{"table":"ps","database_column_name":"default_flag","table_label":"Default Parameter Set","description":"Boolean flag indicating whether given set of planet parameters has been selected as default (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":false,"default":true}
{"table":"ps","database_column_name":"soltype","table_label":"Solution Type","description":"Disposition of planet according to given planet parameter set","in_ps_table":true,"in_ps_comp_pars_table":false,"default":true}
{"table":"ps","database_column_name":"pl_controv_flag","table_label":"Controversial Flag","description":"Flag indicating whether the confirmation status of a planet has been questioned in the published literature (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"ps","database_column_name":"pl_name","table_label":"Planet Name","description":"Planet name most commonly used in the literature","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"ps","database_column_name":"hostname","table_label":"Host Name","description":"Stellar name most commonly used in the literature","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"ps","database_column_name":"pl_letter","table_label":"Planet Letter","description":"Letter assigned to the planetary component of a planetary system","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"hd_name","table_label":"HD ID","description":"Name of the star as given by the Henry Draper Catalog","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"hip_name","table_label":"HIP ID","description":"Name of the star as given by the Hipparcos Catalog","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"tic_id","table_label":"TIC ID","description":"Name of the star as given by the TESS Input Catalog","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"gaia_id","table_label":"GAIA ID","description":"Name of the star as given by the Gaia Catalog","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"sy_snum","table_label":"Number of Stars","description":"Number of stars in the planetary system","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"ps","database_column_name":"sy_pnum","table_label":"Number of Planets","description":"Number of planets in the planetary system","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"ps","database_column_name":"sy_mnum","table_label":"Number of Moons","description":"Number of moons in the planetary system","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"cb_flag","table_label":"Circumbinary Flag","description":"Flag indicating whether the planet orbits a binary system (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"discoverymethod","table_label":"Discovery Method","description":"Method by which the planet was first identified","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"ps","database_column_name":"disc_year","table_label":"Discovery Year","description":"Year the planet was discovered","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"ps","database_column_name":"disc_refname","table_label":"Discovery Reference","description":"Reference name for discovery publication","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"disc_pubdate","table_label":"Discovery Publication Date","description":"Publication Date of the planet discovery referee publication","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"disc_locale","table_label":"Discovery Locale","description":"Location of observation of planet discovery (Ground or Space)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"disc_facility","table_label":"Discovery Facility","description":"Name of facility of planet discovery observations","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"ps","database_column_name":"disc_telescope","table_label":"Discovery Telescope","description":"Name of telescope of planet discovery observations","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"disc_instrument","table_label":"Discovery Instrument","description":"Name of instrument of planet discovery observations","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"rv_flag","table_label":"Detections by Radial Velocity Variations","description":"Flag indicating if the planet host star exhibits radial velocity variations due to the planet (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pul_flag","table_label":"Detected by Pulsar Timing Variations","description":"Boolean flag indicating if the planet host star exhibits pulsar timing variations due to the planet (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"ptv_flag","table_label":"Detected by Pulsation Timing Variations","description":"Boolean flag indicating if the planet host star exhibits pulsation timing variations due to the planet (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"tran_flag","table_label":"Detected by Transits","description":"Flag indicating if the planet transits its host star (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"ast_flag","table_label":"Detected by Astrometric Variations","description":"Flag indicating if the planet host star exhibits astrometrical variations due to the planet (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"obm_flag","table_label":"Detected by Orbital Brightness Modulations","description":"Flag indicating whether the planet exhibits orbital modulations on the phase curve (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"micro_flag","table_label":"Detected by Microlensing","description":"Boolean flag indicating if the planetary system acted as a lens during an observed microlensing event (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"etv_flag","table_label":"Detected by Eclipse Timing Variations","description":"Boolean flag indicating if the planet induces transit timing variations on the orbit of another another planet in the system (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"ima_flag","table_label":"Detected by Imaging","description":"Flag indicating if the planet has been observed via imaging techniques (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"dkin_flag","table_label":"Detection by Disk Kinematics","description":"Boolean flag indicating if the presence of the planet was inferred due to its kinematic influence on the protoplanetary disk of its host star (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_refname","table_label":"Planetary Parameter Reference","description":"Reference of publication used for given planet parameter set","in_ps_table":true,"in_ps_comp_pars_table":false,"default":true}
{"table":"ps","database_column_name":"pl_orbper","table_label":"Orbital Period [days]","description":"Time the planet takes to make a complete orbit around the host star or system","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_orbpererr1 (-) pl_orbpererr2","limit_column":"pl_orbperlim","default":true}
{"table":"ps","database_column_name":"pl_orbper_reflink","table_label":"Orbital Period Reference","description":"Reference of publication used for given planet parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_orbsmax","table_label":"Orbit Semi-Major Axis [au]","description":"The longest radius of an elliptic orbit, or, for exoplanets detected via gravitational microlensing or direct imaging, the projected separation in the plane of the sky","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_orbsmaxerr1 (-) pl_orbsmaxerr2","limit_column":"pl_orbsmaxlim","default":true}
{"table":"ps","database_column_name":"pl_orbsmax_reflink","table_label":"Orbit Semi-Major Axis Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_rade","table_label":"Planet Radius [Earth Radius]","description":"Length of a line segment from the center of the planet to its surface, measured in units of radius of the Earth","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_radeerr1 (-) pl_radeerr2","limit_column":"pl_radelim","default":true}
{"table":"ps","database_column_name":"pl_rade_reflink","table_label":"Planet Radius [Earth Radius] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_radj","table_label":"Planet Radius [Jupiter Radius]","description":"Length of a line segment from the center of the planet to its surface, measured in units of radius of Jupiter","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_radjerr1 (-) pl_radjerr2","limit_column":"pl_radjlim","default":true}
{"table":"ps","database_column_name":"pl_radj_reflink","table_label":"Planet Radius [Jupiter Radius] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_masse","table_label":"Planet Mass [Earth Mass]","description":"Amount of matter contained in the planet, measured in units of masses of the Earth","in_ps_table":true,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) pl_masseerr1 (-) pl_masseerr2","limit_column":"pl_masselim","default":false}
{"table":"ps","database_column_name":"pl_massj","table_label":"Planet Mass [Jupiter Mass]","description":"Amount of matter contained in the planet, measured in units of masses of Jupiter","in_ps_table":true,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) pl_massjerr1 (-) pl_massjerr2","limit_column":"pl_massjlim","default":false}
{"table":"ps","database_column_name":"pl_msinie","table_label":"Planet Mass*sin(i) [Earth Mass]","description":"Minimum mass of a planet as measured by radial velocity, measured in units of masses of the Earth","in_ps_table":true,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) pl_msinieerr1 (-) pl_msinieerr2","limit_column":"pl_msinielim","default":false}
{"table":"ps","database_column_name":"pl_msinij","table_label":"Planet Mass*sin(i) [Jupiter Mass]","description":"Minimum mass of a planet as measured by radial velocity, measured in units of masses of Jupiter","in_ps_table":true,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) pl_msinijerr1 (-) pl_msinijerr2","limit_column":"pl_msinijlim","default":false}
{"table":"ps","database_column_name":"pl_cmasse","table_label":"Planet Mass*sin(i)/sin(i) [Earth Mass]","description":"A calculated quantity indicating the quotient of the lower limit of the measured planet mass, denoted as its mass times the sine of its inclination, and the sine of its inclination, measured in units of the mass of the Earth. This is specified for references in which the inclination is provided as well as the planet mass limit, but the true mass is not reported.","in_ps_table":true,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) pl_cmasseerr1 (-) pl_cmasseerr2","limit_column":"pl_cmasselim","default":false}
{"table":"ps","database_column_name":"pl_cmassj","table_label":"Planet Mass*sin(i)/sin(i) [Jupiter Mass]","description":"A calculated quantity indicating the quotient of the lower limit of the measured planet mass, denoted as its mass times the sine of its inclination, and the sine of its inclination, measured in units of the mass of Jupiter. This is specified for references in which the inclination is provided as well as the planet mass limit, but the true mass is not reported.","in_ps_table":true,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) pl_cmassjerr1 (-) pl_cmassjerr2","limit_column":"pl_cmassjlim","default":false}
{"table":"ps","database_column_name":"pl_bmasse","table_label":"Planet Mass or Mass*sin(i) [Earth Mass]","description":"Best planet mass estimate available, in order of preference: Mass, M*sin(i)/sin(i), or M*sin(i), depending on availability, and measured in Earth masses","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_bmasseerr1 (-) pl_bmasseerr2","limit_column":"pl_bmasselim","default":true}
{"table":"ps","database_column_name":"pl_bmasse_reflink","table_label":"Planet Mass or Mass*sin(i) [Earth Mass] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_bmassj","table_label":"Planet Mass or Mass*sin(i) [Jupiter Mass]","description":"Best planet mass estimate available, in order of preference: Mass, M*sin(i)/sin(i), or M*sin(i), depending on availability, and measured in Jupiter masses","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_bmassjerr1 (-) pl_bmassjerr2","limit_column":"pl_bmassjlim","default":true}
{"table":"ps","database_column_name":"pl_bmassj_reflink","table_label":"Planet Mass or Mass*sin(i) [Jupiter Mass] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_bmassprov","table_label":"Planet Mass or Mass*sin(i) Provenance","description":"Provenance of the measurement of the best mass. Options are: Mass, M*sin(i)/sin(i), and M*sini","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"ps","database_column_name":"pl_dens","table_label":"Planet Density [g/cm**3]","description":"Amount of mass per unit of volume of the planet","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_denserr1 (-) pl_denserr2","limit_column":"pl_denslim","default":false}
