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    User name riordan

    Log entry time 17:55:01 on April 16, 2010

    Entry number 317712

    keyword=GEM Analysis Status

    I've spent a little more time on the GEM analysis to try and make sense
    of the hits we see.  For the most part, the signals seem to be mostly
    reasonable with the exception of a few rogue channels.  I had to make a
    few changes to get the clustering working properly:
    
    1)  The gassiplex channel to strip mapping needed to be modified for half
    the planes (it still needs to be thoroughly, systematically checked).
    2)  Software pedestals implemented
    3)  Event-by-event pedestal noise suppression added
    
    For those of you playing at home, the run I'm showing below is 27356,
    with a few cuts on cluster size and minimum ADC value.  The software I've
    used here is a modified version of Ole's TreeSearch-GEM library, which
    I'll give to him for "production" on the adaq machines once I check a few
    more things.  The replayed file can be found on the adaq machines as:
    
    /adaqfs/home/adaq/happexsp/prex/prex_gem_L_spr_27356.root
    
    The script I used to make most of these plots is here:
    
    /adaqfs/home/adaq/riordan/prex/plotvdc3.C
    
    Additionally, Alex and I believe that the INFN chamber below that doesn't
    show a signal may have had voltage that was too low.  
    
    The event-by-event noise is a more crude version of what Guido/Evaristo
    suggested, but I think it works for now.  The noise subtracted pedestals
    look pretty clean, fig 1.  The noise is roughly the same size as the
    noise-subtracted pedestal, fig 2.  Additionally, the UVA and INFN planes
    seem to have some correlation, fig 3.  The INFN chambers show high
    inter-chamber correlation, fig 4.
    
    I think the clustering may need a little work.  For many events we see
    some nice clean signals, fig 5.  However, for many events we'll see more
    complicated event structures, such as fig 6.  I think these multiple
    messy peaks together are related to the same track, since they show some
    correlation with the projected VDC tracks, fig 7, fig 8.  I think if we
    let the tracking select out a single one of these multiple peaks the
    apparent spatial resolution will improve.  (These could also be a mapping
    problem, I need to check more closely).
    
    What was very nice is the strong cluster ADC sum correlation between the
    orthogonal planes in the same chamber, fig 9, 10.  The second UVA chamber
    probably needs some work and HV adjustment (the hit efficiency on the y
    plane is definitely much lower), but you can clearly see the other two of
    the chambers giving a strong peak.  I'm hoping the stuff around the peak
    is stuff that shouldn't be associated with it.  Believing that, some
    estimates give the XY misassociation probability of ~0.3-0.4, which I
    understand is close to what was seen before.
    
    We do have three working chambers, so it may be worthwhile to try and
    start doing tracking with them using the data we have.  I believe the
    tracking efficiency at this point will be pretty low, but can be improved
    with work.  One of the critical things to do right now is develop HV
    optimization criteria, which will probably be dependent on the tracking
    performance.
    


    A copy of this log entry has been emailed to: riordan, nl8n@virginia.edu, rom, ole, kkumar@physics.umass.edu, souder@physics.syr.edu, evaristo.cisbani@iss.infn.it,camsonne, Guido.Maria.Urciuoli@roma1.infn.it, ks4dk@virginia.edu, bogdanw, ates



    Figure 1 - Corrected pedestal



    Figure 2 - Pedestal Noise



    Figure 3 - UVA/INFN Noise Correlation



    Figure 4 - INFN Noise Correlation



    Figure 5 - Clean Event



    Figure 6 - Messy Event



    Figure 7 - GEM hit pos vs proj VDC pos



    Figure 8 - GEM hit pos, proj VDC pos diff



    Figure 9 - GEM ADC Correlations



    Figure 10 - GEM ADC Differences