Preliminary optical design for the WEAVE two-degree prime focus corrector
2012
We present the preliminary optical design for a new two-degree refractive prime focus corrector for the 4.2m William
Herschel Telescope optimised for the wide-field multi-object spectrograph, WEAVE (WHT Enhanced Area Velocity
Explorer). From the two conceptual designs described previously [1], the counter-rotating atmospheric dispersion
corrector approach was selected and further optimized to meet the flat image surface requirement. The preliminary
design provides good polychromatic image quality. The PSF does not exceed 0.6 arcsec (80% encircled energy) over a
wavelength range from 370 to 1000nm covering a two degree FOV for zenith angles up to 65 degrees. We describe the
corrector's performance and the trade-off between telecentricity and the requirement for a flat image surface. We present
the results of the tolerance and thermal analyses, ghost and scattered light calculations and the finite element analysis
that are necessary to establish the PSF error budget for the corrector.
Keywords:
- Correction
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