{"table":"ps","database_column_name":"pl_dens_reflink","table_label":"Planet Density [g/cm**3] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ps","database_column_name":"pl_orbeccen","table_label":"Eccentricity","description":"Amount by which the orbit of the planet deviates from a perfect circle","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_orbeccenerr1 (-) pl_orbeccenerr2","limit_column":"pl_orbeccenlim","default":true}
{"table":"ps","database_column_name":"pl_orbeccen_reflink","table_label":"Eccentricity Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ps","database_column_name":"pl_insol","table_label":"Insolation Flux [Earth Flux]","description":"Insolation flux is another way to give the equilibrium temperature. It's given in units relative to those measured for the Earth from the Sun.","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_insolerr1 (-) pl_insolerr2","limit_column":"pl_insollim","default":true}
{"table":"ps","database_column_name":"pl_insol_reflink","table_label":"Insolation Flux [Earth Flux] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_eqt","table_label":"Equilibrium Temperature [K]","description":"The equilibrium temperature of the planet as modeled by a black body heated only by its host star, or for directly imaged planets, the effective temperature of the planet required to match the measured luminosity if the planet were a black body","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_eqterr1 (-) pl_eqterr2","limit_column":"pl_eqtlim","default":true}
{"table":"ps","database_column_name":"pl_eqt_reflink","table_label":"Equilibrium Temperature [K] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_orbincl","table_label":"Inclination [deg]","description":"Angle of the plane of the orbit relative to the plane perpendicular to the line-of-sight from Earth to the object","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_orbinclerr1 (-) pl_orbinclerr2","limit_column":"pl_orbincllim","default":false}
{"table":"ps","database_column_name":"pl_tranmid","table_label":"Time of Conjuction (Transit Midpoint) [days]","description":"The time given by the average of the time the planet begins to cross the stellar limb and the time the planet finishes crossing the stellar limb.","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_tranmiderr1 (-) pl_tranmiderr2","limit_column":"pl_tranmidlim","default":false}
{"table":"ps","database_column_name":"pl_tranmid_reflink","table_label":"Time of Conjunction (Transit Midpoint) Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_tsystemref","table_label":"Time Reference Frame and Standard","description":"Time system basis for temporal and orbital parameters","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"ttv_flag","table_label":"Data show Transit Timing Variations","description":"Flag indicating if the planet orbit exhibits transit timing variations from another planet in the system (1=yes, 0=no). Note: Non-transiting planets discovered via the transit timing variations of another planet in the system will not have their TTV flag set, since they do not themselves demonstrate TTVs.","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"ps","database_column_name":"pl_imppar","table_label":"Impact Parameter","description":"The sky-projected distance between the center of the stellar disc and the center of the planet disc at conjunction, normalized by the stellar radius","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_impparerr1 (-) pl_impparerr2","limit_column":"pl_impparlim","default":false}
{"table":"ps","database_column_name":"pl_imppar_reflink","table_label":"Impact Parameter Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_trandep","table_label":"Transit Depth [%]","description":"The size of the relative flux decrement caused by the orbiting body transiting in front of the star","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_trandeperr1 (-) pl_trandeperr2","limit_column":"pl_trandeplim","default":false}
{"table":"ps","database_column_name":"pl_trandep_reflink","table_label":"Transit Depth [%] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_trandur","table_label":"Transit Duration [hrs]","description":"The length of time from the moment the planet begins to cross the stellar limb to the moment the planet finishes crossing the stellar limb","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_trandurerr1 (-) pl_trandurerr2","limit_column":"pl_trandurlim","default":false}
{"table":"ps","database_column_name":"pl_trandur_reflink","table_label":"Transit Duration [hrs] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_ratdor","table_label":"Ratio of Semi-Major Axis to Stellar Radius","description":"The distance between the planet and the star at mid-transit divided by the stellar radius. For the case of zero orbital eccentricity, the distance at mid-transit is the semi-major axis of the planetary orbit.","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_ratdorerr1 (-) pl_ratdorerr2","limit_column":"pl_ratdorlim","default":false}
{"table":"ps","database_column_name":"pl_ratdor_reflink","table_label":"Ratio of Semi-Major Axis to Stellar Radius Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_ratror","table_label":"Ratio of Planet to Stellar Radius","description":"The planet radius divided by the stellar radius","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_ratrorerr1 (-) pl_ratrorerr2","limit_column":"pl_ratrorlim","default":false}
{"table":"ps","database_column_name":"pl_ratror_reflink","table_label":"Ratio of Planet to Stellar Radius Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_occdep","table_label":"Occultation Depth [%]","description":"Depth of occultation of secondary eclipse","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_occdeperr1 (-) pl_occdeperr2","limit_column":"pl_occdeplim","default":false}
{"table":"ps","database_column_name":"pl_occdep_reflink","table_label":"Occultation Depth [%] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_orbtper","table_label":"Epoch of Periastron [deg]","description":"The time of the planet's periastron passage","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_orbtpererr1 (-) pl_orbtpererr2","limit_column":"pl_orbtperlim","default":false}
{"table":"ps","database_column_name":"pl_orbtper_reflink","table_label":"Epoch of Periastron [deg] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_orblper","table_label":"Argument of Periastron [deg]","description":"The angular separation between the orbit's ascending node and periastron. Note: there are a varying conventions in the exoplanet literature regarding argument of periastron (or periapsis). For example, some publications refer the planet's orbit, others to the host star's reflex orbit, which differs by 180 deg. The values in the Exoplanet Archive are not corrected to a standardized system, but are as-reported for each publication.","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_orblpererr1 (-) pl_orblpererr2","limit_column":"pl_orblperlim","default":false}
{"table":"ps","database_column_name":"pl_rvamp","table_label":"Radial Velocity Amplitude [m/s]","description":"Half the peak-to-peak amplitude of variability in the stellar radial velocity","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_rvamperr1 (-) pl_rvamperr2","limit_column":"pl_rvamplim","default":false}
{"table":"ps","database_column_name":"pl_rvamp_reflink","table_label":"Radial Velocity Amplitude Reference [m/s]","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_projobliq","table_label":"Projected Obliquity [deg]","description":"The angle between the angular momentum vector of the rotation of the host star and the angular momentum vector of the orbit of the planet, projected into the plane of the sky. Depending on the choice of coordinate system, projected obliquity is represented in the literature as either lambda (λ) or beta (β), where λ is defined as the negative of β (i.e., λ = -β). Since λ is reported more often than β, all values of β have been converted to λ.","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_projobliqerr1 (-) pl_projobliqerr2","limit_column":"pl_projobliqlim","default":false}
{"table":"ps","database_column_name":"pl_projobliq_reflink","table_label":"Projected Obliquity [deg] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_trueobliq","table_label":"True Obliquity [deg]","description":"The angle between the angular momentum vector of the rotation of the host star and the angular momentum vector of the orbit of the planet","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_trueobliqerr1 (-) pl_trueobliqerr2","limit_column":"pl_trueobliqlim","default":false}
{"table":"ps","database_column_name":"pl_trueobliq_reflink","table_label":"True Obliquity [deg] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"st_refname","table_label":"Stellar Parameter Reference","description":"Reference of publication used for given stellar parameter set","in_ps_table":true,"in_ps_comp_pars_table":false,"default":true}
{"table":"ps","database_column_name":"st_spectype","table_label":"Spectral Type","description":"Classification of the star based on their spectral characteristics following the Morgan-Keenan system","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"st_spectype_reflink","table_label":"Spectral Type Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"st_teff","table_label":"Stellar Effective Temperature [K]","description":"Temperature of the star as modeled by a black body emitting the same total amount of electromagnetic radiation","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) st_tefferr1 (-) st_tefferr2","limit_column":"st_tefflim","default":true}
{"table":"ps","database_column_name":"st_teff_reflink","table_label":"Stellar Effective Temperature [K] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
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{"table":"ps","database_column_name":"sy_kepmag_reflink","table_label":"Kepler Magnitude Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"rowupdate","table_label":"Date of Last Update","description":"Date of last update of the planet parameters","in_ps_table":true,"in_ps_comp_pars_table":false,"default":true}
{"table":"ps","database_column_name":"pl_pubdate","table_label":"Planetary Parameter Reference Publication","description":"Date of the publication of the given planet parameter set","in_ps_table":true,"in_ps_comp_pars_table":false,"default":true}
{"table":"ps","database_column_name":"releasedate","table_label":"Release Date","description":"Date that the given planet parameter set was publicly released by the NASA Exoplanet Archive","in_ps_table":true,"in_ps_comp_pars_table":false,"default":true}
{"table":"ps","database_column_name":"st_nphot","table_label":"Number of Photometry Time Series","description":"Number of photometric time series records, including planet transit light curves, general transit light curves, and amateur light curves.","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"st_nrvc","table_label":"Number of Radial Velocity Time Series","description":"Number of literature radial velocity curves available for this star in the NASA Exoplanet Archive.","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_ntranspec","table_label":"Number of Transmission Spectroscopy Measurements","description":"Number of literature transmission spectrum measurements for this star in the NASA Exoplanet Archive","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"pl_nespec","table_label":"Number of Emission Spectroscopy Measurements","description":"Number of literature emission spectrum measurements for this star in the NASA Exoplanet Archive","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ps","database_column_name":"st_nspec","table_label":"Number of Stellar Spectra Measurements","description":"Number of literature spectra available for this star in the NASA Exoplanet Archive","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"default_flag","table_label":"Default Parameter Set","description":"Boolean flag indicating whether given set of planet parameters has been selected as default (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":false,"default":true}
