This database provides access to IDOC catalogues and complementary information on clusters of galaxies observed through the Sunyaev-Zeldovich (SZ) effect.
The AMIGA project is an international collaboration. The core team is
located in Granada, while researchers from different centers collaborate
in the project at different levels. We are producing and analysing a
multiwavelength database for a refinement of the pioneering Catalog of
Isolated Galaxies (CIG: Karachentseva 1973; n = 1050 galaxies) including
optical, IR and radio line and continuum measures in order to
characterise all phases of the ISM.
The Australian National University Supercomputer Facility
Short Name:
ANUSF
Date:
19 Jun 2019 15:50:33
Publisher:
The Australian National University Supercomputer Facility
Description:
The Australian National University Supercomputer Facility hosts several astronomy data archives and maintains interfaces and services which make this data available publicly. Some of these services conform to IVOA Virtual Observatory specifications and standards.
Founded in 1956, the NRAO provides state-of-the-art radio telescope facilities for use by the international scientific community. NRAO telescopes are open to all astronomers regardless of institutional or national affiliation. Observing time on NRAO telescopes is available on a competitive basis to qualified scientists after evaluation of research proposals on the basis of scientific merit, the capability of the instruments to do the work, and the availability of the telescope during the requested time. NRAO also provides both formal and informal programs in education and public outreach for teachers, students, the general public, and the media. The NRAO is funded by the National Science Foundation (NSF) under the terms of a cooperative agreement between the NSF and Associated Universities, Inc. (AUI), a science management corporation.
VOPSAT is a set of southern sky digital surveys based on ESO-R, SRC-J and POSS1-E atlases. The plates have been digitized with the MAMA microdensitometer with a resolution of 0.7 arc-sec. Pixel resampling will allow mosaicing neighbouring Schmidt fields up to hundreds of square degrees.