Very wide field camera

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Observatories, Nebulae, Ultraviolet Photometry, Ultraviolet Radiation, Ultraviolet Spectroscopy, Ultraviolet Telescopes, All Sky Photography, Astronomical Spectroscopy, Galaxies, Optical Equipment, Spacelab Payloads, Ultraviolet Photography, Wide Angle Lenses

Scientific paper

The study of galactic and faint extragalactic extended sources and peculiar ultraviolet objects by a very wide field of view camera, operated in the ultraviolet photometric and spectrometric modes is discussed. The photometric mode is direct photography through filters for observation of the following sources: (1) large scale distribution of ultraviolet radiation in the Milky Way; (2) diffusion of the galactic light above the galactic plane and in front of the large absorbing clouds; (3) the optical emission of the interstellar matter; (4) stars, and starlike objects with diameters less than 3 arc minutes. In the spectrometric mode (nebular spectrograph) the light from the center of the photometric field is concentrated on a slit covering 10 degrees by 10 arc minutes on the sky.

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