Crossed Dragone
The Crossed Dragone Telescope is an off-axis telescope design consisting of a parabolic primary mirror and a large concave secondary mirror arranged so that the focal plane is at right angles to the incoming light. In this configuration the polarization of light is preserved through the optics.
Other advantages of this design are a large field of view in a compact volume. Due to its off-axis nature the secondary mirror does not block any of the incoming light. At millimeter and submillimeter wavelengths this greatly decreases systematic effects due to diffraction. The main disadvantage is that the size of the secondary mirror is of similar size to the primary mirror making it expensive to make and heavy. However, for professional applications where low systematic effects are critical, the benefits of low systematics across a large field of view can far out-weight these disadvantages.
History
Corrado Dragone, from whom this optical design gets its name, first described the design in his 1978 paper. Several follow-up papers were published in the 1980s, however it was not until recently that astronomers have been able to build focal planes large enough to warrant the extra construction costs associated with the large secondary mirror of the Cross Dragone design. Older millimeter or submillimeter telescopes have typically been of Gregorian or Cassegrain designs.Examples
Some examples of existing and planned telescopes that use this design include:- The QUIET experiment
- The Atacama B-mode Search (ABS)
- EPIC-IM
- Fred Young Submillimeter Telescope
- Simons Observatory
- CMB-S4 Experiment
- BINGO (telescope)