{"table":"pscomppars","database_column_name":"soltype","table_label":"Solution Type","description":"Disposition of planet according to given planet parameter set","in_ps_table":true,"in_ps_comp_pars_table":false,"default":true}
{"table":"pscomppars","database_column_name":"pl_controv_flag","table_label":"Controversial Flag","description":"Flag indicating whether the confirmation status of a planet has been questioned in the published literature (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"pscomppars","database_column_name":"pl_name","table_label":"Planet Name","description":"Planet name most commonly used in the literature","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"pscomppars","database_column_name":"hostname","table_label":"Host Name","description":"Stellar name most commonly used in the literature","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"pscomppars","database_column_name":"pl_letter","table_label":"Planet Letter","description":"Letter assigned to the planetary component of a planetary system","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"hd_name","table_label":"HD ID","description":"Name of the star as given by the Henry Draper Catalog","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"hip_name","table_label":"HIP ID","description":"Name of the star as given by the Hipparcos Catalog","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"tic_id","table_label":"TIC ID","description":"Name of the star as given by the TESS Input Catalog","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"gaia_id","table_label":"GAIA ID","description":"Name of the star as given by the Gaia Catalog","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"sy_snum","table_label":"Number of Stars","description":"Number of stars in the planetary system","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"pscomppars","database_column_name":"sy_pnum","table_label":"Number of Planets","description":"Number of planets in the planetary system","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"pscomppars","database_column_name":"sy_mnum","table_label":"Number of Moons","description":"Number of moons in the planetary system","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"cb_flag","table_label":"Circumbinary Flag","description":"Flag indicating whether the planet orbits a binary system (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"discoverymethod","table_label":"Discovery Method","description":"Method by which the planet was first identified","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"pscomppars","database_column_name":"disc_year","table_label":"Discovery Year","description":"Year the planet was discovered","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"pscomppars","database_column_name":"disc_refname","table_label":"Discovery Reference","description":"Reference name for discovery publication","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"disc_pubdate","table_label":"Discovery Publication Date","description":"Publication Date of the planet discovery referee publication","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"disc_locale","table_label":"Discovery Locale","description":"Location of observation of planet discovery (Ground or Space)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"disc_facility","table_label":"Discovery Facility","description":"Name of facility of planet discovery observations","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"pscomppars","database_column_name":"disc_telescope","table_label":"Discovery Telescope","description":"Name of telescope of planet discovery observations","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"disc_instrument","table_label":"Discovery Instrument","description":"Name of instrument of planet discovery observations","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"rv_flag","table_label":"Detections by Radial Velocity Variations","description":"Flag indicating if the planet host star exhibits radial velocity variations due to the planet (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pul_flag","table_label":"Detected by Pulsar Timing Variations","description":"Boolean flag indicating if the planet host star exhibits pulsar timing variations due to the planet (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"ptv_flag","table_label":"Detected by Pulsation Timing Variations","description":"Boolean flag indicating if the planet host star exhibits pulsation timing variations due to the planet (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"tran_flag","table_label":"Detected by Transits","description":"Flag indicating if the planet transits its host star (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"ast_flag","table_label":"Detected by Astrometric Variations","description":"Flag indicating if the planet host star exhibits astrometrical variations due to the planet (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"obm_flag","table_label":"Detected by Orbital Brightness Modulations","description":"Flag indicating whether the planet exhibits orbital modulations on the phase curve (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"micro_flag","table_label":"Detected by Microlensing","description":"Boolean flag indicating if the planetary system acted as a lens during an observed microlensing event (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"etv_flag","table_label":"Detected by Eclipse Timing Variations","description":"Boolean flag indicating if the planet induces transit timing variations on the orbit of another another planet in the system (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"ima_flag","table_label":"Detected by Imaging","description":"Flag indicating if the planet has been observed via imaging techniques (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"dkin_flag","table_label":"Detection by Disk Kinematics","description":"Boolean flag indicating if the presence of the planet was inferred due to its kinematic influence on the protoplanetary disk of its host star (1=yes, 0=no)","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_refname","table_label":"Planetary Parameter Reference","description":"Reference of publication used for given planet parameter set","in_ps_table":true,"in_ps_comp_pars_table":false,"default":true}
{"table":"pscomppars","database_column_name":"pl_orbper","table_label":"Orbital Period [days]","description":"Time the planet takes to make a complete orbit around the host star or system","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_orbpererr1 (-) pl_orbpererr2","limit_column":"pl_orbperlim","default":true}
{"table":"pscomppars","database_column_name":"pl_orbper_reflink","table_label":"Orbital Period Reference","description":"Reference of publication used for given planet parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_orbsmax","table_label":"Orbit Semi-Major Axis [au]","description":"The longest radius of an elliptic orbit, or, for exoplanets detected via gravitational microlensing or direct imaging, the projected separation in the plane of the sky","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_orbsmaxerr1 (-) pl_orbsmaxerr2","limit_column":"pl_orbsmaxlim","default":true}
{"table":"pscomppars","database_column_name":"pl_orbsmax_reflink","table_label":"Orbit Semi-Major Axis Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_rade","table_label":"Planet Radius [Earth Radius]","description":"Length of a line segment from the center of the planet to its surface, measured in units of radius of the Earth","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_radeerr1 (-) pl_radeerr2","limit_column":"pl_radelim","default":true}
{"table":"pscomppars","database_column_name":"pl_rade_reflink","table_label":"Planet Radius [Earth Radius] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_radj","table_label":"Planet Radius [Jupiter Radius]","description":"Length of a line segment from the center of the planet to its surface, measured in units of radius of Jupiter","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_radjerr1 (-) pl_radjerr2","limit_column":"pl_radjlim","default":true}
{"table":"pscomppars","database_column_name":"pl_radj_reflink","table_label":"Planet Radius [Jupiter Radius] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_masse","table_label":"Planet Mass [Earth Mass]","description":"Amount of matter contained in the planet, measured in units of masses of the Earth","in_ps_table":true,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) pl_masseerr1 (-) pl_masseerr2","limit_column":"pl_masselim","default":false}
{"table":"pscomppars","database_column_name":"pl_massj","table_label":"Planet Mass [Jupiter Mass]","description":"Amount of matter contained in the planet, measured in units of masses of Jupiter","in_ps_table":true,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) pl_massjerr1 (-) pl_massjerr2","limit_column":"pl_massjlim","default":false}
{"table":"pscomppars","database_column_name":"pl_msinie","table_label":"Planet Mass*sin(i) [Earth Mass]","description":"Minimum mass of a planet as measured by radial velocity, measured in units of masses of the Earth","in_ps_table":true,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) pl_msinieerr1 (-) pl_msinieerr2","limit_column":"pl_msinielim","default":false}
{"table":"pscomppars","database_column_name":"pl_msinij","table_label":"Planet Mass*sin(i) [Jupiter Mass]","description":"Minimum mass of a planet as measured by radial velocity, measured in units of masses of Jupiter","in_ps_table":true,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) pl_msinijerr1 (-) pl_msinijerr2","limit_column":"pl_msinijlim","default":false}
{"table":"pscomppars","database_column_name":"pl_cmasse","table_label":"Planet Mass*sin(i)/sin(i) [Earth Mass]","description":"A calculated quantity indicating the quotient of the lower limit of the measured planet mass, denoted as its mass times the sine of its inclination, and the sine of its inclination, measured in units of the mass of the Earth. This is specified for references in which the inclination is provided as well as the planet mass limit, but the true mass is not reported.","in_ps_table":true,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) pl_cmasseerr1 (-) pl_cmasseerr2","limit_column":"pl_cmasselim","default":false}
{"table":"pscomppars","database_column_name":"pl_cmassj","table_label":"Planet Mass*sin(i)/sin(i) [Jupiter Mass]","description":"A calculated quantity indicating the quotient of the lower limit of the measured planet mass, denoted as its mass times the sine of its inclination, and the sine of its inclination, measured in units of the mass of Jupiter. This is specified for references in which the inclination is provided as well as the planet mass limit, but the true mass is not reported.","in_ps_table":true,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) pl_cmassjerr1 (-) pl_cmassjerr2","limit_column":"pl_cmassjlim","default":false}
{"table":"pscomppars","database_column_name":"pl_bmasse","table_label":"Planet Mass or Mass*sin(i) [Earth Mass]","description":"Best planet mass estimate available, in order of preference: Mass, M*sin(i)/sin(i), or M*sin(i), depending on availability, and measured in Earth masses","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_bmasseerr1 (-) pl_bmasseerr2","limit_column":"pl_bmasselim","default":true}
{"table":"pscomppars","database_column_name":"pl_bmasse_reflink","table_label":"Planet Mass or Mass*sin(i) [Earth Mass] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_bmassj","table_label":"Planet Mass or Mass*sin(i) [Jupiter Mass]","description":"Best planet mass estimate available, in order of preference: Mass, M*sin(i)/sin(i), or M*sin(i), depending on availability, and measured in Jupiter masses","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_bmassjerr1 (-) pl_bmassjerr2","limit_column":"pl_bmassjlim","default":true}
{"table":"pscomppars","database_column_name":"pl_bmassj_reflink","table_label":"Planet Mass or Mass*sin(i) [Jupiter Mass] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_bmassprov","table_label":"Planet Mass or Mass*sin(i) Provenance","description":"Provenance of the measurement of the best mass. Options are: Mass, M*sin(i)/sin(i), and M*sini","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"pscomppars","database_column_name":"pl_dens","table_label":"Planet Density [g/cm**3]","description":"Amount of mass per unit of volume of the planet","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_denserr1 (-) pl_denserr2","limit_column":"pl_denslim","default":false}
