-- AmnonHarel - 21 Feb 2009

Relevant hyperlinks

Inputs to statistical analysis

Contact interaction models @3pb

plot_ci_model.png
  • The SM line is not visible since it is behind the other lines - all contact interaction models are set to SM above lambda

Technical tests

SM models @3pb

plot_sm_model.png

Effects of systematic variations

  • Correlation coefficients of the LLR with various nuisance parameters from lambda=500 (total counts from June 14 dataset of 10.5nb-1). Only 1000 PDSs per ensemble, will redo with more statistics.
    • in the contact interaction case, the LLR is dominated by the JES. This is explained below smile
  JES relative JES flat shift scale
SM 0.07 -0.34 0.04 0.15
lambda=500 0.66 -0.13 0.07 0.01
  • Complete systematic variations from likelihood-based code .root format):
    plot_smr_syst.png

Side band fit

  • The SM ratio before and after the fit - sideband_fit_50nb.txt
  • The function is implemented in C++. It's "fittedSM_evaluate_ratio" which is the first function in fittedSM.c
  • Automated sideband fit output with 50nb-1:
    sideband_fit_man.png

JES variations

  • Visualization of JES systematics in lambda=500 contact interactions:
    • this is, in effect, a huge signal modeling uncertainty
      plot_ci_jes.png
  • Test of unbinned technique used for SM and contact interaction in [4].
  • Test of binned JES systematics used in q* models (rough models from 2010-Apr-18):
    plot_qs_jes.png

q* modeling plots

  • Test of q* interpolation:
    plot_qs_2shapes.png
  • Visualization of why we use only the core of the q* shapes - there are fits created by Dan with:
    • extended tails (0.18<x<1.82)
    • upper tail fitted to smooth out statistical fluctuations (fit and its chi^2 look great, but I don't have a plot handy to demonstrate that)
      plot_qs_model.png

string resonance modeling plots

plot_str_model.png

Talk drafts

plots for talks

3fb push

Selected LLR plots:
Pythia QCD model
Lambda=2.4TeV Lambda=3.0TeV Lambda=4.0TeV
.png      
.root    

Wiki not ready yet - all plots etc. are in a tar file on lxplus...

Feel good statistic:

  • All numbers here are not yet final...
  • The p-values are for the "with systematics" histogram. They include interpolation within the key bin, and supersede the older p-value number.
  • the fit is not shown for the NLOcorr plot, as it is of very low quality (chi^2/n.d.f. ~74, fails to capture the large upper tail)
SM model NLO (with non perturbative corrections Pythia with k-factor Pythia Flat ratio
plot plot_fg.png not updated plot_fg_pyt.png plot_fg_flat.png

120.0 nb-1, contact interaction results

  with systematics without systematics
Normal view zoomed in Normal view zoomed in
.png clim1_4KI0_12d.png clim1_4Kz0_2I0_12d.png clim2_4KI0_12d.png clim2_4Kz0_3I0_12d.png
.root clim1_4KI0_12d.root N/A clim2_4KI0_12d.root N/A
Notes:
  • The prediction and limit curves all used the observed total counts. So the natural expectation for a smooth curve is false - data fluctuations are apparent here.
    • in particular the "peaks" in LLR for 1150, 1400, and 1600 GeV are related to similar peaks in the total data counts of the 120nb-1 dataset.
    • the LLR jumps from 1700-2000 may be due to the discrete jumps in the turn_on, as in that region, each two lambda (e.g. 1700 and 1750) share the same turn on bin and value. However, this does not full explain the structure
      • these are not statistical fluctuation from the limiter ensemble sizes! Those are basically sqrt(4000)=63 times smaller than the 1sigma band =~0.022 in LLR, which is smaller than the marker size.

Feel good statistic:

  • The p-values are for the "with systematics" histogram. They include interpolation within the key bin, and supersede the older p-value number.
  • the fit is not shown for the NLOcorr plot, as it is of very low quality (chi^2/n.d.f. ~74, fails to capture the large upper tail)
  • plots were overwritten. See AN...

