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The paper will describe the detector performance and discuss the studies performed with cosmic ray data, such as alignment and the Lorentz angle measurement.
Since initial synchronization should reliably be performed for all ACM levels, it is important to verify the detector performance at this low SNR range.
The detector performance of with-memory signaling is compared with the detector performance for no-memory signaling.
An illustration of the detector performance is given.
Near a frequency of 0.15 the detector performance decreases to zero.
Simulation of the detector performance and the status of the prototype are reported.
With increasing beam-induced background, a degradation of the detector performance is expected.
The load resistor value is selected to optimize the detector performance.
Finally, we evaluate the detector performance and precision of shower reconstructions.
Possible solutions for increasing the photoelectron number, and thus the detector performance, are presented.
The detector performance was optimized with cosmic rays and Monte-Carlo simulations.
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