{"table":"pscomppars","database_column_name":"pl_dens_reflink","table_label":"Planet Density [g/cm**3] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"pscomppars","database_column_name":"pl_orbeccen","table_label":"Eccentricity","description":"Amount by which the orbit of the planet deviates from a perfect circle","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_orbeccenerr1 (-) pl_orbeccenerr2","limit_column":"pl_orbeccenlim","default":true}
{"table":"pscomppars","database_column_name":"pl_orbeccen_reflink","table_label":"Eccentricity Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"pscomppars","database_column_name":"pl_insol","table_label":"Insolation Flux [Earth Flux]","description":"Insolation flux is another way to give the equilibrium temperature. It's given in units relative to those measured for the Earth from the Sun.","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_insolerr1 (-) pl_insolerr2","limit_column":"pl_insollim","default":true}
{"table":"pscomppars","database_column_name":"pl_insol_reflink","table_label":"Insolation Flux [Earth Flux] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_eqt","table_label":"Equilibrium Temperature [K]","description":"The equilibrium temperature of the planet as modeled by a black body heated only by its host star, or for directly imaged planets, the effective temperature of the planet required to match the measured luminosity if the planet were a black body","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_eqterr1 (-) pl_eqterr2","limit_column":"pl_eqtlim","default":true}
{"table":"pscomppars","database_column_name":"pl_eqt_reflink","table_label":"Equilibrium Temperature [K] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_orbincl","table_label":"Inclination [deg]","description":"Angle of the plane of the orbit relative to the plane perpendicular to the line-of-sight from Earth to the object","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_orbinclerr1 (-) pl_orbinclerr2","limit_column":"pl_orbincllim","default":false}
{"table":"pscomppars","database_column_name":"pl_tranmid","table_label":"Time of Conjuction (Transit Midpoint) [days]","description":"The time given by the average of the time the planet begins to cross the stellar limb and the time the planet finishes crossing the stellar limb.","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_tranmiderr1 (-) pl_tranmiderr2","limit_column":"pl_tranmidlim","default":false}
{"table":"pscomppars","database_column_name":"pl_tranmid_reflink","table_label":"Time of Conjunction (Transit Midpoint) Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_tsystemref","table_label":"Time Reference Frame and Standard","description":"Time system basis for temporal and orbital parameters","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"ttv_flag","table_label":"Data show Transit Timing Variations","description":"Flag indicating if the planet orbit exhibits transit timing variations from another planet in the system (1=yes, 0=no). Note: Non-transiting planets discovered via the transit timing variations of another planet in the system will not have their TTV flag set, since they do not themselves demonstrate TTVs.","in_ps_table":true,"in_ps_comp_pars_table":true,"default":true}
{"table":"pscomppars","database_column_name":"pl_imppar","table_label":"Impact Parameter","description":"The sky-projected distance between the center of the stellar disc and the center of the planet disc at conjunction, normalized by the stellar radius","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_impparerr1 (-) pl_impparerr2","limit_column":"pl_impparlim","default":false}
{"table":"pscomppars","database_column_name":"pl_imppar_reflink","table_label":"Impact Parameter Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_trandep","table_label":"Transit Depth [%]","description":"The size of the relative flux decrement caused by the orbiting body transiting in front of the star","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_trandeperr1 (-) pl_trandeperr2","limit_column":"pl_trandeplim","default":false}
{"table":"pscomppars","database_column_name":"pl_trandep_reflink","table_label":"Transit Depth [%] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_trandur","table_label":"Transit Duration [hrs]","description":"The length of time from the moment the planet begins to cross the stellar limb to the moment the planet finishes crossing the stellar limb","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_trandurerr1 (-) pl_trandurerr2","limit_column":"pl_trandurlim","default":false}
{"table":"pscomppars","database_column_name":"pl_trandur_reflink","table_label":"Transit Duration [hrs] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_ratdor","table_label":"Ratio of Semi-Major Axis to Stellar Radius","description":"The distance between the planet and the star at mid-transit divided by the stellar radius. For the case of zero orbital eccentricity, the distance at mid-transit is the semi-major axis of the planetary orbit.","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_ratdorerr1 (-) pl_ratdorerr2","limit_column":"pl_ratdorlim","default":false}
{"table":"pscomppars","database_column_name":"pl_ratdor_reflink","table_label":"Ratio of Semi-Major Axis to Stellar Radius Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_ratror","table_label":"Ratio of Planet to Stellar Radius","description":"The planet radius divided by the stellar radius","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_ratrorerr1 (-) pl_ratrorerr2","limit_column":"pl_ratrorlim","default":false}
{"table":"pscomppars","database_column_name":"pl_ratror_reflink","table_label":"Ratio of Planet to Stellar Radius Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_occdep","table_label":"Occultation Depth [%]","description":"Depth of occultation of secondary eclipse","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_occdeperr1 (-) pl_occdeperr2","limit_column":"pl_occdeplim","default":false}
{"table":"pscomppars","database_column_name":"pl_occdep_reflink","table_label":"Occultation Depth [%] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_orbtper","table_label":"Epoch of Periastron [deg]","description":"The time of the planet's periastron passage","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_orbtpererr1 (-) pl_orbtpererr2","limit_column":"pl_orbtperlim","default":false}
{"table":"pscomppars","database_column_name":"pl_orbtper_reflink","table_label":"Epoch of Periastron [deg] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_orblper","table_label":"Argument of Periastron [deg]","description":"The angular separation between the orbit's ascending node and periastron. Note: there are a varying conventions in the exoplanet literature regarding argument of periastron (or periapsis). For example, some publications refer the planet's orbit, others to the host star's reflex orbit, which differs by 180 deg. The values in the Exoplanet Archive are not corrected to a standardized system, but are as-reported for each publication.","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_orblpererr1 (-) pl_orblpererr2","limit_column":"pl_orblperlim","default":false}
{"table":"pscomppars","database_column_name":"pl_rvamp","table_label":"Radial Velocity Amplitude [m/s]","description":"Half the peak-to-peak amplitude of variability in the stellar radial velocity","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_rvamperr1 (-) pl_rvamperr2","limit_column":"pl_rvamplim","default":false}
{"table":"pscomppars","database_column_name":"pl_rvamp_reflink","table_label":"Radial Velocity Amplitude Reference [m/s]","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_projobliq","table_label":"Projected Obliquity [deg]","description":"The angle between the angular momentum vector of the rotation of the host star and the angular momentum vector of the orbit of the planet, projected into the plane of the sky. Depending on the choice of coordinate system, projected obliquity is represented in the literature as either lambda (λ) or beta (β), where λ is defined as the negative of β (i.e., λ = -β). Since λ is reported more often than β, all values of β have been converted to λ.","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_projobliqerr1 (-) pl_projobliqerr2","limit_column":"pl_projobliqlim","default":false}
{"table":"pscomppars","database_column_name":"pl_projobliq_reflink","table_label":"Projected Obliquity [deg] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_trueobliq","table_label":"True Obliquity [deg]","description":"The angle between the angular momentum vector of the rotation of the host star and the angular momentum vector of the orbit of the planet","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) pl_trueobliqerr1 (-) pl_trueobliqerr2","limit_column":"pl_trueobliqlim","default":false}
{"table":"pscomppars","database_column_name":"pl_trueobliq_reflink","table_label":"True Obliquity [deg] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"st_refname","table_label":"Stellar Parameter Reference","description":"Reference of publication used for given stellar parameter set","in_ps_table":true,"in_ps_comp_pars_table":false,"default":true}
{"table":"pscomppars","database_column_name":"st_spectype","table_label":"Spectral Type","description":"Classification of the star based on their spectral characteristics following the Morgan-Keenan system","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"st_spectype_reflink","table_label":"Spectral Type Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"st_teff","table_label":"Stellar Effective Temperature [K]","description":"Temperature of the star as modeled by a black body emitting the same total amount of electromagnetic radiation","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) st_tefferr1 (-) st_tefferr2","limit_column":"st_tefflim","default":true}
{"table":"pscomppars","database_column_name":"st_teff_reflink","table_label":"Stellar Effective Temperature [K] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"st_rad","table_label":"Stellar Radius [Solar Radius]","description":"Length of a line segment from the center of the star to its surface, measured in units of radius of the Sun","in_ps_table":true,"in_ps_comp_pars_table":true,"uncertainties_column_positive_negative":"(+) st_raderr1 (-) st_raderr2","limit_column":"st_radlim","default":true}
{"table":"pscomppars","database_column_name":"st_rad_reflink","table_label":"Stellar Radius [Solar Radius] Reference","description":"Reference of publication used for given parameter set","in_ps_table":false,"in_ps_comp_pars_table":true,"default":false}
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{"table":"pscomppars","database_column_name":"rowupdate","table_label":"Date of Last Update","description":"Date of last update of the planet parameters","in_ps_table":true,"in_ps_comp_pars_table":false,"default":true}
{"table":"pscomppars","database_column_name":"pl_pubdate","table_label":"Planetary Parameter Reference Publication","description":"Date of the publication of the given planet parameter set","in_ps_table":true,"in_ps_comp_pars_table":false,"default":true}
{"table":"pscomppars","database_column_name":"releasedate","table_label":"Release Date","description":"Date that the given planet parameter set was publicly released by the NASA Exoplanet Archive","in_ps_table":true,"in_ps_comp_pars_table":false,"default":true}
{"table":"pscomppars","database_column_name":"st_nphot","table_label":"Number of Photometry Time Series","description":"Number of photometric time series records, including planet transit light curves, general transit light curves, and amateur light curves.","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"st_nrvc","table_label":"Number of Radial Velocity Time Series","description":"Number of literature radial velocity curves available for this star in the NASA Exoplanet Archive.","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_ntranspec","table_label":"Number of Transmission Spectroscopy Measurements","description":"Number of literature transmission spectrum measurements for this star in the NASA Exoplanet Archive","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"pl_nespec","table_label":"Number of Emission Spectroscopy Measurements","description":"Number of literature emission spectrum measurements for this star in the NASA Exoplanet Archive","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"pscomppars","database_column_name":"st_nspec","table_label":"Number of Stellar Spectra Measurements","description":"Number of literature spectra available for this star in the NASA Exoplanet Archive","in_ps_table":true,"in_ps_comp_pars_table":true,"default":false}
