The PADC TAP Server on voparis-tap-planeto.obspm.fr's TAP end point. The Table Access
Protocol (TAP) lets you execute queries against our database tables,
inspect various metadata, and upload your own data. It is thus the
VO's premier way to access public data holdings.Tables exposed through this endpoint include: epn_core from the apis schema, epn_core from the basecom schema, epn_core, observatories from the bdip schema, epn_core from the crism_speclib schema, epn_core from the dynastvo schema, epn_core from the exoplanet schema, epn_core from the gmap schema, epn_core from the hst_planeto schema, epn_core from the iks schema, epn_core from the lunar_craters schema, epn_core from the m4ast schema, epn_core from the mars_craters schema, epn_core from the mars_craters_lagain schema, epn_core from the mercury_craters schema, epn_core from the meteor_showers schema, epn_core from the moonsprop schema, epn_core from the planets schema, epn_core from the spectro_asteroids schema, epn_core from the spectro_m_ast schema, epn_core from the spectro_planets schema, epn_core from the spectro_stars schema, epn_core from the spectro_trojans schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the titan_profiles schema, epn_core from the tnosarecool schema, epn_core from the usgs_wms schema, epn_core from the venus_craters schema, epn_core from the vims_satellites schema, epn_core from the vir_ros schema, epn_core from the voccdb schema, epn_core from the vros_geocor schema, epn_core from the vvex schema.
To locate columns "by physics", as it were, use UCD in
↗tap_schema.columns. For instance,
to find everything talking about the mid-infrared about 10µm, you
could write:
SELECT * FROM tap_schema.columns
WHERE description LIKE '%em.IR.8-15um%'