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SVN DESY Paper

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From my computer I can check it out)

worked:

kinit novgorod@DESYNOSPAMPLEASE.DE

svn co https://svnsrv.desy.de/basic/FCAL/Documents/paperTB2011

svn ci

svn co http://svnsrv.desy.de/public/FCAL/Documents/paperTB2011

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30.01.2013 S/N ratio for the thesis

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The S/N calculation for the TB10 is somhere here, at least the histograms are there, where is the plot making

/home/daq/TMP/Olga/PutFilesTogether/cluster4_spectra150samples

Final plot for thesis was done for first fit of cluster 4 channel 27

and script is located at lcdaq pc /usr1/scratch/Olga/TB10_Olga folder

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11.01.2013 Test pulses measurements over the shutdown week:

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TestPulses_data_2013-01-08_14-17-22_Tue.root Ch 3 - Amplitude - 20.9593 : 98.8362

//TestPulses_data_2013-01-08_14-17-22_Tue.root //Ch 3 - Amplitude - 20.9593 : 98.8362

TestPulses_data_2013-01-09_10-05-51_Wed.root Ch 3 - Amplitude - 20.5734 : 97.5005

TestPulses_data_2013-01-09_14-51-46_Wed.root Ch 3 - Amplitude - 20.8487 : 97.8932

TestPulses_data_2013-01-09_20-05-10_Wed.root Ch 3 - Amplitude - 20.421 : 97.5555

TestPulses_data_2013-01-10_09-51-08_Thu.root Ch 3 - Amplitude - 20.5247 : 97.7579

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10.01.2013 Baseline over 2011-2012 years summary:

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/d1/brmpro/data/bcm1f/ADC/baseline monttBL_plus.C : subtracted min value : problems with time format, but in the root file it is changeble by touching the timeformat

Files from 2011 are on brmbcmctrl3 in the folder /nfshome0/olga/BCM1F/baseline

File - baselineRecord_2011_all.dat

I put two files together and plot the final baseline dependence, hurra - two years data)

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14.12.2012 Test Pulses Raw Data:

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/afs/ifh.de/group/cms/olga/bcm1f/measurements/PlotTPch3.C

Was:

double amplitudedata3[N]={27.99, 27.72, 26.84, 26.47, 26.58, 25.1, 25., 27.1, 25.69, 24.5, 23.45., 23.42, 21.87, 21.62,21.29,20.97};

double baselinedata3_[N]={139, 137, 134, 130, 129, 125.8, 124, 130.3, 131, 126.6, 113.2, 108.6, 104.9, 101., 100.,98.88};

double Time[N]= {0., 0.01, 0.5, 2.4, 2.8, 4.8, 6., 6.1, 6.5, 7.2, 17.5, 21, 23.5, 25, 26.5 , 26.5 };

Proven data:

double amplitudedata3[N]={27.99, 27.72,26.84,26.47, 26.58,25.10,25.0, 27.16,25.67,23.48,23.01,21.87,21.62,21.29,23.06,21.76}

double baselinedata3_[N]={124.8,127.2,134.5,135.6,135.6,135.6,129.4,130.4,131.9,112.3,108.5,105.2,101.5,100.9,112,101.4}

double Time[N]={0.,0.01,0.5,2.4,2.8,4.4,5.5,6.13,7.2,18.,21.,24.5,26.,27.42,29.36,29.36}

16.10.2009 --> 27.99 --> 0 --> 28.3 --> 124.828 -->data_Fri_Oct_16_10.48.53_2009_397305.root

=====2011============== 44 pb

21.02.2011 --> 27.72 -->0.01--> 27.61 --> 127.2 --> data_2011-02-21_15-51-11_Mon.root

25.05.2011 --> 26.84 --> 0.5 --> 26.70 --> 134.5 --> data_2011-05-25_16-08-29_Wed.root

15.08.2011 --> 26.47 --> 2.4 --> 26.55 --> 135.6 --> data_2011-08-15_15-56-03_Mon.root

30.08.2011 --> 26.58 --> 2.8 --> 26.55 --> 135.6 --> data_2011-08-30_15-51-36_Tue.root

19.10.2011 --> 25.10 --> 4.4 --> 25.24 --> 135.7 --> data_2011-10-19_09-18-10_Wed.root

