The IAP - DaCHS Services'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 cpstasm schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the thmsm schema, epn_core from the thmwp3 schema.
IDOC: Integrated Data and Operating Center TAP service
Short Name:
IDOC TAP
Date:
16 Nov 2023 16:51:52
Publisher:
IDOC
Description:
The IDOC: Integrated Data and Operating Center'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 eit_syn schema, epn_core from the gaia_dem schema, epn_core from the omega_cubes schema, epn_core from the omega_maps schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema.
INAF IA2 TAP service dedicated to projects and surveys that are
not direct outcome of IA2 managed observatory/telescope archival
efforts.
Currently serving Exo Mer-Cat.
The INAF-OATs VESPA Data Service Hub'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 artecs schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema.
WFAU, Institute for Astronomy, University of Edinburgh
Description:
The Infrared Astronomical Satellite Archive is an implementation of the IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986). This is a catalogue of some 250,000 well-confirmed infrared point sources observed by the Infrared Astronomical Satellite, i.e., sources with angular extents less than approximately 0.5, 0.5, 1.0, and 2.0 arcmin in the in-scan direction at 12, 25, 60, and 100 microns, respectively.
This service provides access to tables and catalogues of the ISO ESA mission.
The Infrared Space Observatory (ISO) was the world's first true orbiting infrared observatory. Equipped with four highly-sophisticated and versatile scientific instruments, it was launched by Ariane in November 1995 and provided astronomers world-wide with a facility of unprecedented sensitivity and capabilities for a detailed exploration of the Universe at infrared wavelengths. The two spectrometers (SWS and LWS), a camera (ISOCAM) and an imaging photo-polarimeter (ISOPHOT) jointly covered wavelengths from 2.5 to around 240 microns with spatial resolutions ranging from 1.5 arcseconds (at the shortest wavelengths) to 90 arcseconds (at the longer wavelengths). Its 60 cm diameter telescope was cooled by superfluid liquid helium to temperatures of 2-4 K.
