Concerning the alignment of modern telescopes: theory, practice, and tolerances illustrated by the ESO NTT

Details Concerning the alignment of modern telescopes: theory, practice, and tolerances illustrated by the ESO NTT Concerning the alignment of modern telescopes: theory, practice, and tolerances illustrated by the ESO NTT

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997pasp..109...53w&link_type=abstract

Publications of the Astronomical Society of the Pacific, v.109, p.53-60

Astronomy and Astrophysics

Astronomy

4

Telescopes, Instrumentation: Miscellaneous

Scientific paper

A recent paper by Bhatia (1995) suggest from calculations based on the optical geometry of the NTT that the zero-coma condition is a necessary but insufficient condition for the alignment of modern telescopes and that analysis of separate decenter effects is necessary to cope with decentering astigmatism aberrations near the field c enter. We show here that, while Bhatia's calculations are quite correct, their basis shows a misunderstanding of how the NTT was actually aligned and that this "passive" alignment was sufficiently good that the decentering astigmatism effects he indicates were negligible. More dangerous are the wide-field effects of decentering astigmatism discussed by McLeod (1996). However, we show that these effects, linear with field, are also negligible with the NTT alignment quality achieved, provided the correct effective shift of the astigmatic field center is allowed for int he active correction software. This is of great importance in the NTT because the image analyser operates at the edge of the field and the correct field astigmatism must be subtracted to give the necessary active correction at the mechanical field center. This approach is valid for the technical use of the edge field of an aplanatic (RC) telescope limited by field astigmatism. Decentering astigmatism will be much more critical at the field edge for anastigmatic telescopes is a wide field is also used for astronomical observation. (SECTION: Astronomical Instrumentation)

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