Multiwavelength astronomy using ESIS

Details Multiwavelength astronomy using ESIS Multiwavelength astronomy using ESIS

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13..621g&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 13, no. 12, p. (12)621-(12)625

Astronomy and Astrophysics

Astronomy

Aerospace Sciences, Data Bases, Information Systems, Infrared Astronomy, Light (Visible Radiation), Radio Astronomy, Ultraviolet Astronomy, X Ray Astronomy, Active Galactic Nuclei, Astronomical Catalogs, European Space Agency, Exosat Satellite, Heao 2, Imagery, Infrared Astronomy Satellite, Iue, Seyfert Galaxies, Spectral Energy Distribution, Spectrograms

Scientific paper

We present results on multi-frequency astronomy obtained using the European Space Information System (ESIS). ESIS is an ESA service designed to access, manipulate and combine archival data from a number of remote archives in the fields of Astronomy and Space Physics. The examples presented here include plots of radio-to-X-ray energy distribution of Active Galactic Nuclei, spectrograms of IUE/UV data, direct comparison of images from different experiments and overlay of catalogue sources on image data. The ESIS project is currently reaching the end of its pilot phase. Its services will be available to the general astronomical community in 1993.

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