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The Calar Alto Deep Imaging Survey

Published online by Cambridge University Press:  25 May 2016

H. Hippelein ,
S. Beckwith ,
R. Fockenbrock ,
J. Fried ,
U. Hopp ,
C. Leinert ,
K. Meisenheimer ,
H.-J. Röser ,
E. Thommes  and
C. Wolf
H. Hippelein
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg
S. Beckwith
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg
R. Fockenbrock
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg
J. Fried
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg
U. Hopp
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg
C. Leinert
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg
K. Meisenheimer
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg
H.-J. Röser
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg
E. Thommes
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg
C. Wolf
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg

Extract

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The Calar Alto Deep Imaging Survey (CADIS) combines deep multicolor imaging in broad and narrow band filters with deep probing in several selected wavelength intervals through a Fabry-Pérot (FP) interferometer with a spectral resolution of ∼450.

Type
Part 5. Extra-Galactic Astronomy
Information
Symposium - International Astronomical Union , Volume 179: New Horizons from Multi-Wavelength Sky Surveys , 1998 , pp. 293 - 295
Copyright
Copyright © Kluwer 1998 

References

Thommes, & Meisenheimer, 1994, Galaxies in the Young Universe, p.242.Google Scholar