Paper
20 July 2000 Final alignment of the VLT
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Abstract
In a recent paper McLeod proposed and used measurements of the field dependence of third order astigmatism to collimate a Ritchey-Chretien telescope with the stop at the primary mirror. We adapt this method to the Cassegrain focus of the ESO Very Large Telescope, where the stop is at the secondary mirror and the telescope is only corrected for spherical aberration. In addition, we study the effects of the practical definition that the center of the field is the center of the adapter. We present measurements of the field astigmatism and discuss the accuracy of this collimation method.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Lothar Noethe and Stephane Guisard "Final alignment of the VLT", Proc. SPIE 4003, Optical Design, Materials, Fabrication, and Maintenance, (20 July 2000); https://doi.org/10.1117/12.391501
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CITATIONS
Cited by 17 scholarly publications.
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KEYWORDS
Monochromatic aberrations

Mirrors

Telescopes

Active optics

Collimation

Wavefronts

Error analysis

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