Selected LLR plots:

lambda 1.7TeV 1.85TeV 2.0TeV
.png psd17001I0_12.png psd18501I0_12.png psd20001I0_12.png
.root psd17001I0_12.root psd18501I0_12.root psd20001I0_12.root

50.0 nb-1, contact interaction results

with systematics without systematics
clim1_4Kz0_7I0_05.png clim2_4Kz0_7I0_05.png

Some LLR plots with systematics

Lambda=1050 Lambda=1100
ps10501I0_05.png ps11001I0_05.png

Feel good statistic:

  • The p-values are for the "with systematics" histogram. They include interpolation within the key bin, and supersede the older p-value number.
  • the fit is not shown for the NLOcorr plot, as it is of very low quality (chi^2/n.d.f. ~74, fails to capture the large upper tail)
  • plots were overwritten, can be recreated if needed

11.4 nb-1, contact interaction results

  • Contact limits w. data, from June 23:
    • the purple line is the CLs line - at high lambdas the separation is low and no CLs limit exists
      clim1_4KI0_01.png
  • feel good statistic @ 11.4nb-1:
    • the fit is to the no statistics curve, and of the form [0]*TMath::GammaDist(x,[1]/2,0,[2])
    • the numbers in parenthesis are the uncertainties on the last digits. However, this is a fairly rough estimate (not using Bahadur representation here)
    • the plots with the p-values of the feel good statistics were overwritten, and can be restored if need be.
  • LLR plots at various interesting lambdas:
lambda With systematics
400 psd4001I0_01.png
450 psd4501I0_01.png
500 psd5001I0_01.png
600 psd6001I0_01.png

Older plots for talks

Are exclusion probabilities linear near the limit?

Two examples:
dataset with systematics without systematics
11.4nb-1 data ceff1_4KI0_01.png ceff2_4KI0_01d.png
100nb-1 predictions not made ceff2_6KI0_1.png

  • contact limit plots
integrated luminosity full plot zoom in without systematics
100nb-1 clim1_1KI0.1.png clim1_1Kz0_3I0.1.png clim2_4Kz0_3I0_1.png
300nb-1 clim1_4KI0.3.png clim1_4Kz0_2I0.1.png clim2_1Kz0_3I0_3.png
  • x-sec limits for 700GeV q*:
integrated luminosity full plot zoom in without systematics
300nb-1 xlim0_71_1KI0_3.png xlim0_71_1Kz0_4I0_3.png xlim0_72_1KI0_3.png
  • PLOT IS SUSPECT!
    x-section limits summary for 700GeV q* @ 100nb-1: PLOT IS SUSPECT
    xlim0.71_1K.png
  • limits on 500GeV q* @ 300nb-1, without systematics:
    xlim0_52_1KI0_3.png

Performance with the different "modes" of limit setting

  • LLR for lambda=1TeV, "old style"=each ensemble used only its hypothesis, so that in the NP ensembles the total event counts came from the NP hypothesis.
    • This is a valid analysis, but no the one we want and perform in "data mode" (below). This kind of limit setting implicitly uses the total counts, spoiling our orthogonallity to the dijet spectrum measurement.
      pso10002I0_1.png
  • LLR for lambda=1TeV, predictions mode (both ensembles use the SM total event counts):
    ps10002I0_1.png
  • LLR for lambda=1TeV, data mode (both ensembles use total counts from data), fake data statistics happen to be low (3012 events):
    psd10002I0_1_t3012.png
  • LLR for lambda=1TeV, data mode (both ensembles use total counts from data), fake data statistics happen to be high (3426 events):
    psd10002I0_1_t3426.png

Verifying the choice of minimal stat. uncertainty - 5%

  • New study - mq* = 500GeV at 100nb-1 - the signal starts at the very first bin!
  • Each shaded band represents half a sigma (from -2 to 2) on the SM distribution.
  • The 5% criterion leads to starting with bin #9 (starting from the bin at 156)
  • the absolute statistical errors on the first bin ranged from <1% (bin #3) to >11% (bin #13). Note that bin #13 starts at 489GeV, so about half the signal region is excluded.
  • the statistical errors shows in the summary plots are the sum in quadrature of the statistical uncertainties on the 95% quantile (approximated using the "Bahadur representation") and the statistical uncertainties on the fraction of SM below the nominal cut.

first bin LLR distributions first bin LLR distributions
summary plot min_stat_opt.png no syst. ps500_1472_2I0_1.png
1 ps15001I0.1.png 3 ps500_1472_1I0_1F3.png
5 ps500_1472_1I0_1F5.png.png 7 ps500_1472_1I0_1F7.png
9 ps500_1472_1I0_1F9.png 11 ps500_1472_1I0_1F11.png
13 ps500_1472_1I0_1F9.png    
  • conclusions:
    • when the systematics are held constant, the statistical analysis is not overly sensitive to the choice of the sideband region. In this example the 5% criterion led to a decent choice of cut off, though a lower value may be slightly better.

