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This report provides an overview of the first testbeam results for the ISIS sensor, including analysis of pedestals and noise, signal characteristics, track correlations, position resolution, and a summary of the findings. It also outlines future plans for publication and further testing with the EUDET telescope.
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First Testbeam results • Overview • Pedestal & Noise • Signals • Tracks • Position resolution • Summary • Future plans Jaap Velthuis, University of Bristol
Overview • Beam test October-November 2007 • DESY 1…6 GeV e- • Self contained ISIS telescope • 5 ISIS in a row Jaap Velthuis, University of Bristol
ISIS sensor • Build a complete testbeam/lab DAQ system within 3 months! • Prototype LCFI ‘Proof of Principle’ ISIS1 Sensor (produced by e2v). • 16×16 pixels each 40×160μm2 • Total active area 0.5×2.24mm2 • Needed precision mounting Jaap Velthuis, University of Bristol
Pedestal Noise Pedestals and Noise • Calculate average offset for each pixel • Reiterate to remove hits • Random noise calculated as std dev after pedestal removal • No common mode found Jaap Velthuis, University of Bristol
η=Qright/(Qleft+Qright) Signals • Cluster cut • 5σ seed cut • 2σ next cut • Clusters small • Pitch 160 μm in X • Almost no charge sharing in X • η in Y demonstrates charge sharing • S/N=33.6±0.4 Jaap Velthuis, University of Bristol
x(sensor) vs. x(sensor) y(sensor) vs. y(sensor) Tracks • Tracks result in correlations between hits in different ISIS sensors Jaap Velthuis, University of Bristol
Position resolution • Using ISIS 0,1 and 3 to predict ISIS 2 • Alignment can still be improved • σ = 11.6± 0.4 μm • Doesn’t work X: • Pixels too large • Beam parallel Jaap Velthuis, University of Bristol
Summary • Performed successful beam test • Demonstrated that ISIS works well as a sensor • Results: • S/N=33.6±0.4 • σ = 11.6± 0.4 μm • Very good! Note that: • Thinning to ILC thickness does not affect S/N • Pixels still very large Jaap Velthuis, University of Bristol
Future plans • Publish results • Beam test in August 2008 at CERN using EUDET telescope • Need this to study in-pixel variations • Possible due to high momentum particles and precision EUDET telescope • Optimise operation parameters • Need to test and compare p-type ISIS Jaap Velthuis, University of Bristol