SAMP is a messaging protocol that enables astronomy software tools
to interoperate and communicate. IVOA members have recognised
that building a monolithic tool that attempts to fulfil all the
requirements of all users is impractical, and it is a better use of
our limited resources to enable individual tools to work together
better. One element of this is defining common file formats for the
exchange of data between different applications. Another important
component is a messaging system that enables the applications to
share data and take advantage of each other's functionality. SAMP
supports communication between applications on the desktop and in
web browsers, and is also intended to form a framework for more
general messaging requirements.
SkyBoT is a VO service which allows to seek and identify solar system objects (planet, satellites, asteroids, comets) in any field of view at a given epoch (cone-search method). It provides also a solar system object name resolver which convert the name or the designation of solar system objects into their celestial coordinates at a given epoch (resolver method). The SkyBoT service are available through a Web interface and a Web service (SOAP+WSDL+HTTP) which implements the IVOA Simple Cone-Search protocol.
SkyBoT is a VO service which allows to seek and identify solar system objects (planet, satellites, asteroids, comets) in any field of view at a given epoch (cone-search method). It provides also a solar system object name resolver which convert the name or the designation of solar system objects into their celestial coordinates at a given epoch (resolver method). The SkyBoT service are available through a Web interface and a Web service (SOAP+WSDL+HTTP) which implements the IVOA Simple Cone-Search protocol.
The Australian National University Supercomputer Facility
Description:
The HIPASS Project Data Archive.
The acquisition of HI Parkes All Sky Survey (HIPASS) southern sky data commenced at the Australia Telescope National Facility's Parkes 64-m telescope in 1997 February, and was completed in 2000 March. HIPASS is the deepest HI survey yet of the sky south of declination +2°, and is sensitive to emission out to 170 h75-1 Mpc.
Ultimately all types in a VO-DML model are defined as hierarchies
of primitive types. This Model defines a special, predefined model
that contains a set of the most common of such types: integer,
real, string etc. This
UKIDSS DR10 - UKIRT Infrared Deep Sky Survey Data Release 10
Date:
12 Dec 2014 11:22:23
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)
