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The Calar Alto Deep Imaging Survey: First Results

Published online by Cambridge University Press:  25 May 2016

E. Thommes ,
K. Meisenheimer ,
R. Fockenbrock ,
H. Hippelein  and
H.-J. Röser
E. Thommes
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg, Germany
K. Meisenheimer
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg, Germany
R. Fockenbrock
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg, Germany
H. Hippelein
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg, Germany
H.-J. Röser
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg, Germany

Extract

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The Calar Alto Deep Imaging Survey (CADIS) is a very deep emission line survey using a Fabry-Pérot (FP), combined with deep broad- and medium-band photometry (for an overview see Hippelein et al. 1996). This survey is specifically designed to detect primeval galaxies, but it will in addition produce a large data base for investigations of faint galaxies at intermediate redshifts (0.2 < z < 1.2). We present some first results from the initial data recorded with the CADIS strategy.

Type
Part 5. Extra-Galactic Astronomy
Information
Symposium - International Astronomical Union , Volume 179: New Horizons from Multi-Wavelength Sky Surveys , 1998 , pp. 296 - 298
Copyright
Copyright © Kluwer 1998 

References

Colles, et al., 1996, to appear in The Early Universe with the VLT, proceedings of ESO-workshop held in Garching bei München, Springer, Berlin, Heidelberg, New York, pp. 87.Google Scholar
Hippelein, et al. 1996, this volume, 293.Google Scholar