Absolute normalization for TOWER gains.

  1. Comparison of mean MIP MPV for: CuCu data (red line), pp data (green line,lower), and ideal M-C (blue squares) vs. eta bin.
    Y-axis: MPV (ADC), X-axis: eta bin

    #comparison of mean MPV of MIP (in ADC ch) for 2005 run
    # etaBin, CuCu,  pp,    ideal,   Cu/pp
    1         6.7    6.8    6.86      0.99
    2         7.6    7.8    7.58      0.97
    3         8.4    8.4    8.33      1.00
    4         8.7    8.9    9.17      0.98
    5         9.4    9.3    10.05     1.01
    6         10.2   10.0   10.96     1.02
    7         11.5   10.8   11.92     1.06
    8         12.8   12.3   12.90     1.04
    9         13.8   13.1   13.91     1.05
    10        15.3   13.9   15.01     1.10
    11        17.0   15.5   16.21     1.10
    12        17.1   15.3   17.36     1.12
    
    The mean MIP peak position differs for up to 12% for CuCu vs. pp data. The plausible reason of larger reconstructed MIP response for CuCu minB events is higher occupancy than for pp events.

  2. The ETOW gains from CuCu data were divided by the eta-dependent factor shown in the last column.

  3. A motivation.
    The MIP isolation conditions required for towers:
    * 7 inactive strips on either side of fired strip(s) in both planes - this forms a cross 7 cm wide, at 45 deg to the tower grid
    * fiducial volume cut requiring UxV sits in 50% area of the tower
    For small towers at large eta~2 (eta bin 1) both conditions cover the whole tower area. However for large tiles at eta ~1 (eta bin 12) there

  4. Distribution of reconstructed MIP's in the Endcap using only SMD information, from minB triggered events. The eta dependence for CuCu differs from pp. Note, plots show projection of a sphere on a plane, so it is the CuCu data which show strong eta(=theta) dependence.

    p+p minB events:

    p+p minB events


    Cu+Cu minB events (view from outside):


  5. BTW, do you see it too that sectors 3,6,9,and 12 count ~10-20% more MIPs? Especially in the CuCu data?

    I'm working on Endcap calibration very long, to long and start to see things. But I convinced Steve the cross is there. And he even came up with a plausible explanation:
    Plot below shows SMD layer 1, the closest to IP. There is a sheet of passive plastic in front of the 1st active SMD layer for sectors 3,6,9,and 12 - it absorbs low energy particles so the UxV condition requiring no signal (in total of 7*2*2=28 consecutive strips on each side of the fired strips) has bigger chance to be fulfilled.


    gnuplot> 
    set key 5,5
    set xlabel "eta bin"
    plot [0:13][0:20] 'mpv.dat' using 1:2 with  linespoints, 'mpv.dat' using 1:3 with linespoints,'mpv.dat' using 1:4 with point