Astron. Astrophys. Suppl. Ser. 130, 395-401
S. Morel - L. Koechlin
Send offprint request: S. Morel
Laboratoire d'Astrophysique de Toulouse,
Observatoire Midi-Pyrénées,
14 avenue Édouard Belin, F-31400 Toulouse, France
e-mail: morel@obs-mip.fr
Received June 18; accepted December 17, 1997
In this paper we present new ideas for a high
sensitivity array detector, which yields the space and time
coordinates of photo-events at sustained count rates superior to
one million per second. The DELTA camera (Detector Enhancement by Linear-projections on
Three Axes) has been initially designed for astronomy.
However, it has advantages for a wide range of high-resolution
problems in the visible and near I.R. It is noticeable for its
optical design, its smooth flat field and its very high temporal
resolution and throughput in photon counting mode. The resolution
of the prototype described is pixels in space
and 2.6
s in time.
The principle of this detector is based on a projection -
back-projection scheme (the
-process) and on the use of
three one-dimensional CCDs. We describe the technical solutions
which could lead to an operational prototype. From numerical
simulations of the
-process, we give some expected
characteristics of this camera.
Key words: instrumentation: detectors -- techniques: interferometric
Copyright The European Southern Observatory (ESO)