{"table":"ML","database_column_name":"pl_name","table_label":"Planet Name","description":"Planet name","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ML","database_column_name":"rastr","table_label":"RA [sexagesimal]","description":"Right ascension of the microlensing event, in sexagesimal format","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ML","database_column_name":"decstr","table_label":"Dec [sexagesimal]","description":"Declination of the microlensing event, in sexagesimal format","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ML","database_column_name":"pl_massj","table_label":"Planet Mass [Jupiter mass]","description":"Mass of planet, in Jupiter masses","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) pl_orbmassjerr1 (-) pl_massjerr2","limit_column":"pl_massjlim","default":false}
{"table":"ML","database_column_name":"pl_masse","table_label":"Planet Mass [Earth mass]","description":"Mass of planet, in Earth masses","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) pl_orbmasseerr1 (-) pl_masseerr2","limit_column":"pl_masselim","default":false}
{"table":"ML","database_column_name":"pl_orbsmax","table_label":"Planet-star Projected Semi-major Axis [au]","description":"Projected physical separation of the planet and the host star in the plane of the sky at the time of the event","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) pl_orbsmaxerr1 (-) pl_orbsmaxerr2","limit_column":"pl_orbsmaxlim","default":false}
{"table":"ML","database_column_name":"st_mass","table_label":"Lens Mass [Solar mass]","description":"Host star mass","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) st_masserr1 (-) st_masserr2","limit_column":"sy_dist","default":false}
{"table":"ML","database_column_name":"sy_dist","table_label":"Lens Distance [pc]","description":"Distance from the observer to the lens system","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) sy_disterr1 (-) sy_disterr2","limit_column":"sy_distlim","default":false}
{"table":"ML","database_column_name":"ml_dists","table_label":"Source Distance [pc]","description":"Distance from the observer to the source system","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_distserr1 (-) ml_distserr2","limit_column":"ml_distslim","default":false}
{"table":"ML","database_column_name":"ml_tsepmin","table_label":"Time of Lens-source Minimum Separation [days]","description":"Time of lense-source minimum separation in the plane of the sky","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_tsepminerr1 (-) ml_tsepminerr2","limit_column":"ml_tsepmin","default":false}
{"table":"ML","database_column_name":"ml_sepminnorm","table_label":"Normalized Lens-source Minimum Separation","description":"Angular lens-source minimum separation in the plane of the sky, normalized to the angular Einstein radius (microlens impact parameter)","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_sepminnormerr1 (-) ml_sepminnormerr2","limit_column":"ml_sepminnormlim","default":false}
{"table":"ML","database_column_name":"ml_xtimeein","table_label":"Einstein Crossing Time [days]","description":"Time for the lens-source separation to change by one angular Einstein radius","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_xtimeeinerr1 (-) ml_xtimeeinerr2","limit_column":"ml_xtimeeinlim","default":false}
{"table":"ML","database_column_name":"ml_radsnorm","table_label":"Normalized Source Angular Radius (10-3)","description":"Ratio of angular source star radius to the angular Einstein radius (x 10-3)","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_radsnormerr1 (-) ml_radsnormerr2","limit_column":"ml_radsnormlim","default":false}
{"table":"ML","database_column_name":"ml_sepinsnorp","table_label":"Instantaneous Planet-star Projected and Normalized Separation","description":"Projected, angular separation of the planet and the host star in the plane of the sky at the time of the event, normalized to the angular Einstein radius","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_sepinsnorperr1 (-) ml_sepinsnorperr2","limit_column":"mlmassratio","default":false}
{"table":"ML","database_column_name":"ml_massratio","table_label":"Planet-star Mass Ratio (10-4)","description":"Ratio of the planet mass to the host star mass (lens system; x 10-4)","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_massratioerr1 (-) ml_massratioerr2","limit_column":"ml_massratiolim","default":false}
{"table":"ML","database_column_name":"ml_angstlax","table_label":"Source Trajectory-lens Axis Angle [rad]","description":"Angle of the source system trajectory relative to the lens system axis","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_angstlaxerr1 (-) ml_angstlaxerr2","limit_column":"ml_angstlaxlim","default":false}
{"table":"ML","database_column_name":"ml_magis","table_label":"Source I-band [mag]","description":"Brightness of the unmagnified source star, in I-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_magiserr1 (-) ml_magiserr2","limit_column":"ml_magislim","default":false}
{"table":"ML","database_column_name":"ml_magibl","table_label":"Blend I-band [mag]","description":"Brightness of all objects, excluding the source star, superposed at the time of the event, in I-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_magiblerr1 (-) ml_magiblerr2","limit_column":"ml_magibllim","default":false}
{"table":"ML","database_column_name":"ml_radeinang","table_label":"Angular Einstein Radius [mas]","description":"Angular radius of the Einstein ring","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_radeinangerr1 (-) ml_radeinangerr2","limit_column":"ml_radeinanglim","default":false}
{"table":"ML","database_column_name":"ml_pmrells","table_label":"Lens-source Relative Proper Motion [mas/yr]","description":"Lens-source relative proper motion","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_pmrellserr1 (-) ml_pmrellserr2","limit_column":"ml_pmrellslim","default":false}
{"table":"ML","database_column_name":"ml_modeldef","table_label":"Default Model","description":"Binary flag indicating whether given microlens model is the default; best-fit model (1=yes; 0=no)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ML","database_column_name":"htmllink","table_label":"Reference","description":"Reference","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ML","database_column_name":"ra","table_label":"RA [deg]","description":"Right ascension of the microlensing event, in decimal degrees","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ML","database_column_name":"dec","table_label":"Dec [deg]","description":"Declination of the microlensing event, in decimal degrees","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ML","database_column_name":"glon","table_label":"Galactic Longitude [deg]","description":"Galactic longitude of the microlensing event, in decimal degrees","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ML","database_column_name":"glat","table_label":"Galactic Latitude [deg]","description":"Galactic latitude of the microlensing event, in decimal degrees","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ML","database_column_name":"ml_plxrel","table_label":"Lens-source Relative Parallax","description":"Lens-source relative parallax","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_plxrelerr1 (-) ml_plxrelerr2","limit_column":"ml_plxrellim","default":false}
{"table":"ML","database_column_name":"ml_plxmicro","table_label":"Microlens Parallax","description":"Lens-source relative parallax normalized to the angular Einstein radius","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_plxmicroerr1 (-) ml_plxmicroerr2","limit_column":"ml_plxicrolim","default":false}
{"table":"ML","database_column_name":"ml_plxmicron","table_label":"Microlens Parallax (North Component)","description":"North component of the microlens parallax","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_plxmicronerr1 (-) ml_plxmicronerr2","limit_column":"ml_plxmicronlim","default":false}
{"table":"ML","database_column_name":"ml_plxmicroe","table_label":"Microlens Parallax (East Component)","description":"East component of the microlens parallax","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_plxmicroeerr1 (-) ml_plxmicroeerr2","limit_column":"ml_plxmicroelim","default":false}
{"table":"ML","database_column_name":"ml_dsdt","table_label":"Planet-star Separation Rate of Change [yr-1]","description":"Time rate of change of the projected, angular, normalized separation of the planet and host star in the plane of the sky due to orbital motion of the lens components","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_dsdterr1 (-) ml_dsdterr2","limit_column":"ml_dsdtlim","default":false}
{"table":"ML","database_column_name":"ml_dalphadt","table_label":"Source Trajectory Angle Rate of Change [rad/yr]","description":"Time rate of change of the angle of the source system trajectory to the lens system axis due to the orbital motion of the lens components","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_dalphadterr1 (-) ml_dalphadterr2","limit_column":"ml_dalphadtlim","default":false}
{"table":"ML","database_column_name":"ml_radsang","table_label":"Source Angular Radius [microas]","description":"Angular source star radius","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_radsangerr1 (-) ml_radsangerr2","limit_column":"ml_radsanglim","default":false}
{"table":"ML","database_column_name":"ml_radsphy","table_label":"Source Physical Radius [Solar radii]","description":"Physical source star radius","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_radsphyerr1 (-) ml_radsphyerr2","limit_column":"ml_radsphylim","default":false}
{"table":"ML","database_column_name":"ml_xtimesrc","table_label":"Source Crossing Time [days]","description":"Time for the lens-source separation to change by one angular source radius","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_xtimesrcerr1 (-) ml_xtimesrcerr2","limit_column":"ml_xtimesrclim","default":false}
{"table":"ML","database_column_name":"ml_efftime","table_label":"Effective Timescale [days]","description":"Effective timescale, equal to the product of the microlens impact parameter and the Einstein crossing time","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_efftimeerr1 (-) ml_efftimeerr2","limit_column":"ml_efftimelim","default":false}
{"table":"ML","database_column_name":"ml_pms","table_label":"Source Proper Motion [mas/yr]","description":"Source system proper motion","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_pmserr1 (-) ml_pmserr2","limit_column":"ml_pmslim","default":false}
{"table":"ML","database_column_name":"ml_magvs","table_label":"Source V-band [mag]","description":"Brightness of the unmagnified source star, in V-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_magvserr1 (-) ml_magvserr2","limit_column":"ml_magvslim","default":false}
{"table":"ML","database_column_name":"ml_magvso","table_label":"Source De-reddened V-band [mag]","description":"De-reddened brightness of the unmagnified source star, in V-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_magvsoerr1 (-) ml_magvsoerr2","limit_column":"ml_magvsolim","default":false}
{"table":"ML","database_column_name":"ml_magiso","table_label":"Source De-reddened I-band [mag]","description":"De-reddened brightness of the unmagnified source star, in I-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_magisoerr1 (-) ml_magisoerr2","limit_column":"ml_magisolim","default":false}
{"table":"ML","database_column_name":"ml_magjs","table_label":"Source J-band [mag]","description":"Brightness of the unmagnified source star, in J-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_magjserr1 (-) ml_magjserr2","limit_column":"ml_magjslim","default":false}
{"table":"ML","database_column_name":"ml_magjso","table_label":"Source De-reddened J-band [mag]","description":"De-reddened brightness of the unmagnified source star, in J-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_magjsoerr1 (-) ml_magjsoerr2","limit_column":"ml_magjsolim","default":false}
