Table of contents :
Takahashi TOA 130 and 150 in UV
Dall Kirkham 200 mm F/4- F/15, Mewlon 210 F/2.9-F11.9 and Mewlon 250 F/3-F15
Cassegrain 200 mm F/4-F/15 and Cassegrain 350 F4.9-F29.2
Celestron "classic" and Edge-HD versions overview
Celestron 8 classic and Edge-HD
Celestron 14 with optimized Schmidt plate position
Celestron 8 with optimized Schmidt plate position
Celestron 14 classic and Edge HD
Maksutov-Gregory 90 mm f/15.7, Maksutov-Gregory 200 mm f/15,Maksutov-Rumak 200 mm f/10
OSLO model:
NB: By comparison, the M1-M2 distance of the Astrosib RC 500 f/3-8 is 994 mm (instead of 1009.1 mm) while the backfocus (from the surface of M1) is 335 mm (instead of 300 mm).
Sensitivity of Strelh ratio to backfocus:
The RC design is very sensitive to backfocus. In order to keep the Strelh ratio > 0.9, the backfocus should be within +/- 20 mm of its nominal value.
By comparison, the field covered by the ASI1600 (4536 pixels × 3520 pixels × 3.8 microns) at 0.08 arsec/pixel resolution is 0.1° × 0.08°
For the nominal M1-M2 spacing, the radius of the diffraction limited flat field of the RC 500 f/3-8 is 0.11° :
rms Optical Path Difference of a 0.11° radius:
With the 2× "Long Barlow" lens (f=-142.3 mm), the radius of the diffraction-limited flat field is 0.074° in green light:
Back to comparison of telescope optical design for high resolution imaging