 1024 science rows enumerated as rows 20 through 1043. Collateral data is enumerated as rows 0 through 19 and 1044 through 1069. Values outside 0 through 1069 are enumerated in order to provide information about how far off a target is from the CCD channel. (KIC targets only) | range -229 to 1043 | long |
| kct_column_season_1 | Column_1 | Column number for season 1 defined like the Row values. Each channel has 1132 columns. There are 1100 science channels described as columns 12 - 1111. Collateral values range from 0-11 and 1112-1131. Other values ranging from -205 to -1 describe how far a target is from the CCD channel. (KIC targets only) | range -204 to 1111 | long |
| kct_channel_season_2 | Channel_2 | Integer channel number for season 2. There are 21 modules, each with 4 outputs for a total of 84 channels. CHANNEL is an integer ranging from 1 to 84 that uniquely specifies the MODULE/OUTPUT pair. An object can have a non-zero channel number if it is off, but near, a CCD. Such cases can be identified by examining the expected ROW and COLUMN values for a specified season. (KIC targets only) | range: 1 to 84 | long |
| kct_module_season_2 | Module_2 | Integer module number for season 2. A module refers to a pair of CCDs that share a field flattener and are read out simultaneously by the detector electronics. There are 21 modules on the focal plane. MODULE is an integer from the set [2-4,6-20,22-24]. An object can have a non-zero module number if it is off, but near, a CCD. Such cases can be identified by examining the expected ROW and COLUMN values for a specified season. (KIC targets only) | 2-4,6-20,22-24 | long |
| kct_output_season_2 | Output_2 | Each module has four output channels (two per CCD). Each output is read out by a unique analog signal chain (e.g. amplifier). OUTPUT is an integer ranging from 1 to 4. An object can have a non-zero output number if it is off, but near, a CCD. Such cases can be identified by examining the expected ROW and COLUMN values for a specified season. (KIC targets only) | range 1 to 4 | long |
| kct_row_season_2 | Row_2 | Row number for season 2 with values ranging from -232 to 1098. Each channel has 1132 columns and 1070 rows. There are 1024 science rows enumerated as rows 20 through 1043. Collateral data is enumerated as rows 0 through 19 and 1044 through 1069. Values outside 0 through 1069 are enumerated in order to provide information about how far off a target is from the CCD channel. (KIC targets only) | range -223 to 1092 | long |
| kct_column_season_2 | Column_2 | Column number for season 2 defined like the Row values. Each channel has 1132 columns. There are 1100 science channels described as columns 12 - 1111. Collateral values range from 0-11 and 1112-1131. Other values ranging from -205 to -1 describe how far a target is from the CCD channel. (KIC targets only) | range -200 to 1111 | long |
| kct_channel_season_3 | Channel_3 | Integer channel number for season 3. There are 21 modules, each with 4 outputs for a total of 84 channels. CHANNEL is an integer ranging from 1 to 84 that uniquely specifies the MODULE/OUTPUT pair. An object can have a non-zero channel number if it is off, but near, a CCD. Such cases can be identified by examining the expected ROW and COLUMN values for a specified season. (KIC targets only) | range: 1 to 84 | long |
| kct_module_season_3 | Module_3 | Integer module number for season 3. A module refers to a pair of CCDs that share a field flattener and are read out simultaneously by the detector electronics. There are 21 modules on the focal plane. MODULE is an integer from the set [2-4,6-20,22-24]. An object can have a non-zero module number if it is off, but near, a CCD. Such cases can be identified by examining the expected ROW and COLUMN values for a specified season. (KIC targets only) | 2-4,6-20,22-24 | long |
| kct_output_season_3 | Output_3 | Each module has four output channels (two per CCD). Each output is read out by a unique analog signal chain (e.g. amplifier). OUTPUT is an integer ranging from 1 to 4. An object can have a non-zero output number if it is off, but near, a CCD. Such cases can be identified by examining the expected ROW and COLUMN values for a specified season. (KIC targets only) | range 1 to 4 | long |
| kct_row_season_3 | Row_3 | Row number for season 3 with values ranging from -232 to 1098. Each channel has 1132 columns and 1070 rows. There are 1024 science rows enumerated as rows 20 through 1043. Collateral data is enumerated as rows 0 through 19 and 1044 through 1069. Values outside 0 through 1069 are enumerated in order to provide information about how far off a target is from the CCD channel. (KIC targets only) | range -228 to 1096 | long |
| kct_column_season_3 | Column_3 | Column number for season 3 defined like the Row values. Each channel has 1132 columns. There are 1100 science channels described as columns 12 - 1111. Collateral values range from 0-11 and 1112-1131. Other values ranging from -205 to -1 describe how far a target is from the CCD channel. (KIC targets only) | range -202 to 1111 | long |
| ktswcKey | Table key | A unique sequential number assigned to each target in the table. | range: 1 to 10,425,666 | long |
| condition_flag | Condition flag | Flags various categories of data as a semi-colon separated list. | See the condition_flag page for currently flagged conditions. | char |
| Column Name | Column Label | Description | Examples/Valid Values | Data Type |
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