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If not, can the resolution of the detector be improved to increase the significance of the signal?
Measurements with ultraviolet light yield a spatial resolution of the detector at the Nyquist limit.
The resolution of the detector is characterized by the point spread function (PSF) which describes the spatial distribution of observed photons from a point source.
In contrast, conventional cameras are restricted as they are forced to distribute the limited resolution of the detector uniformly over a single contiguous field of view.
The energy resolution is limited by the figure errors of the optical elements and the spatial resolution of the detector.
The first benchmark experiments have been conducted in order to calibrate and confirm the position resolution of the detector.
Similar(32)
Spatial resolution of the detectors amounts to about 1 mm.
Spatial origin of gamma-ray radiation from these sources cannot be fathom due to the poor angular resolution of the detectors.
The position resolution of the detectors was determined to be 0.45 mm FWHM and time resolution was estimated to be 400 ps FWHM.
The long-term stability of the energy resolution of the detectors is ensured by periodically resetting the bias [20] every 3 min as the detector heads rotate.
Alignment constants of the sensitive coordinates are determined to submicron precision and are hence much smaller than the intrinsic resolution of the detectors used.
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