The following table lists all of the data columns in the Kepler Stellar table that can be returned through the Exoplanet Archive's Application Programming Interface (API).
These column definitions apply to all deliveries of the Kepler stellar table. There are similar documents for the Confirmed Planets, TCE, Kepler Names and KOI tables.
The stellar table contains parameters for all targets observed by Kepler for the purpose of finding transiting planets. The current stellar table matches the values used by the Kepler pipeline when fitting TCEs identified in the Q1-12, Q1-16, Q1-17 DR 24 and Q1-17 DR 25 data. One additional table, the Q1-17 DR 25 Supplemental Stellar, includes values provided by the Kepler Stellar Properties Working Group (SPWG) independent of any pipeline processing in order to report their most current stellar values. See the Kepler Stellar documentation page for more information about each delivery.
Objects with KIC or KepID numbers over 100,000,000 are custom apertures. Please note that although stellar values may be listed here as these objects were processed through the Kepler pipeline, not all of these objects are stars. More information on custom apertures is available in section 2.2.1 of the archive manual.
Additional Links:
Questions about the structure and use of this table in the archive format should be submitted through the Exoplanet Archive's Helpdesk. Questions about the content descriptions should be sent to MAST.
If you use archive data or services for your research, please include the following Digital Object Identifier (DOI) as part of your acknowledgment:
DOI 10.26133/NEA6
See Acknowledging the Archive for dataset-specific language. See the full list of NASA Exoplanet Archive DOIs for other data sets and services.
Skip to:
Database Column Name | Table Label | Description | Uncertainties Column (positive +) (negative -) |
Displayed String Name |
---|---|---|---|---|
st_delivname† | Delivery Name | The stellar table delivery name from the Kepler Project. | ||
kepid† | KepID (KIC number) | Target identification number, as listed in the Kepler Input Catalog (KIC). The KIC was derived from a ground-based imaging survey of the Kepler field conducted prior to launch. The survey's purpose was to identify stars for the Kepler exoplanet survey by magnitude and color. The full catalog of 13 million sources can be searched at the MAST archive. The subset of 4 million targets found upon the Kepler CCDs can be searched via the Kepler Target Search form. The Kepler ID is unique to a target and there is only one Kepler ID per target. | ||
tm_designation† | 2MASS designation | 2MASS designation | ||
ra† | RA (deg) | KIC Right Ascension | ||
dec† | Dec (deg) | KIC Declination | ||
kepmag† | Kepler-band (mag)† | Kepler-band magnitude | ||
teff† | Stellar Effective Temperature (Kelvin) | The photospheric temperature of the star. | teff_err1, teff_err2 | teff_str |
logg† | Stellar Surface Gravity (log10(cm s-2)) | The base-10 logarithm of the acceleration due to gravity at the surface of the star. | logg_err1, logg_err2 | logg_str |
feh† | Stellar Metallicity | The base-10 logarithm of the Fe to H ratio at the surface of the star, normalized by the solar Fe to H ratio. | feh_err1, feh_err2 | feh_str |
teff_prov† | Effective Temperature Provenance |
A flag describing the source of the stellar effective
temperature, surface gravity and metallicity.
If the letter code is trailed by a number, the number corresponds to a specific paper. That list is available here. |
||
logg_prov† | Surface Gravity Provenance | |||
feh_prov† | Metallicity Provenance | |||
radius† | Stellar Radius (solar radii) | The photospheric radius of the star. | radius_err1, radius_err2 | radius_str |
mass† | Stellar Mass (solar mass) | The mass of the star. | mass_err1, mass_err2 | mass_str |
dens† | Stellar Density (gm/cm**3) | The density of the star. | dens_err1, dens_err2 | dens_str |
prov_sec† | Provenance of Secondary Stellar Parameters |
The internal parameters (R, M, rho) codes:
If the letter code is trailed by a number, the number corresponds to a specific paper. That list is available here. |
||
dist | Distance (pc) | Distance to the star in units of parsecs | dist_err1, dist_err2 | dist_str |
av | Av Extinction (mag) | Absorption and scattering of light in the V-band due to dust and gas in the line of sight. | av_err1, av_err2 | av_str |
limbdark_coeff1 | Limb Darkening Coefficient 1 | These report values for the four-parameter, non-linear model of Claret & Bloemen (2011) assuming the DR25 stellar parameters (Mathur et al. 2016). | ||
limbdark_coeff2 | Limb Darkening Coefficient 2 | |||
limbdark_coeff3 | Limb Darkening Coefficient 3 | |||
limbdark_coeff4 | Limb Darkening Coefficient 4 | |||
nconfp† | Number of Associated Confirmed Planets | Number of Confirmed Planets identified in a system. | ||
nkoi† | Number of KOIs | Number of Kepler Objects of Interest identified in a system. | ||
ntce† | Number of TCEs | Number of Kepler TCEs identified in a system. | ||
st_quarters† | Quarterly data exists | A string of 17 zeros and ones indicating which quarters have Kepler data (i.e., at least a target pixel file). The left-most bit represents quarter 1 and the quarters increase to the right. A target that has data for quarters 1, 5, 6, 7, 8, 14, and 16 will have the following string: 10001111000001010. | ||
st_vet_date† | Date of Last Update | Date of the last parameter update for this KepID |
Database Column Name | Table Label and Units | Description | Uncertainties Column (positive +) (negative -) |
Displayed String Name |
---|---|---|---|---|
jmag | J-band (2MASS) (mag) | Brightness of the star as measured using the J (2MASS) band in units of magnitude. Uncertainty values larger than 8 indicate that a reliable estimate of the photometric error could not be determined. | jmag_err | jmag_str |
hmag | H-band (2MASS) (mag) | Brightness of the star as measured using the H (2MASS) band in units of magnitude. Uncertainty values larger than 8 indicate that a reliable estimate of the photometric error could not be determined. | hmag_err | hmag_str |
kmag | K-band (2MASS) (mag) | Brightness of the star as measured using the K (2MASS) band in units of magnitude. Uncertainty values larger than 8 indicate that a reliable estimate of the photometric error could not be determined. | kmag_err | kmag_str |
datalink_dvr | Link to DV Report | Link to DV Report |
Last updated: 10 February 2021