{"table":"ML","database_column_name":"ml_maghs","table_label":"Source H-band [mag]","description":"Brightness of the unmagnified source star, in H-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_maghserr1 (-) ml_maghserr2","limit_column":"ml_maghslim","default":false}
{"table":"ML","database_column_name":"ml_maghso","table_label":"Source De-reddened H-band [mag]","description":"De-reddened brightness of the unmagnified source star, in H-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_maghsoerr1 (-) ml_maghsoerr2","limit_column":"ml_maghsolim","default":false}
{"table":"ML","database_column_name":"ml_magks","table_label":"Source K-band [mag]","description":"Brightness of the unmagnified source star, in K-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_magkserr1 (-) ml_magkserr2","limit_column":"ml_magkslim","default":false}
{"table":"ML","database_column_name":"ml_magkso","table_label":"Source De-reddened K-band [mag]","description":"De-reddened brightness of the unmagnified source star, in K-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_magksoerr1 (-) ml_magksoerr2","limit_column":"ml_magksolim","default":false}
{"table":"ML","database_column_name":"ml_magibase","table_label":"Event Baseline I-band [mag]","description":"Brightness of all objects, including the unmagnified source star, superposed at the time of the event, in I-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_magibaseerr1 (-) ml_magibaseerr2","limit_column":"ml_magibaselim","default":false}
{"table":"ML","database_column_name":"sy_vmag","table_label":"Lens V-band [mag]","description":"Brightness of the lens star, in V-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) sy_vmagerr1 (-) sy_vmagerr2","limit_column":"sy_vmaglim","default":false}
{"table":"ML","database_column_name":"sy_icmag","table_label":"Lens I-band [mag]","description":"Brightness of the lens star, in I-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) sy_icmagerr1 (-) sy_icmagerr2","limit_column":"sy_icmaglim","default":false}
{"table":"ML","database_column_name":"sy_jmag","table_label":"Lens J-band [mag]","description":"Brightness of the lens star, in J-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) sy_jmagerr1 (-) sy_jmagerr2","limit_column":"sy_jmaglim","default":false}
{"table":"ML","database_column_name":"sy_hmag","table_label":"Lens H-band [mag]","description":"Brightness of the lens star, in H-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) sy_hmagerr1 (-) sy_hmagerr2","limit_column":"sy_hmaglim","default":false}
{"table":"ML","database_column_name":"sy_kmag","table_label":"Lens K-band [mag]","description":"Brightness of the lens star, in K-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) sy_kmagerr1 (-) sy_kmagerr2","limit_column":"sy_kmaglim","default":false}
{"table":"ML","database_column_name":"ml_extvfld","table_label":"Line-of-sight V-Band Extinction [mag]","description":"Line-of-sight extinction toward the source system, in V-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_extvflderr1 (-) ml_extvflderr2","limit_column":"ml_extvfldlim","default":false}
{"table":"ML","database_column_name":"ml_extifld","table_label":"Line-of-sight I-Band Extinction [mag]","description":"Line-of-sight extinction toward the source system, in I-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_extiflderr1 (-) ml_extiflderr2","limit_column":"ml_extifldlim","default":false}
{"table":"ML","database_column_name":"ml_extjfld","table_label":"Line-of-sight J-Band Extinction [mag]","description":"Line-of-sight extinction toward the source system, in J-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_extjflderr1 (-) ml_extjflderr2","limit_column":"ml_extjfldlim","default":false}
{"table":"ML","database_column_name":"ml_exthfld","table_label":"Line-of-sight H-Band Extinction [mag]","description":"Line-of-sight extinction toward the source system, in H-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_exthflderr1 (-) ml_exthflderr2","limit_column":"ml_exthfldlim","default":false}
{"table":"ML","database_column_name":"ml_extkfld","table_label":"Line-of-sight K-Band Extinction [mag]","description":"Line-of-sight extinction toward the source system, in K-band","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_extkflderr1 (-) ml_extkflderr2","limit_column":"ml_extkfldlim","default":false}
{"table":"ML","database_column_name":"ml_colvis","table_label":"Source (V-I) [mag]","description":"Color of the unmagnified source star, V minus I","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_colviserr1 (-) ml_colviserr2","limit_column":"ml_colvislim","default":false}
{"table":"ML","database_column_name":"ml_mcolviso","table_label":"Source De-reddened (V-I) [mag]","description":"De-reddened color of the unmagnified source star, V minus I","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_mcolvisoerr1 (-) ml_mcolvisoerr2","limit_column":"ml_mcolvisolim","default":false}
{"table":"ML","database_column_name":"ml_colvks","table_label":"Source (V-K) [mag]","description":"Color of the unmagnified source star, V minus K","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_colvkserr1 (-) ml_colvkserr2","limit_column":"ml_colvkslim","default":false}
{"table":"ML","database_column_name":"ml_colvkso","table_label":"Source De-reddened (V-K) [mag]","description":"De-reddened color of the unmagnified source star, V minus K","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_colvksoerr1 (-) ml_colvksoerr2","limit_column":"ml_colvksolim","default":false}
{"table":"ML","database_column_name":"ml_colihs","table_label":"Source (I-H) [mag]","description":"Color of the unmagnified source star, I minus H","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_colihserr1 (-) ml_colihserr2","limit_column":"ml_colihslim","default":false}
{"table":"ML","database_column_name":"ml_colihso","table_label":"Source De-reddened (I-H) [mag]","description":"De-reddened color of the unmagnified source star, I minus H","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_colihsoerr1 (-) ml_colihoserr2","limit_column":"ml_colihsolim","default":false}
{"table":"ML","database_column_name":"ml_colhks","table_label":"Source (H-K) [mag]","description":"Color of the unmagnified source star, H minus K","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_colhkserr1 (-) ml_colhkserr2","limit_column":"ml_colhkslim","default":false}
{"table":"ML","database_column_name":"ml_colhkso","table_label":"Source De-reddened (H-K) [mag]","description":"De-reddened color of the unmagnified source star, H minus K","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_colhksoerr1 (-) ml_colhkoserr2","limit_column":"ml_colhksolim","default":false}
{"table":"ML","database_column_name":"ml_colvibl","table_label":"Blend (V-I) [mag]","description":"Combined color of all objects, excluding the source star, superposed at the time of the event, V minus I","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_colviblerr1 (-) ml_colviblerr2","limit_column":"ml_colvibllim","default":false}
{"table":"ML","database_column_name":"ml_redvi","table_label":"Line-of-sght Reddening E(V-I) [mag]","description":"Line-of-sight reddening toward the source system, E(V-I)","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_redvierr1 (-) ml_redvierr2","limit_column":"ml_redvilim","default":false}
{"table":"ML","database_column_name":"ml_redvk","table_label":"Line-of-sight Reddening E(V-K) [mag]","description":"Line-of-sight reddening toward the source system, E(V-K)","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_redvkerr1 (-) ml_redvkerr2","limit_column":"ml_redvklim","default":false}
{"table":"ML","database_column_name":"ml_redhk","table_label":"Line-of-sight Reddening E(H-K) [mag]","description":"Line-of-sight reddening toward the source system, E(H-K)","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) ml_redhkerr1 (-) ml_redhkerr2","limit_column":"ml_redhklim","default":false}
{"table":"ML","database_column_name":"ml_modelchisq","table_label":"Model Chi-squared","description":"Chi-squared of the microlens model selected as the best fit","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ML","database_column_name":"cb_flag","table_label":"Circumbinary Flag","description":"Binary flag indicating whether lens system is a stellar binary (1=yes; 0=no)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ML","database_column_name":"ml_description","table_label":"Model Description","description":"Microlensing model description and notes","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"keplernames","database_column_name":"kepid","table_label":"Kepler Identification or KepID","description":"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.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"keplernames","database_column_name":"koi_name","table_label":"KOI Name","description":"A number used to identify and track a Kepler Object of Interest (KOI). A KOI is a target identified by the Kepler Project that displays at least one transit-like sequence within Kepler time-series photometry that appears to be of astrophysical origin and initially consistent with a planetary transit hypothesis. A KOI name has an integer and a decimal part of the format KNNNNN.DD. The integer part designates the target star; the two-digit decimal part identifies a unique transiting object associated with that star. It is not necessarily the planetary candidate listed in that order within a DV report, nor does it indicate the distance of the planet from the the host star relative to other planets in the system.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true,"notes":"Previously known as kepoi_name"}
{"table":"keplernames","database_column_name":"kepler_name","table_label":"Kepler Name","description":"Kepler number name of the form \"Kepler-N\" plus a lower-case letter identifying the planet. In general, these numbers are easier to remember than the corresponding KOI or KIC/KepID designations and are intended to clearly indicate a class of objects that have been confirmed or validated as planets—a step up from the planet candidate designation.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"keplernames","database_column_name":"pl_name","table_label":"Confirmed Name","description":"The planet name as used in the Exoplanet Archive Planetary Systems tables.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true,"notes":"Previously known as alt_name"}
{"table":"keplernames","database_column_name":"koi_list_flag","table_label":"Is In KOI List?","description":"This flag indicates whether the planet is listed in the KOI candidate list (value of \"YES\") or not (value of \"NOT\"). KOI candidates are identified through transit signatures from the Kepler light curves. Follow-up observations may confirm the presence of additional planets via signatures that are not those of transiting objects, for example via Transit Timing Variations.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true,"notes":"No longer used"}
{"table":"keplernames","database_column_name":"tm_designation","table_label":"2MASS Name","description":"2MASS designation from the 2MASS point source catalog (Skrutskie et al. 2006, ApJ, 131, 1163).","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false,"notes":"No longer used"}
{"table":"keplernames","database_column_name":"last_update","table_label":"Date of Last Update","description":"Date of last update for this Kepler planet","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true,"notes":"No longer used"}
{"table":"keplernames","database_column_name":"ra","table_label":"RA (deg)","description":"KIC Right Ascension","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"ra_err","default":false,"notes":"No longer used"}
{"table":"keplernames","database_column_name":"dec","table_label":"Dec (deg)","description":"KIC Declination","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"dec_err","default":false,"notes":"No longer used"}
{"table":"keplernames","database_column_name":"ra_str","table_label":"RA (sex)","description":"KIC Right Ascension","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true,"notes":"No longer used"}
{"table":"keplernames","database_column_name":"dec_str","table_label":"Dec (sex)","description":"KIC Declination","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true,"notes":"No longer used"}
{"table":"k2names","database_column_name":"epic_id","table_label":"EPIC ID","description":"Target identification number, as listed in the Ecliptic Plane Input Catalog (EPIC).","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true,"notes":"Previously known as epic_host"}
