Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-11-18
Rev.Sci.Instrum. 74 (2003) 3802-3806
Astronomy and Astrophysics
Astrophysics
17 pages, 6 figures
Scientific paper
10.1063/1.1592877
We describe a technique for improving the response of a telescope chopping secondary mirror assembly by using a signal processing method based on the Lucy deconvolution technique. This technique is general and could be used for any systems, linear or non-linear, where the transfer function(s) can be measured with sufficient precision. We demonstrate how the method was implemented and show results obtained at the Caltech Submillimeter Observatory using different chop throw amplitudes and frequencies. No intervention from the telescope user is needed besides the selection of the chop throw amplitude and frequency. All the calculations are done automatically once the appropriate command is issued from the user interface of the observatory's main computer.
Holt Lynn C.
Houde Martin
Nelson Patrick M.
Yoshida Hiroshige
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