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Wide-Field Spectroscopy - Proceedings of the 2nd Conference of the Working Group of IAU Commission 9 on "Wide-Field Imaging" held in Athens, Greece, May 20-25, 1996 (Paperback, Softcover reprint of the original 1st ed. 1997)
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Wide-Field Spectroscopy - Proceedings of the 2nd Conference of the Working Group of IAU Commission 9 on "Wide-Field Imaging" held in Athens, Greece, May 20-25, 1996 (Paperback, Softcover reprint of the original 1st ed. 1997)
Series: Astrophysics and Space Science Library, 212
Expected to ship within 10 - 15 working days
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E. KONTIZAS Astronomical Institute National Observatory of Athens
P. O. Box 20048 Athens GR-1181O GREECE The international conference
on "Wide-Field Spectroscopy" and its sub ject matter were agreed
during the general assembly of the International Astronomical Union
(IAU) in August 1994 by the Working Group of Com mision 9 "Wi
de-Field Imaging". This meeting gave an opportunity to world
experts on this subject to gather in Athens, in order to discuss
the cur rent exploitation and the impending opportunities that
exist in the area of multi-object spectroscopy, with particular
emphasis on: 1. Astronomical instruments, data acquisition,
processing and analysis techniques. 2. Astrophysical problems best
tackled through wide-field, multi-object spectroscopy. The new
fibre optic technology offers an important tool for the advancement
of basic research and the development of industrial applications.
Astronom ical spectroscopy is a field of astronomy which has
contributed much to the advancement of fundamental physics. The
spectra of hot stars have been used to determine the well-known
Balmer formula for the wavelength of hydrogen lines, in the late
19th century. Since then, spectroscopy has made enormous progress
in stellar atmosphere studies, in kinematics, and in the detection
of high redshifts in the Universe. The traditional techniques of
obtaining wide-field spectroscopic data are based on slitless
spectroscopy (objective prism). Several observations, world wide,
make use ofthese tech niques in order to obtain information on the
spectral properties of objects in large areas of the sky.
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