Difference between revisions of "HRS Detector Calibrations"

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   </tr>
 
   </tr>
 
   <tr>
 
   <tr>
     <td>11.02</td>
+
     <td>4.481</td>
     <td>1.0</td>  
+
     <td>0.75</td>  
     <td>48.8</td>
+
     <td>48.0</td>
 
     <td>None</td>
 
     <td>None</td>
     <td>15 cm LH2</td>
+
     <td>Optics</td>
 
     <td>2 mm x 2 mm</td>
 
     <td>2 mm x 2 mm</td>
     <td>20&mu;A</td>
+
     <td>5&mu;A</td>
 
     <td>S0&&S2m</td>
 
     <td>S0&&S2m</td>
 
   </tr>
 
   </tr>
* Use LH2 "white" spectra to get maximum coverage of planes, take 250K events.
+
* Use Optics "white" spectra to get maximum coverage of planes, take 250K events.
 
</table>
 
</table>
 
<ol>
 
<ol>

Revision as of 13:21, 4 February 2016

  • Use Optics "white" spectra to get maximum coverage of planes, take 250K events.
Ebeam [GeV] P0 [GeV/c] θe [deg] Collimator Target Fast Raster
X x Y
Beam Current Trigger
4.481 0.75 48.0 None Optics 2 mm x 2 mm 5μA S0&&S2m
  1. Check the timing and calibration constants (shower ADC gains, pedestals, timing offsets, pulse height corrections, attenuation lengths, efficiencies, position dependencies).
  2. VDCs and Straw Chambers
    * Look at drift time spectra, is the shape reasonable? in the right time range?
    * Fit for new time-to-distance map
    * Look at focal plane distributions.
    * Check fiducial tracking efficiency, is it > 95%, If not, then check TDC windows and tracking parameters.
  3. HRS Scintillators
    * Look at all channels, compare against standard histograms.
    * Are any channels firing at high rate (possible light leak)?
  4. Gas Cherenkov (Barak Schmookler)
    * Look at histograms (Npe vs. x, and Npe vs. Shower), compare with standard distributions, ideally there shoudl be no x dependence.
  5. Electromagnetic calorimeters
    * Make sure all ADC channels have signals.
    * Calibrate with electrons. Maybe not be possible at this energy due to low rates.
  • After these steps, the detectors should be fairly well calibrated.