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This telescope is a prototype for a small-angle luminosity monitor, the Pixel Luminosity Telescope (PLT), for CMS.
The advantage is that statistical analysis can be run on a small number of scalar coefficients rather than on the full data set of pixel luminosity values.
A new detector is the pixel luminosity telescope consisting of 8 telescopes, equipped with silicon pixel sensors, on both ends of the interactions point.
The Pixel Luminosity Telescope (PLT) system is an innovative luminosity monitor being developed as an early upgrade for the CMS detector at the LHC.
Pixel luminosity encodes the DOI in the respective point.
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Background pixels resulting from luminosity of bright-field images were removed by threshold analysis.
The histograms were set to display statistical details of the selected pixel area in the "luminosity" channel.
The video-frame-based PSNR is defined in (1), where a frame size of M × N pixels is assumed, and ( f i, j - f i,j ′ ) stands for the luminosity difference per pixel due to the video quality degradation.
Thus, to focus on the propagating PMAFs and airglow patches, we subtracted a background defined as the average luminosity at each pixel during the 2-h period prior to the satellite measurement at that pixel location (dashed line).
We report on the 3-year INFN ATLAS CMS joint research activity in collaboration with FBK, started in 2014, and aimed at the development of new thin pixel detectors for the High Luminosity LHC Phase-2 upgrades.
This could make 3D detectors useful as pixel detectors for future high-luminosity colliders, such as the Super-LHC.
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