Status of HRS Detectors Barak Schmookler DVCS - 12/19/20131.

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Presentation transcript:

Status of HRS Detectors Barak Schmookler DVCS - 12/19/20131

Overview Standard detector stack Upgrades*: – VDC: Replaced the old discriminator cards – One straw chamber from FPP is installed in each arm – Gas Cherenkov: New windows, new PMTs, S0 on front *Partially Completed DVCS - 12/19/20132

3

VDC DVCS - 12/19/20134 Replaced discriminator cards with new MAD cards HRS-L: gas, DAQ restored & tested HRS-R: in progress Install new threshold PS module for cards (Dec 2013): currently set to 3V for cosmic data runs

FPP Straw chambers installed in each arm Gas operational in L-HRS; need clean gas line in R- HRS All cables installed; HV distribution active Low voltage supply for read-out modules operational (Nov 2013) Signals checkout: in progress DVCS - 12/19/20135

Gas Cherenkov/S0 Gas Cherenkov /S0 installed in both arms Added extension to L- HRS Gas Cherenkov New windows added; mirror alignment completed PMTs should be installed in Jan-Feb 2014 DVCS - 12/19/20136

Gas Cherenkov/S0 DVCS - 12/19/20137

Gas Cherenkov: New Windows & Mirror Alignment Replaced 3 out of 4 windows New frame is half thickness of old frame; new aluminum windows are thinner We could not install new window in back of L-HRS GC, because of fixtures attached to two mirrors Used old window with aluminum plate instead DVCS - 12/19/20138 Placed light source a certain distance from mirrors and adjusted image located at PMT position

Gas Cherenkov: New PMTs Mirror Reflectivity tests done Deterioration in reflectivity was observed for all mirrors tested Reduction in relative efficiency for BURLE PMTs ~7% DVCS - 12/19/20139

Gas Cherenkov: New PMTs Will use new PMTs (ET Enterprises, model: 9390KB) Tested 4 different types of wavelength –shifting (WLS) paint to increase efficiency – Goal: At least 10 PE in the experiment DVCS - 12/19/201310

Gas Cherenkov: New PMTs DVCS - 12/19/201311

Gas Cherenkov: New PMTs Tested four different WLS paint samples: – EJ-289 #2 (commercially available) – EJ A – EJ C Evaluation samples specially developed by Eljen Technologies – EJ E Sample EJ E gave best improvement in number of photo-electrons Setup # painted(y/n) # of PE % increase in gain A no B no C no A yes B yes C yes Different Setups correspond to different locations of the silica disks Results are reproducible with different PMTs and over time (~2 weeks) DVCS - 12/19/201312

Gas Cherenkov: New PMTs Tested four different WLS paint samples: – EJ-289 #2 (commercially available) – EJ A – EJ C Evaluation samples specially developed by Eljen Technologies – EJ E Sample EJ E gave best improvement in number of photo-electrons Setup # painted(y/n) # of PE % increase in gain A no B no C no A yes B yes C yes Different Setups correspond to different locations of the silica disks Results are reproducible with different PMTs and over time (~2 weeks) DVCS - 12/19/ Paint turns cloudy after 2-3 days but this does not affect QE

Data Acquisition Took data in L-HRSwith cosmic particles over last week Triggered on coincidence between S2M and old S0 After some work: VDC, S2M, and Calorimeter are functioning well. (Need to perform gain matching) FPP map/database is complete; but need to determine which wire in bunch was hit DVCS - 12/19/201314

Summary VDC upgrades are completed Gas Cherenkov/S0 should be operational in Jan-Feb 2014 Work continues on FPP chambers DVCS - 12/19/201315