rd51 gem telescope: results from june 2010 test beam and work in progress
DESCRIPTION
RD51 GEM Telescope: results from June 2010 test beam and work in progress. Matteo Alfonsi on behalf of CERN GDD group and Siena/PISA INFN group. Outline. Overview GEM tracking chambers details Electronics and DAQ Results from June 2010 test beam - PowerPoint PPT PresentationTRANSCRIPT
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RD51 GEM Telescope:
results from June 2010 test beam
and work in progress
Matteo Alfonsion behalf of CERN GDD group
and Siena/PISA INFN group
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Outline
• Overview• GEM tracking chambers
details• Electronics and DAQ• Results from June 2010 test
beam• Synchronizing two different
DAQs and other ongoing improvements
• Conclusions and future plans
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CERN experimental table
Mechanics with 5 movable supports mounted over rails.
GEM telescope and MICROMEGAS telescope(both with 3 X-Y stations)
Trigger scintillators (triple coincidence)
Table with wheels and possibility to rotate in the “cosmic ray stand” position
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Triple GEM tracking chamber
Active area: 10 x 10 cm2
“COMPASS” X-Y strip readout, with ~ 0.4 mm pitch
Sealed Triple GEM detector with a compact design:− HV divider: only 1 HV channel− Ar/CO2 70%/30% cheap premix
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GEM Tracker characterization
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Rate (Hz/mm2)
Ga
in
Cu x-rays ΔEFWHM/E = 19.8%
Fe x-raysX-Y strips correlation
Rate capabilityGain vs. voltage on the divider
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Electronics and DAQ
• VFAT2 front-end electronics• Readout board “TURBO”
developed by Siena and PISA INFN
• Some slides from E. Oliveri.. (and a special thank to him for the support in the beam!!)
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The readout chip: VFAT2
128channels
Gain 60mV/fCShaping Tine 22ns
LV 1A Latency 6.4s
Stretching up to 8 clock cycles
ANALOG AND ASYNCRONOUS
DIGITAL AND SYNCRONOUS
Amplification and
Shaping
Comparisonwith a
programmableThreshold Synchronization
AndTime stretching
Data Storage and Transmission
FAST OR Triggeroutput
Triggering and tracking synchronous front-end ASIC designed primary for the TOTEM experiment and characterized by:• Preamplifier-shaper-comparator readout chains (128) to detect signals above a programmable threshold.• Fast-OR lines (up to 8) that merge channels of programmable sectors to provide a trigger signal.
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TURBO
Input/Output LVDS/NIM/CMOS(clk, trigger,…..)
QuickUSB
DAC OutTurbo PowerVFAT2 Digital PowerVFAT2 Analog Power DCU
8 x
VFA
T2
TURBOs ChainControl/Data BUS
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RD51 June TB Set Up
USB
USB
Trigger/VETO/CLK…
Trigger/VETO/CLK…
8 VFAT2
8 VFAT2
Control and DataAcquisition from 24 VFAT2s
USB8 VFAT2
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TURBO REGISTERS
VFAT2 REGISTERS
TURBO/VFAT2 CONTROL and DAQ with LabVIEWCa
libra
tion
Puls
e Sc
an
Simple Acquisition
etc. etc. etc……
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Results from the test beam
Test beam performed together with CMS MPGD group, which used tracks information for their devices under test.
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Test beam setup in June 2010
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Binary raw data file
ROOT raw data (“hits”)
ROOT reconstructed data (“clusters” and “tracks”)
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Raw data “hits”
In June tracking chambers were 75% equipped, with:− 2 VFATs on the (vertical) X-strips, i.e. 256 channels over 10 cm− only 1 on the (horizontal) Y-strips, i.e. 128 channels over 5cm.
The noise level with fully equipped detectors was in fact higher and, taking into account the beam size, decision was taken to postpone the investigation of the proper grounding and shielding.
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Clustering algorithm• Neighbouring (with one channel gap maximum) channels
belong to the same cluster.• Cluster position is the centre of gravity of the included hits
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Beam profile
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Alignment correction
• Before tracks reconstruction, alignment is corrected with the correlation plots
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Misalignment (in strip units) between chambers
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Track reconstruction
• Few limitations at the moment:– Combinatorial to be implemented (tracks are
reconstructed only in the events with one cluster per station)
– Tracks are reconstructed separately in the “X” projection and the “Y” projection
Tracks information available around 80% of the events
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Spatial resolution• Only 3 stations a preliminary information can
obtained from the broadening of the cluster position difference between two stations
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• Assuming two identical devices:
√(2σ2) = 1.11 × 0.4 mm
σ ~ 300μm(preliminary result!)
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Future plans
• Synchronizing two different DAQs
• Other ongoing work
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More DAQs synchronization
Very hard to find an universal solution, so we propose a reasonable strategy that could work over a large number of cases:Each DAQ must be able to VETO the trigger (on the common NIM coincidence unit!!!), for example when it busy or not runningEach DAQ must implement a reliable trigger counter, which can be reset at the beginning of the runSeparate datafiles can be merged again by a proper event builder
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Other ongoing work
• Event builder: new raw data “hits” ROOT file with a “zero suppressed” format (to reduce file size)
• Generalization of the algorithm for any readout shape (useful for the TOTEM wedge-shaped chamber in August)
• Clustering algorithm for analog readout (in case of APV chip in October)
• Track reconstruction improvements• All algorithms in a small “software framework”
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Conclusion
• The GEM telescope is a good instrument for RD51 groups that need track information
• DAQ with digital VFAT2 readout is ready and improvement are ongoing
• Minimal analysis software is ready and further developments are ongoing
• A priority for the next test beam is the integration with different DAQs
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Backup
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