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Surface fit regression algorithm for CTA mirror measurements

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Qt Software for Parabolic Mirror Surface Fit Regression

Motivation

The Cherenkov Telescope Array is a prototype telescope comprised of several independent mirror panels. This software allows for the fitting of measured points on a given mirror panel based on a regression algorithm in order to determine the accuracy of the panel as related to the theoretical shape.

Stack

The App is built on C++ using Qt. The algorithm logic uses the Armadillo C++ Linear Algebra Library. Plotting is done using MathGL. Boost C++ libraries are also used.

A sample video of the App can be found here.

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Surface fit regression algorithm for CTA mirror measurements

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