Title: Early Commissioning of ATLAS
1Early Commissioning of ATLAS
- First North American ATLAS Physics Workshop
- Tucson
J. Pilcher University of Chicago
2Early Commissioning of ATLAS
10 Dec 04
3Commissioning Goals
- Establish operation of full systems
- Readout
- Calibration systems
- Low Voltage, High Voltage
- Control and Monitoring
- Cryogenics, Gas, Cooling
- Establish initial calibrations
- Mev/ADC count
- Alignment and timing
- Chamber or sensors within a detector system
- Relative alignment and timing of different
detector systems - Demonstrate performance levels
- Noise levels
- Physics signals
4Commissioning Stages
- Calibration systems only
- Cosmic ray muons
- MIP signals and inelastic interactions
- Stand-alone detector systems (2005-6)
- Full ATLAS detector (2007)
- Initial beam operation
- Single beam operation
- Beam-gas interactions
- Beam halo muons
- Beam-beam operation
- Minimum bias interactions
- Early beam-beam collisions
- Use physics signals ( , ?-j, Z-j,
j-j, )
5- This talk
- Concentrate on first three stages
- Other talks on commissioning with beam-beam
physics signals - Special emphasis on calorimeter systems
- More details at
- Tatra Workshop
- http//agenda.cern.ch/fullAgenda.php?idaa041267
- Overview week at Freiburg commissioning session
- http//agenda.cern.ch/fullAgenda.php?idaa041780s
0 - Overview week at Prague commissioning session
- http//agenda.cern.ch/fullAgenda.php?idaa03190s2
- This talk draws on the work of many people
- R. Teuscher, R. McPherson, J. Huston,
6- Preliminary commissioning already being done
- Combined test beam in 2004
- Tilecal operation on cosmic muons in Bldg. 185
- LAr operation on cosmic muons in Bldg. 180
- Muon chamber operation with cosmics
- TileCal barrel on HF truck in UX15
- Commissioning is iterative with larger scale
integration at each step
7Now TileCal Commissioning on HF Truck in UX15
Record data from UX15 testing TTC, CANbus, HV,
laser fibres via LED, BCID _at_ 100 kHz L1A, CIS,
readout noise,
Charge Injection Pulses OK
Noise Test OK
RMS (ADC counts)
Photo from September 28, 2004
8- Barrel calorimeters move to z0 August 2005 when
BT is assembled - Detectors fully assembled and equipped with
on-detector electronics - Connect to services
- Stand-alone commissioning with calibration
systems - Eg. for TileCal (1/2 the system)
- Charge injection to all readout channels (4K in
barrel) - Cesium source activates tiles and fibers (220K in
barrel) - Laser system activates each PMT (4K in barrel)
- First large-scale detailed commissioning
9Charge Injection Calibration of TileCal
- Pulse individual channels over full dynamic range
- establish gain, linearity, stability
Uncorrected channel-to-channel uniformity RMS
1.3 counts/pC (1.6)
Gain variation over 4 months of CTB RMS 0.2
10Cs Calibration of TileCal
- Cs-137 source illuminates individual tiles
- Stainless tubes pass through all tiles in the
system - Source capsule driven through tubes hydraulically
- Single tile response measured at 2 level
- Cell response measured at 0.3 level
- Week-to-week variations in cell response 0.5
11Cosmic Ray Commissioning
- Full G3 simulation done by Rob McPherson and
Pavel Nevski
12Cosmic Ray Commissioning
- Rates are substantial
- 2.3 KHz for a hit anywhere in detector
- 0.5 Hz for Z
- Natural to trigger with muon system RPCs
- Global ATLAS cosmic muon run planned for 40 days
in April 2007 before LHC starts - Attractive to run barrel calorimeters on cosmics
from late 2005 - Before RPCs available
- Evaluated trigger using TileCal
- back-to-back trigger towers
13TileCal Response to Muons
- Test beam data for 180 GeV muons at ?0.05
- Energy depends on path length through calorimeter
- 1K muons in a tower gives response to 1
Tower Energy (pC) (1.1 pC/GeV)
14TileCal Cosmic-Muon Trigger
- Consider back-to-back TileCal towers
- ?? x ??0.1 x 0.1, full calorimeter depth
- Especially useful because tracks pass close to
interaction point - Analyze McPherson/Nevski simulation for rate and
event properties - S. Zenz (Chicago undergraduate)
15TileCal Cosmic-Muon Trigger
- Require 2 back-to-back towers with E 1.5 GeV
- Lower peak corresponds to additional towers
struck (corners clipped)
Rate is 130 ?/hr for 16 top 16 bottom
modules in coincidence 100K / month
16TileCal Cosmic-Muon Trigger
- Effect of PX14 shaft is
- clearly seen
17Typical Events
18Typical Events (2/2)
Example of muon scattering in detector
19Muons in LAr Barrel
Due to Accordion geometry, muons are
reconstructed in middle compartment by summing
two cells in ?.