Sensitivity to uncertainty on shifting

  • same scenario as above, but the first bin is #3.
  • the "1.3" number comes from adding in quadrature the expected uncertainty on a shifting constant fit to the two lowest bins in the data, i.e., in the corresponding sideband. This is for 100nb-1.
shifting uncertainty (in %, absolute) 0 1.1 (nominal) 1.3
LLR distributions ps500_1472_1I0_1_S10_1.png ps500_1472_1I0_1F3.png ps500_1472_1I0_1_S10_1_1_3.png
  • Conclusions: no significant sensitivity, can afford using only these two bins as the sideband region.

What do things look like with a badly fluctuating dataset?

  • Study done at 100nb-1. Found a pseudo dataset with a shift ~2sigma from expeced: -0.0130, fitted uncertainty: 0.0067.
  • ratio of a PDS with a particularly Bad Shift (-0.0130 +/- 0.0067):
    bs_pds_ratio.png
  • contact summary for a PDS with a particularly Bad Shift (-0.0130 +/- 0.0067):
    clim1_1001z0_9I0_1_bs_PDF_with_its_ensembles.png
  • contact summary for a PDS with a particularly Bad Shift (-0.0130 +/- 0.0067), but with the normal ensembles:
    clim1_4Kz0_3I0_1_bs_PDF_normal_ensembles.png

7.2 nb-1, contact interaction results

plots for lambda=500,750GeV, and summary plots with and without systematics were formerly available, but since deleted
  • only the bins above 230GeV are used (optimized for this lumi).
  • the plotting macros don't account for weirdness that happens at low statistics, such as negative predictions. We expect to further process plots for a publication...
    • the odd predictions are since we will only publish with enough data and enough simulated lambda values such that a linear interpolation, such as used to find the limits, suffices.

2.84 nb-1, contact interaction results

  • these plots were mostly overwritten in the wiki page - can be uploaded again if needed.
  • only the bins above 230GeV are used. This was chosen for 10nb-1, and isn't quite optimal for 2.84nb-1.
  • the plotting macros don't account for weirdness that happens at low statistics, such as negative predictions. We expect to further process plots for a publication...
    • the odd predictions are since we will only publish with enough data and enough simulated lambda values such that a linear interpolation, such as used to find the limits, suffices.

Code

  • gzipped tar file for source codes of binom statistics, model, & basic null-hypothesis ensembles tests
    • rBInom.c contains the poisson ratio as a binomial (per-bin) statistics functions (including ROOT wrappers)
    • model.h & model.c contain the model class, which also calculates the multi-bin statistics
    • ensembles.c contains the ensemble_tester class (just basic NULL-hypothesis tests for now).
    • usejr.c loads everything (do root -l usejr.c or from CINT .x usejr.c)
    • rjetUtil.c so far contains only plotting utils, used in rBinom's built in visual tests.

  • gzipped tar file for source codes of discreteDistribution & poisRatDist class
    • discreteDistribution is a generic class, independent of ROOT.
    • poisRatDist analysis specific
      • calculation of R can be optimized further (comments in code on how to do it)
    • can calculate R(1000, 2000) in 17 sec and read it from a file in 0.3 sec
    • improved "effective binning" option
    • pri.c contains the continuum limit, testPRs.c tests it and makes plots with it

Random info

  • plot_sm_jes.png:
    plot_sm_jes.png
  • Contact limits w. approval data, without systematics:
    clim2_4KI0_01d.png
  • dcr_rf1.tgz: gzipped tar file of code and workspace for mock RooStats analysis

Attachments

  • LLR distributions for lambda=3TeV, 3pb-1 (QCD from Pythia):
    cpsdp30001I2_88.png

  • LLR distributions for lambda=3TeV, 3pb-1 (QCD from corrected NLO):
    cpsdn30001I2_88.png