09.11.2011 --> 25.00 --> 5.5 --> 26.95 --> 129.4 --> data_2011-11-09_12-32-35_Wed.root

======2012============= 6.13 fb

01.02.2012 --> 27.16 --> 6.13 --> 130.4 --> data_2012-02-01_09-50-34_Wed.root

05.03.2012 --> 25.67 --> 7.20 --> 131.9 --> data_2012-03-05_15-28-49_Mon.root

16.08.2012 --> 23.48 --> 18.00 --> 112.3 --> TestPulses_data_2012-08-16_11-54-01_Thu.root

03.09.2012 --> 23.01 --> 21.00 --> 108.5 --> TestPulses_data_2012-09-03_11-10-22_Mon.root

18.10.2012 --> 21.87 --> 24.50 --> 105.2 --> data_2012-10-18_16-41-08_Thu.root

31.10.2012 --> 21.62 --> 26.00 --> 101.5 --> TestPulses_data_2012-10-31_12-02-30_Wed.root

06.11.2012 --> 21.29 --> 27.42 --> 100.9 --> TestPulses_data_2012-11-06_18-00-51_Tue.root

14.12.2012 --> 23.06 --> 29.36 --> 112 --> TestPulses_data_2012-12-14_14-37-04_Fri.root

17.12.2012 --> 21.76 --> 29.36 --> 101.4 --> TestPulses_data_2012-12-17_12-45-25_Mon.root

========2013=======

08.01.2013 --> 20.97 --> --> 98.88 --> TestPulses_data_2013-01-08_14-18-27_Tue.root

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06.11.2012 Location of test pulse plot:

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/afs/ifh.de/group/cms/olga/bcm1f/measurements/PlotTPch3.C

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25.10.2012 Integration within 300 ns in case thresholds are applied:

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Included integration of signals for FT like files to see MIP peak as a function of time for 2012 07 to 10 monthes as i recorded a lot of FT files. I can also make analysis for the FT I measured in 2011

[brmpro@BRMBCMCTRL3 ADConline]$ ./AmplSpectr_newBL_BCM1F_everyhourscan_integral /d2/brmpro/data/bcm1f/ADC/CASTOR/2012/FT_data_2012-09-07_23-16-42_Fri.root

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How to convert all eps files to gif files:

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for f in *.eps; do convert $f `basename $f .eps`.gif; done

For CASTOR Files moving to lxplus back: for f in `nsls /castor/cern.ch/user/o/olga/ADC_2012/DATA/`; do nohup rfcp /castor/cern.ch/user/o/olga/ADC_2012/DATA/$f /tmp/olga/. &; done

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*15.10.2012

Tungsten Searches for Test Beam 2011

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Scripts to run files corresponding to the different shaper and preamplifier modes: WHLscript.sh WLHscript.sh Wscript.sh Location: /home/daq/TB_HH_11/tb-eudaq/trunk/bin Next programs were written:

1. Tungsten.exe - to read out files from new DAQ and see full deposition in the BeamCal from all particles in the runs

2. Tungsten_Fit.exe - to analyse results from Tungsten.exe files and plot profile of showers for MPV and mean values Script for this is WFit.sh

3. Tungsten_2D.exe - this is for the 2D plot in XY and in XZ planes to see the shower profile and estimate R_m

2. Tungsten_Fit2D.exe - to analyse results from Tungsten.exe files and plot profile of showers for MPV and mean values and for longitudinal profile - not ready problems with reading bins from 2D histogram Script for this is WFit.sh Results are shown in my thesis)

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* 07.09.2012*

Compression of the FT files on the brmbcmctrl3 machine:

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./FlatTopFilesSuppretion_nocoinsidence - program to save only entries with one or more signal in the orbit in one of the diamonds of BCM1F.

Location: ~/olga/scripts/

Output files are:

/d2/brmpro/data/bcm1f/ADC/CASTOR/2012/Out_Supression_no_coinc_092012e.root

/d2/brmpro/data/bcm1f/ADC/CASTOR/2012/Out_Supression_no_coinc_082012end.root

Idea is to suppress all files and be able to do integration. As signals are rare, integration can be done over full orbit.