- With 100 events muon signal in LAr can be
measured with - 3 precision
- For first shake-down
- Could use cosmic ray muons to measure first LAr
physics pulse shapes and compare to calibration
pulses. - Useful to reconstruct combined muons in LAr
TileCal to match EM energy scale and timing.
Note S/N ratio too small in strip and back
compartments
20Muons in LAr Using TileCal Trigger
- TileCal Trigger tower size (0.1?0.1) corresponds
to 4?4 LAr middle cells - Resulting maximum non-projectivity ? 3º, muons
can cross at most 2 cells in ? and in ? - ? non-projectivity probably not a problem, due to
natural sharing between ? cells (two cells are
summed)
- Studies of rate in LAr using TileCal cosmic
trigger (back-to back towers) by Philippe
Schwemling and Emmanuel Monnier. - Est. 6 months run
21With 100 muons/cell in middle compartment
- Check calorimeter timing to optimal filtering in ROD
- Check calorimeter position in ? / ? wrt other
sub-detectors to
Test-beam data
- 1 precision measured with 1000 ?
- with 5000 ? 0.5 precision
- ( 100 ? /cell integrated over ?)
22Hardware Needed for TileCal Cosmic Trigger
- Electronics drawers in barrel (128)
- LV power (in TileCal fingers)
- Bulk LV power (200V for USA15)
- Cabling and fibers
- TTC hardware
- Standalone clock
- LVL1 trigger interface hardware
- Patch panels to separate tower and muon signals
- Receiver boards (64 towers each)
- Initially use custom trigger logic for cosmic ray
running - ROD/LVL2 hardware
- ROD modules, ROD crate and controller (ROD crate
DAQ) - Output hardware from ROD crate to PC via Ethernet
- Later use ROBIN/ROS
23TileCal Muon Trigger Logic
- LVL1 trigger not designed to run on back-to-back
muons - Adapting it would be a diversion
- Also scheduled to arrive late compared to initial
stand-alone calorimeter operation - Build some simple coincidence logic
- Test by injecting muon signal into trigger tower
- Vary tower threshold and check efficiency
24Time Table for Cosmic Ray Commissioning
- TileCal barrel complete Mar-06 (following
checkout) - Stand alone operation begins
- LAr barrel complete Aug-06 (following checkout)
- Stand alone operation begins
- Global commissioning Dec-06 through Feb-07
- ATLAS cosmic run
- Mar-07 through Apr-07
- ATLAS ready for beam 4/27/07
25First commissioning with single beam
- Beam halo muons
- Generated by machine group
- Simulated in ATLAS
- Beam gas events
26A typical beam-gas event
Beam-gas collisions are essentially boosted
minimum-bias events ? low-pT particles
Rate 2500 interactions/m/s
27Beam-gas Rates Properties
28Beam Halo Muons
Especially useful for endcaps and ID disks and
wheels
29Beam-Halo Rates
- Estimate rates for 200 times less current than
design - Totals in table for 2 month run at 30 efficiency
30Triggering on Beam Halo and Beam-Gas events
- Minimum-bias scintillators being added in front
of LAr end caps - z 3.5 m
- 14 cm
- 1.9
- 8 channels in ?, 2 channels in ?
- Readout via TileCal electronics drawer
Joey Huston is project leader on this.
31Conclusions
- Good prospects for progressive commissioning
process - Stand alone detector systems with calibration
systems and cosmic muons - Global detector with cosmic muons
- Beam halo muons and beam-gas events in early 2007
- Minimum bias beam-beam interactions by mid 2007
- Fully simulated samples of cosmic muons,
beam-halo muons and beam gas events exist - R. McPherson et al.
- Final commissioning phase will be with physics
signals - Essential for final tune-up
- Essential for showing we understand the detector
behavior