It has a Cassegrain telescope in its single dome.

The design was largely superseded by the Cassegrain telescope.

It is a modified form of a Cassegrain telescope, with light reflected sideways before reaching the primary mirror again.

The final dome to be erected contains a 1 m Cassegrain telescope, the largest and most modern of the observatory's telescopes.

It hosted a single 60 cm Cassegrain telescope and a small cottage for the operators, located amongst the instruments funded by other organizations.

As in the Cassegrain telescope, the light falls on a concave primary mirror, then is rejected towards a convex secondary mirror.

There is evidence that Laurent Cassegrain was the obscure namesake of the Cassegrain telescope.

The observatory has one 0.6 metre Cassegrain telescope along with a photometer and a CCD camera.

The QMax, a portable solar spectrometer built to fit their line of Maksutov Cassegrain telescopes.

The building incorporated a polar Cassegrain telescope, a transit telescope (no longer functional), a solar telescope, and a sundial, on the south wall.

DFM makes medium size Cassegrain telescopes and their associated systems including telescope optics, control systems, and mounts.

Soon afterwards, a C14 Schmidt Cassegrain telescope was added, along with CCD imaging equipment.

In 1980 the General Electric company donated the Boller and Chivens 16" Cassegrain telescope.

The CZCS used a rotating plane mirror at a 45 degree angle to the optic axis of a Cassegrain telescope.

The imaging system, the Television Photography Experiment, consisted of two 15 cm (5.9") Cassegrain telescopes feeding vidicon tubes.

The outdoor Flandrau Observatory has free viewing through its 16-inch Cassegrain telescope on Wednesday through Saturday nights from 7 to 10.

First, the members constructed a 12.5" Dall-Kirkham Cassegrain telescope to place in the new observatory, then they attempted to purchase a plot of land for $1000 dollars.

Grants from the Sherman Fairchild and National Science foundations helped pay for the Cassegrain telescope, other astronomical equipment and computers for the observatory.

The observatory started out with a single 15 cm Cassegrain telescope, then added on an 60 cm Cassegrain telescope in 1965.

The Argunov Cassegrain telescope is a catadioptric telescope design first introduced in 1972 by P. P. Argunov.

The Cassegrain telescope (sometimes called the "Classic Cassegrain") was first published in an 1672 design attributed to Laurent Cassegrain.

It consists of a dome, library, 41cm Newtonian telescope, a meeting hall seating 100 people, and a roll-off roof observatory with a 35cm Schmidt Cassegrain Telescope.

The Cassegrain antenna design was adapted from the Cassegrain telescope, a type of reflecting telescope developed around 1672 and attributed to French priest Laurent Cassegrain.

The optics of CTX consist of a 350 mm focal length Maksutov Cassegrain telescope with a 5,064 pixel wide line array CCD.

The main optic of SWAS is a 55 cm x 71 cm elliptical off-axis Cassegrain telescope, sending light into a pair of Schottky diode receivers.