  • 3pb-1 contact limits, without syst., corrNLO, zoomed in:
    clim2n_4Kz0_1I2_88d.png

  • 3pb-1 contact limits, without syst., pythia, zoomed in:
    clim2p_4Kz0_1I2_88d.png

  • LLR distributions for lambda=4TeV, 3pb-1 (QCD from Pythia):
    cpsdp40001I2_88.png

  • 3pb-1 contact limits, corrNLO, zoomed in:
    clim1n_4Kz0_16I2_88d.png

  • 3pb-1 contact limits, Pythia QCD, zoomed in:
    clim1p_4Kz0_2I2_88d.png
Topic attachments
I Attachment History Action Size Date Who Comment
PNGpng bs_pds_ratio.png r1 manage 8.2 K 2010-06-25 - 15:02 AmnonHarel ratio of a PDS with a particularly Bad Shift (-0.0130 +/- 0.0067)
PNGpng ceff1_4KI0_01.png r1 manage 13.0 K 2010-07-06 - 12:15 AmnonHarel exclusion probability for 11.4nb-1 (with syst)
PNGpng ceff2_4KI0_01d.png r1 manage 12.5 K 2010-07-06 - 12:28 AmnonHarel exclusion probability for 11.4nb-1 (w.o. syst)
PNGpng ceff2_6KI0_1.png r1 manage 12.3 K 2010-07-06 - 12:14 AmnonHarel exclusion probability for 100nb-1 (w.o. syst)
PNGpng clim1_1001z0_9I0_1_bs_PDF_with_its_ensembles.png r1 manage 16.8 K 2010-06-25 - 15:14 AmnonHarel contact summary for a PDS with a particularly Bad Shift (-0.0130 +/- 0.0067)
PNGpng clim1_1KI0.1.png r1 manage 16.2 K 2010-05-26 - 12:36 AmnonHarel contact limits, 100nb-1
Unknown file formatroot clim1_1KI0_12d.root r1 manage 16.3 K 2010-07-18 - 21:03 AmnonHarel Canvas of low-statistics contact interaction limits, 120nb-1 dataset
PNGpng clim1_1Kz0_3I0.1.png r1 manage 15.6 K 2010-05-26 - 12:36 AmnonHarel contact limits, zoomed in, 100nb-1
Unknown file formatroot clim1_2500I0_12d.root r1 manage 16.3 K 2010-07-18 - 21:54 AmnonHarel Canvas of low-statistics(2.5K) contact interaction limits, 120nb-1 dataset
PNGpng clim1_4KI0.3.png r1 manage 14.7 K 2010-05-26 - 11:18 AmnonHarel contact limits, 300nb-1
PNGpng clim1_4KI0_01.png r1 manage 16.6 K 2010-06-23 - 15:11 AmnonHarel Contact limits w. data, from June 23
PNGpng clim1_4KI0_12d.png r1 manage 18.8 K 2010-07-19 - 13:51 AmnonHarel contact limits, 120nb-1 dataset
Unknown file formatroot clim1_4KI0_12d.root r1 manage 16.7 K 2010-07-19 - 13:49 AmnonHarel contact limits, 120nb-1 dataset
PNGpng clim1_4Kz0_2I0.3.png r1 manage 16.0 K 2010-05-26 - 11:17 AmnonHarel contact limits, zoomed in, 300nb-1
PNGpng clim1_4Kz0_2I0_12d.png r1 manage 20.1 K 2010-07-19 - 13:50 AmnonHarel contact limits, 120nb-1 dataset, zoom in
PNGpng clim1_4Kz0_3I0_05d.png r1 manage 16.5 K 2010-07-13 - 20:08 AmnonHarel Contact limits w. 5-nb-1 of data
PNGpng clim1_4Kz0_3I0_1_bs_PDF_normal_ensembles.png r1 manage 16.6 K 2010-06-25 - 15:14 AmnonHarel contact summary for a PDS with a particularly Bad Shift (-0.0130 +/- 0.0067), but with the normal ensembles
PNGpng clim1_4Kz0_7I0_05.png r1 manage 17.8 K 2010-07-14 - 12:09 AmnonHarel contact summary 50nb-1, i.e. ICHEP limits
