Speaker
Description
The Small Sized Telescopes (SST) of the Cherenkov Telescope Array Observatory are one of three designs to be used in the array, specifically focused on observing TeV gamma-rays. A partial prototype of the final camera design for these telescopes (QCAMi) has been built, and will undergo on-sky testing in Tenerife this June/July. As part of this commissioning process, waveform data is produced in a controlled lab environment by flashing the camera with a laser. This data can then be analysed for anomalies, processed to assess charge extraction performance, and compared to the existing SST simulation configuration. In this presentation, I will show my progress in processing and analysing QCAMi data, and outline future steps of the commissioning process.