{"table":"k2names","database_column_name":"k2_campaign (interactive table) or k2_campaign_str†(API queries)","table_label":"K2 Campaign number","description":"The K2 Campaign number for this target. Note: When constructing API queries, use k2_campaign_str. When downloading values from the interactive table, the column appears as k2_campaign. Also, E refers to the Engineering campaign in both the API and interactive table download files. (To filter on E campaigns in the interactive table, enter -1.)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true,"notes":"No longer used"}
{"table":"k2names","database_column_name":"k2_name","table_label":"K2 Name","description":"K2 number name of the form \"K2-N\" plus a lower-case letter identifying the planet. In general, these numbers are easier to remember than the corresponding EPIC designations and are intended to clearly indicate a class of objects that have been confirmed or validated as planets—a step up from the planet candidate designation.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"k2names","database_column_name":"pl_name","table_label":"Default Name","description":"The planet name as used in the Exoplanet Archive confirmed planet table.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true,"notes":"Previously known as alt_name"}
{"table":"k2names","database_column_name":"k2_kepmag","table_label":"Stellar Kepler Magnitude Value","description":"Brightness of the host star in the Kepler-band in units of magnitudes","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true,"notes":"No longer used"}
{"table":"k2names","database_column_name":"tm_designation","table_label":"2MASS Name","description":"2MASS designation from the 2MASS point source catalog (Skrutskie et al. 2006, ApJ, 131, 1163).","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true,"notes":"No longer used"}
{"table":"k2names","database_column_name":"last_update","table_label":"Date of Last Update","description":"Date of last update for this Kepler planet","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true,"notes":"No longer used"}
{"table":"k2names","database_column_name":"ra_str","table_label":"RA [decimal degrees]","description":"EPIC Right Ascension","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true,"notes":"No longer used"}
{"table":"k2names","database_column_name":"dec_str","table_label":"Dec [decimal degrees]","description":"EPIC Declination","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true,"notes":"No longer used"}
{"table":"k2names","database_column_name":"ra","table_label":"RA [decimal degrees]","description":"EPIC Right Ascension","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false,"notes":"No longer used"}
{"table":"k2names","database_column_name":"dec","table_label":"Dec [decimal degrees]","description":"EPIC Declination","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false,"notes":"No longer used"}
{"table":"emissionspec","database_column_name":"plntname","table_label":"Planet Name","description":"Planetary name most commonly used in the literature.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"emissionspec","database_column_name":"centralwavelng","table_label":"Central Wavelength [microns]","description":"Central wavelength of the emission spectroscopy observation.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"emissionspec","database_column_name":"bandwidth","table_label":"Band Width [microns]","description":"Band width of the emission spectroscopy observation.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"emissionspec","database_column_name":"especlipdep","table_label":"Eclipse Depth [percentage]","description":"The size of the relative flux decrement caused by the star transiting in front of the planet; also often referred to as the flux ratio between the planetary flux and the stellar flux.","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) especlipdeperr1 (-) especlipdeperr2","limit_column":"especlipdeplim","default":false,"displayed_string_name":"especlipdepstr"}
{"table":"emissionspec","database_column_name":"espbritemp","table_label":"Brightness Temperature [K]","description":"The temperature of a black body of the same size and flux as the exoplanet at the observed wavelength.","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) espbritemperr1 (-) espbritemperr2","limit_column":"espbritemplim","default":false,"displayed_string_name":"espbritempstr"}
{"table":"emissionspec","database_column_name":"plntreflink","table_label":"Reference","description":"Link to the refereed publication describing the emission spectroscopy observations.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"emissionspec","database_column_name":"facility","table_label":"Facility","description":"Name of the telescope used to perform the emission spectroscopy observation.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"emissionspec","database_column_name":"instrument","table_label":"Instruments","description":"Name of the instrument used to perform the emission spectroscopy observation.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"transitspec","database_column_name":"plntname","table_label":"Planet Name","description":"Planetary name most commonly used in the literature.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"transitspec","database_column_name":"centralwavelng","table_label":"Central Wavelength [microns]","description":"Central wavelength of the transmission spectroscopy observation","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"transitspec","database_column_name":"bandwidth","table_label":"Band Width [microns]","description":"Band width of the transmission spectroscopy observation","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"transitspec","database_column_name":"plntransdep","table_label":"Transit Depth [percentage]","description":"The size of the relative flux decrement caused by the orbiting body transiting in front of the star","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) plntransdeperr1 (-) plntransdeperr2","limit_column":"plntransdeplim","default":false,"displayed_string_name":"plntransdepstr"}
{"table":"transitspec","database_column_name":"plnradj","table_label":"Planet Radius [Jupiter radii]","description":"Length of a line segment from the center of the planet to its surface, measured in units of radius of Jupiter","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) plnradjerr1 (-) plnradjerr2","limit_column":"plnradjlim","default":false,"displayed_string_name":"plnradjstr"}
{"table":"transitspec","database_column_name":"plnratror","table_label":"Ratio of Planet to Stellar Radius","description":"Ratio of the radius of the orbiting body to the radius of the stellar host","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) plnratrorerr1 (-) plnratrorerr2","limit_column":"plnratrorlim","default":false,"displayed_string_name":"plnratrorstr"}
{"table":"transitspec","database_column_name":"plntranreflink","table_label":"Reference","description":"Link to the refereed publication describing the transmission spectroscopy observations","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"transitspec","database_column_name":"plntranmid","table_label":"Transit Mid-Point [BJD]","description":"The time given by the average of the time the planet begins to cross the stellar limb and the time the planet finishing crossing the stellar limb","in_ps_table":false,"in_ps_comp_pars_table":false,"uncertainties_column_positive_negative":"(+) plntranmiderr1 (-) plntranmiderr2","limit_column":"plntranmidlim","default":false,"displayed_string_name":"plntranmidstr"}
{"table":"transitspec","database_column_name":"facility","table_label":"Facility","description":"Name of the telescope used to perform the transmission spectroscopy observation","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"transitspec","database_column_name":"instrument","table_label":"Instruments","description":"Name of the instrument used to perform the transmission spectroscopy observation","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"sourceid","table_label":"Source ID","description":"Long-form ID specifiying Photometry Method, Survey Year, Galactic Bulge Region, Field ID, CCD ID, and Index of unique UKIRT light curve. Example: ukirt_c_2016_s_33_1_0065104","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"obs_year","table_label":"Survey Year","description":"UKIRT microlensing survey year (2015–2018)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"bulge","table_label":"Galactic Bulge Region","description":"Galactic bulge region: central [specified target fields of 2017–2018 surveys], or northern [2015 survey and specified target fields of 2017–2018 surveys], or southern [2016 survey and specified target fields of 2017–2018 surveys].","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"field","table_label":"Field ID","description":"UKIRT microlensing survey field ids, which are numbered as such: 2015: 11–14; 21–24; 31–34; 41–44; 5; 6 2016: 11–14; 21–24; 31–34; 41–44; 51–54; 61–64; 71–74; 81–84 2017–2018: central: 11–14; 21–24; 31–34; 41–41 northern: 11–14; 21–24; 31–34; 41–41 southern: 11–14; 21–24; 31–34; 41–41; 51–54; 61–64 For more coverage information, see the UKIRT Coverage Maps and Magnitude Ranges page.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"ccdid","table_label":"CCD ID","description":"UKIRT microlensing survey CCD number, within a given field (Range: 1–4)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"ra","table_label":"RA [decimal degrees]","description":"Right Ascension corresponding to light curve, in decimal degrees","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"dec","table_label":"Dec [decimal degrees]","description":"Declination corresponding to light curve, in decimal degrees","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"hjdstart","table_label":"Start HJD [days]","description":"Date of first point in light curve; the time system is the number of days since the Reference HJD (i.e., HJD - 2450000)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"hjdstop","table_label":"End HJD [days]","description":"Date of last point in light curve; the time system is the number of days since the Reference HJD (i.e., HJD - 2450000)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"hjd_ref","table_label":"Reference HJD [days]","description":"Reference HJD for hjdstart and hjdstop database entries (HJD = 2450000)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"h_mag","table_label":"H-band [mag]","description":"Mean H-band magnitude of light curve","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"k_mag","table_label":"K-band [mag]","description":"Mean K-band magnitude of light curve","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"npts","table_label":"Points in Light Curve","description":"Number of data points in light curve (i.e., number of epochs that are not \"null\")","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"k2c9_flag","table_label":"K2 Campaign 9 Field Overlap Flag","description":"Binary flag indicating whether given light curve was observed by K2 during its Campaign 9 microlensing survey (1 = yes; 0 = no)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"ukirt_evt_flag","table_label":"UKIRT Event Flag","description":"Binary flag indicating whether given light curve was identified as a possible microlensing event by the UKIRT Microlensing Team event detection pipeline (1 = yes; 0 = no)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"ukirt_id","table_label":"UKIRT Event ID","description":"UKIRT microlensing event ID (Null unless UKIRT Event Flag = 1)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"ogle_evt_flag","table_label":"OGLE Event Flag","description":"Binary flag indicating whether given light curve matches to a microlensing event identified by the OGLE-IV Early Warning System for the corresponding survey year (1 = yes; 0 = no)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"ogle_id","table_label":"OGLE Event ID","description":"OGLE-IV microlensing event ID (Null unless OGLE Event Flag = 1)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"moa_evt_flag","table_label":"MOA Event Flag","description":"Binary flag indicating whether given light curve matches to a microlensing event identified by the MOA-II Transient Alert for the corresponding survey year (1 = yes; 0 = no)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"moa_id","table_label":"MOA