Content Level: Research / Capability Type: Custom Service

ID:: ivo://vopdc.obspm/lerma/simrepo
Title:: SimDAL Repository
Short Name:: SimDAL Repo
Date:: 10 Jan 2017
Publisher:: Paris Astronomical Data Centre - LERMA
Description:: The SimDAL repository hosts numerical projects descriptions as standard XML documents following the Simulation Data Model serialization xsd. It allows clients to search (fulltext) for simulation projects or associated protocols of interest and get URIs towards other SimDAL components: SimDAL Search and SimDAL Data Access.

ID:: ivo://svo.cab/simdal/repository-iso
Title:: SimDAL Repository service for isochrones and evolutionary tracks
Short Name:: Isochrones
Date:: 14 Mar 2019 08:14:12
Publisher:: SVO CAB
Description:: SimDAL repository for collections of isochrones and evolutionary tracks.

ID:: ivo://svo.cab/simdal/search/ames-cond
Title:: SimDAL Search service for AMES-cond isochrones and evolutionary tracks
Short Name:: AMES-cond iso
Date:: 14 Mar 2019 08:14:12
Publisher:: SVO CAB
Description:: SimDAL search service for AMES-cond isochrones and evolutionary tracks. Dust in equilibrium with gas phase, with dust opacities ignored, (only GNS1993 available) valid for Teff smaller than 1400 K

ID:: ivo://svo.cab/simdal/search/ames-dusty
Title:: SimDAL Search service for AMES-dusty isochrones and evolutionary tracks
Short Name:: AMES-dusty iso
Date:: 14 Mar 2019 08:14:12
Publisher:: SVO CAB
Description:: SimDAL search service for AMES-dusty isochrones and evolutionary tracks. Dust in equilibrium with gas phase, (only GNS1993 available) valid for Near-IR studies with Teff larger than 1700 K

ID:: ivo://purx/simg/simg-hipsmaster
Title:: simg.de HiPS Service (master server)
Short Name:: simg hipsmaster
Date:: 28 Sep 2024 11:48:00
Publisher:: simg.de
Description:: Selected results from the Northern Sky Narrowband Survey via HiPS protocol

ID:: ivo://nasa.heasarc/hips/server
Title:: SkyView HiPS Server
Short Name:: SkyView_HiPS
Date:: 29 Mar 2021
Publisher:: NASA/GSFC HEASARC
Description:: The SkyView service at the NASA HEASARC archive has deveoped HiPS data for the combined Swift UVOT and XRT observations covering 2005-mid 2017. Counts, Exposure and Intensity maps are provided for both instruments and for the UVOT are provided in both seven individual filters and two combined color images. This is a service provided by NASA HEASARC.

ID:: ivo://mssl.ucl.ac.uk/solarimg_dsa/solarimg
Title:: Solar Image Data for EIT CDS and Yohkoh
Date:: 11 Aug 2009 14:38:28
Publisher:: Mullard Space Science Laboratory
Description:: Catalogues of solar observations held at MSSL/UCL. Datasets available are SOHO CDS, SOHO EIT, Yohkoh SXT. URL links to data files are provided (EIT data files provided by SDAC, NASA). Reference: http://www.mssl.ucl.ac.uk/www_solar/surfindex.html

ID:: ivo://sao.ru/dsa-cats/wsdb
Title:: Special Astrophysical Observatory of RAS (SAO RAS) DSA-Catalogs Service
Date:: 14 Aug 2019 16:16:36
Publisher:: Special Astrophysical Observatory of RAS (SAO RAS)
Description:: The published catalogs of Special Astrophysical Observatory of RAS (SAO RAS)

ID:: ivo://wfau.roe.ac.uk/ssa-dsa
Title:: SuperCOSMOS Science Archive (SSA)
Short Name:: SuperCOSMOS
Date:: 23 Jan 2024 09:44:26
Publisher:: WFAU, Institute for Astronomy, University of Edinburgh
Description:: The SuperCOSMOS data held in the SSA primarily originate from scans of Palomar and UK Schmidt blue, red and near-IR southern sky surveys. The ESO Schmidt R (dec < -17.5) and Palomar POSS-I E (dec > -17.5) surveys have also been scanned and provide a 1st epoch red measurement. Further details on the surveys, the scanning process and the raw parameters extracted can be found on the further information link. The SSA is housed in a relational database running on Microsoft SQL Server 2000. Data are stored in tables which are inter-linked via reference ID numbers. In addition to the astronomical object catalogues these tables also contain information on the plates that were scanned, survey field centres and calibration coefficients. Most user science queries will only need to access the SOURCE table or to a lesser extent the DETECTION table.

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