The The VO @ ASTRON's sitewide SIAP version 2 service
publishes all the images published through the site. For more advanced
queries including uploads, all this data is also available through
ObsTAP.
The The VO @ ASTRON'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: main from the lbcs schema, main, msssvf_img_main from the mvf schema, frb_det, frb_obs from the arts_dr1 schema, img_main, main from the lofartier1 schema, mosaic, source_catalog from the lolss schema, frb_det, frb_obs from the arts_dr2 schema, main from the svc schema, img_main, main from the tgssadr schema, main, mom0 from the sauron schema, images, source_catalog from the apertif_dr_bootes schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, hetdex_images, main, main_merged from the hetdex schema, img_main from the msss schema, obscore from the ivoa schema, beam_cubes, calibrated_visibilities, continuum_images, flux_cal_visibilities, pol_cal_visibilities, pol_cubes, raw_visibilities, source_catalog, spectral_cubes from the apertif_dr1 schema, main_gausses, main_sources, mosaics from the lotss_dr2 schema.
This service provides oscillator strengths and transition
probabilities. Mainly based on experimental energy levels, these were
calculated with the pseudo-relativistic Hartree-Fock method including
core-polarization corrections.
WFAU, Institute for Astronomy, University of Edinburgh
Description:
The Two Micron All Sky Survey (2MASS) will provide a uniform survey of the entire sky at three near-infrared wavebands: J(lambdaeff = 1.25 micrometers), H(lambdaeff = 1.65 micrometers), and Ks(lambdaeff = 2.16 micrometers). A major goal of the survey is to probe large scale structures in the Milky Way and in the Local Universe, exploiting the relatively high transparency of the interstellar medium in the near-infrared, and the high near-infrared luminosities of evolved low- and intermediate-mass stars.Home page at http://pegasus.phast.umass.edu/
The UCD resolver uses the metadata in the current
Registry to suggest UCDs pertinent to natural language column descriptions.
In that, it fulfills a similar function as the `CDS UCD builder`_
but uses an entirely different approach.
.. _CDS UCD builder: http://cdsweb.u-strasbg.fr/UCD/cgi-bin/descr2ucd
WFAU, Institute for Astronomy, University of Edinburgh
Description:
This DSA hosts data release 2 of the UKIRT Hemisphere Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. The UHS provides continuous J and K-band coverage in the northern hemisphere from a declination of 0 deg to 60 deg.
UKIDSS DR10 - UKIRT Infrared Deep Sky Survey Data Release 10
Short Name:
UKIDSS DR10
Date:
04 Dec 2019 13:39:25
Publisher:
WFAU, Institute for Astronomy, University of Edinburgh
Description:
This DSA hosts data release 10 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. This catalog contains WFCAM data primarily originating from four of the five UKIDSS surveys: Large Area Survey, Galactic Clusters Survey, Deep Extragalactic Survey, and Ultra Deep Survey. (see www.ukidss.org for survey descriptions)
