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Using your models

Gary Bernstein edited this page Apr 30, 2017 · 1 revision

See the Starflat cookbook for some scant information on the C++ programs in the src directory that allow you to image or apply the photometric and astrometric solutions derived. More info is in each programs help message and code.

The analysis directory contains some Python codes that I have used to tabulate or graph properties of the residuals to the fits. These come without documentation, contact me for more information.

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