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.
ARCHES - Astronomical Resource Cross-matching for High Energy Studies
Description:
Each of the archival catalogues used for the crossmatch is referenced by single letter: 3XMM: x, Galex: g, UCAC:u CMC: c, SDSS: s, UKIDSS LAS: l, KIDS GPS: k ALLWISE; w AKARI: a and FIRST_NVSS_COMBO: r
ARCHES - Astronomical Resource Cross-matching for High Energy Studies
Description:
The enhanced 3XMM catalogue (designated 3XMMe) is one of the core elements of the Arches project, representing the X-ray source basis for the cross-correlations with other multi-wavelength catalogues. The 3XMMe catalogue is a derivative of the latest increment of the 3XMM catalogue, i.e. 3XMM-DR5, that was publicly released in April 2015 (Rosen et al., 2015 (submitted to A&A)), tailored for the purposes of the Arches project. The 3XMM-DR5 catalogue, available from the XMM-Newton Science Archive, the XMM-Newton Survey Science Centre (SSC) and other sites listed on the SSC site, contains 565962 detections arising from 396910 unique sources drawn from 7781 XMM observations. These numbers include detections from 356 sub-pointings made in mosaic
Armenian Virtual Observatory SIAP API service gives possibility to make a SIAP http request to ArVO astronomical database, which contains the data gained by Byurakan Observatory. The main part of ArVO astronomical data is the First Byurakan Survey (FBS), which is the largest and the first systematic objective prism survey of the extragalactic sky. It covers 17,000 sq.deg. in the Northern sky together with a high galactic latitudes region in the Southern sky.
Amenian Virtual Observatory (ArVO) is a project of the Byurakan Astrophysical Observatory (BAO) and the Institute for Informatics and Automation Problems (IIAP) of National Academy of Science of the Republic of Armenia (NAS RA) aimed at construction of a modern system for data archiving, extraction, acquisition, correlation, reduction, use and publication. ArVO is based on the Digitized First Byurakan Survey (DFBS) and is the Armenian contribution to the International Virtual Observatory Alliance (IVOA).