Event ID","description":"MOA-II microlensing event ID (Null unless MOA Event Flag = 1)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"statnpts","table_label":"Points in Statistics Calculation","description":"Number of points used in statistics calculations","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"minvalue","table_label":"Minimum Value of Light Curve [mag]","description":"Minimum magnitude value of light curve (i.e., the brightest data point)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"maxvalue","table_label":"Maximum Value of Light Curve [mag]","description":"Maximum magnitude value of light curve (i.e., the faintest data point)","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"mean","table_label":"Mean Value of Light Curve [mag]","description":"Mean magnitude value of light curve","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"stddevwrtmean","table_label":"Std Dev of Light Curve wrt Mean [mag]","description":"Standard deviation with respect to mean magnitude of light curve","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"median","table_label":"Median of Light Curve [mag]","description":"Median magnitude value of light curve","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"stddevwrtmed","table_label":"Std Dev of Light Curve wrt Median [mag]","description":"Standard deviation with respect to median magnitude of light curve","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"n5sigma","table_label":"Number of Points > 5 Sigma from Median","description":"Number of points further than 5 standard deviations from the light curve median magnitude","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"f5sigma","table_label":"Fraction of Points > 5 Sigma from Median","description":"Fraction of points further than 5 standard deviations from the light curve median magnitude","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"medabsdev","table_label":"Median Absolute Deviation of Light Curve [mag]","description":"Median absolute deviation of light curve","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"chisquared","table_label":"Reduced Chi-squared of Light Curve","description":"Reduced chi-squared of light curve with respect to the median magnitude","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"ukirttimeseries","database_column_name":"range595","table_label":"5–95% Range of Light Curve [mag]","description":"5–95 percentile range of light curve","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"kelttimeseries","database_column_name":"kelt_sourceid","table_label":"Source ID","description":"KELT Object Identification","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"kelttimeseries","database_column_name":"kelt_field","table_label":"Survey Field","description":"KELT field of observation. Fields available are N02, N04, N06, N08, N10 and N12","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"kelttimeseries","database_column_name":"kelt_orientation","table_label":"Field Orientation","description":"KELT field orientation; either \"east\" or \"west.\"","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"kelttimeseries","database_column_name":"proc_type","table_label":"Processing","description":"KELT timeseries processing; either \"raw\" or \"tfa.\"","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"kelttimeseries","database_column_name":"ra","table_label":"RA [decimal degrees]","description":"Right Ascension of the target in decimal degrees","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"kelttimeseries","database_column_name":"dec","table_label":"Dec [decimal degrees]","description":"Declination of the target in decimal degrees","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"kelttimeseries","database_column_name":"bjdstart","table_label":"Start BJD [days]","description":"Date of first point in light curve Barycentric Julian Date. For N02, timestamps are in approximate BJD where the correction for the field center to edge difference has not been applied. This correction has a maximum value of 30 seconds, but is typically of order 1-5 seconds. For N04, the timestamps are JD_TT, not BJD.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"kelttimeseries","database_column_name":"bjdstop","table_label":"End BJD [days]","description":"Date of last point in light curve in Barycentric Julian Date. For N02, timestamps are in approximate BJD where the correction for the field center to edge difference has not been applied. This correction has a maximum value of 30 seconds, but is typically of order 1-5 seconds. For N04, the timestamps are JD_TT, not BJD.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"kelttimeseries","database_column_name":"obsstart","table_label":"Calendar Start Time","description":"Calendar Date time-stamp of first point in light curve","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"kelttimeseries","database_column_name":"obsstop","table_label":"Calendar End Time","description":"Calendar Date time-stamp of last point in light curve","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"kelttimeseries","database_column_name":"kelt_mag","table_label":"Magnitude [mag]","description":"Instrumental KELT magnitude","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"kelttimeseries","database_column_name":"npts","table_label":"Points in Statistics Calculation","description":"Number of points used in statistics","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"kelttimeseries","database_column_name":"minvalue","table_label":"Minimum Value of Time Series [mag]","description":"Minimum value of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"kelttimeseries","database_column_name":"maxvalue","table_label":"Maximum Value of Time Series [mag]","description":"Maximum value of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"kelttimeseries","database_column_name":"mean","table_label":"Mean Value of Time Series [mag]","description":"Mean value of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"kelttimeseries","database_column_name":"stddevwrtmean","table_label":"Std Dev of Time Series wrt Mean [mag]","description":"Standard deviation with respect to mean of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"kelttimeseries","database_column_name":"median","table_label":"Median value of Time Series [mag]","description":"Median value of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"kelttimeseries","database_column_name":"stddevwrtmedian","table_label":"Std Dev of Time Series wrt Median [mag]","description":"Standard deviation with respect to median of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"kelttimeseries","database_column_name":"n5sigma","table_label":"Number of points > 5 sigma from median","description":"Number of points further than 5 standard deviations from the magnitude time series median","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"kelttimeseries","database_column_name":"f5sigma","table_label":"Fraction of points > 5 sigma from median","description":"Fraction of points further than 5 standard deviations from the magnitude time series median","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"kelttimeseries","database_column_name":"medabsdev","table_label":"Median Absolute Deviation of Time Series [mag]","description":"Median absolute deviation of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"kelttimeseries","database_column_name":"chisquared","table_label":"Reduced Chi-Squared of Time Series","description":"Reduced chi-squared of the magnitude time series with respect to the median","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"kelttimeseries","database_column_name":"range595","table_label":"5-95% Range of Time Series [mag]","description":"5-95 percentile range of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":true}
{"table":"superwasptimeseries","database_column_name":"sourceid","table_label":"Source ID","description":"SuperWASP Object ID","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"ra","table_label":"RA [decimal degrees]","description":"Right Ascension of the target in decimal degrees","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"dec","table_label":"Dec [decimal degrees]","description":"Declination of the target in decimal degrees","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"hjdstart","table_label":"Start HJD_UTC [days]","description":"Date of first point in light curve. The time system is the number of days since a Heliocentric Julian Date relative to the reference HJD_UTC.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"hjdstop","table_label":"End HJD_UTC [days]","description":"Date of last point in light curve. The time system is the number of days since a Heliocentric Julian Date relative to the reference HJD_UTC.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"hjd_ref","table_label":"Reference HJD_UTC [days]","description":"Reference HJD_UTC for the hjdstart and end_time database entries.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"obsstart","table_label":"Calendar Start Time","description":"Calendar Date time-stamp of first point in light curve.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"obsstop","table_label":"Calendar End Time","description":"Calendar Date time-stamp of last point in light curve.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"tstart","table_label":"Start Time","description":"Time in seconds of the first point in light curve since the reference HJD_UTC.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"tstop","table_label":"Stop Time","description":"Time in seconds of the last point in light curve since the reference HJD_UTC.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"wasp_mag","table_label":"WASP-band [mag]","description":"Apparent magnitude of the target in the WASP bandpass - CCD White light in first year, and a broadband 400-700 nm filter thereafter.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"npts","table_label":"Points in Light Curve","description":"Number of data points in light curve. Must be at least one.","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"tile","table_label":"Survey Tile","description":"Subdivision of DR1 targets for survey processing","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"tm_statnpts","table_label":"Points in Statistics Calculation","description":"Number of points used in statistics calculations","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"tm_minvalue","table_label":"Minimum Value of Time Series","description":"Minimum value of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"tm_maxvalue","table_label":"Maximum Value of Time Series","description":"Maximum value of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"tm_mean","table_label":"Mean Value of Time Series","description":"Mean value of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"tm_stddevwrtmean","table_label":"Std Dev of Time Series wrt Mean","description":"Standard deviation with respect to mean of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"tm_median","table_label":"Median value of Time Series","description":"Median value of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"tm_stddevwrtmed","table_label":"Std Dev of Time Series wrt Median","description":"Standard deviation with respect to median of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"tm_n5sigma","table_label":"Number of points > 5 sigma from median","description":"Number of points further than 5 standard deviations from the magnitude time series median","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"tm_f5sigma","table_label":"Fraction of points > 5 sigma from median","description":"Fraction of points further than 5 standard deviations from the magnitude time series median","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"tm_medabsdev","table_label":"Median Absolute Deviation of Time Series","description":"Median absolute deviation of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"tm_chisquared","table_label":"Reduced Chi-Squared of Time Series","description":"Reduced chi-squared of the magnitude time series with respect to the median","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}
{"table":"superwasptimeseries","database_column_name":"tm_range595","table_label":"5-95% Range of Time Series","description":"5-95 percentile range of magnitude time series","in_ps_table":false,"in_ps_comp_pars_table":false,"default":false}