PNGpng clim1_8KI0_12d.png r1 manage 17.8 K 2010-07-17 - 22:00 AmnonHarel contact limits, 120nb-1 dataset
PNGpng clim1_8Kz0_2I0_12d.png r1 manage 19.9 K 2010-07-17 - 22:00 AmnonHarel contact limits, zoomed in, 120nb-1 dataset
PNGpng clim1n_4Kz0_16I2_88d.png r1 manage 19.1 K 2010-09-07 - 04:33 AmnonHarel 3pb-1 contact limits, corrNLO, zoomed in
PNGpng clim1p_4Kz0_2I2_88d.png r2 r1 manage 19.1 K 2010-09-07 - 05:43 AmnonHarel 3pb-1 contact limits, Pythia QCD, zoomed in
PNGpng clim2_1Kz0_3I0_3.png r1 manage 17.0 K 2010-05-27 - 13:52 AmnonHarel contact limits, 300nb-1, without syst.
PNGpng clim2_4KI0_01d.png r1 manage 17.5 K 2010-07-06 - 12:39 AmnonHarel Contact limits w. approval data, without systematics
PNGpng clim2_4KI0_05.png r1 manage 18.1 K 2010-07-13 - 16:27 AmnonHarel contact summary 50nb-1, no syst
PNGpng clim2_4KI0_12d.png r1 manage 18.9 K 2010-07-18 - 11:56 AmnonHarel contact limits without systematics, 120nb-1 dataset
Unknown file formatroot clim2_4KI0_12d.root r1 manage 16.4 K 2010-07-18 - 12:02 AmnonHarel Canvas for contact limits without systematics, 120nb-1 dataset
PNGpng clim2_4Kz0_3I0_1.png r1 manage 16.5 K 2010-05-27 - 14:32 AmnonHarel contact limits, 100nb-1, without systematics
PNGpng clim2_4Kz0_3I0_12d.png r1 manage 21.6 K 2010-07-18 - 11:56 AmnonHarel contact limits without systematics, 120nb-1 dataset, zoomed in
PNGpng clim2_4Kz0_7I0_05.png r1 manage 19.7 K 2010-07-14 - 11:45 AmnonHarel contact summary 50nb-1, no syst
PNGpng clim2n_4Kz0_1I2_88d.png r1 manage 21.5 K 2010-09-06 - 17:45 AmnonHarel 3pb-1 contact limits, without syst., corrNLO, zoomed in
PNGpng clim2p_4Kz0_1I2_88d.png r1 manage 21.5 K 2010-09-06 - 20:25 AmnonHarel 3pb-1 contact limits, without syst., pythia, zoomed in
C source code filec clopper.c r1 manage 5.9 K 2009-06-14 - 20:15 AmnonHarel Attachment doesn't exist anymore, so delete fails
PDFpdf cmsnote_v1.2.pdf r1 manage 228.0 K 2009-10-08 - 17:08 AmnonHarel Draft of internal AN
PNGpng cpsdn30001I2_88.png r1 manage 18.0 K 2010-09-06 - 17:14 AmnonHarel LLR distributions for lambda=3TeV, 3pb-1 (QCD from NLO_NPcorr)
Unknown file formatroot cpsdn30001I2_88.root r1 manage 16.0 K 2010-09-07 - 02:49 AmnonHarel LLR distributions for lambda=3TeV, 3pb-1 (QCD from NLO_NPcorr)
PNGpng cpsdp30001I2_88.png r1 manage 18.4 K 2010-09-06 - 16:59 AmnonHarel LLR distributions for lambda=3TeV, 3pb-1 (QCD from Pythia)
Unknown file formatroot cpsdp30001I2_88.root r1 manage 16.0 K 2010-09-07 - 02:48 AmnonHarel LLR distributions for lambda=3TeV, 3pb-1 (QCD from Pythia)
PNGpng cpsdp40001I2_88.png r1 manage 16.8 K 2010-09-07 - 03:07 AmnonHarel LLR distributions for lambda=4TeV, 3pb-1 (QCD from Pythia)
Compressed Zip archivetgz dcr_rf1.tgz r1 manage 9.8 K 2010-08-24 - 16:55 AmnonHarel gzipped tar file of code and workspace for mock RooStats analysis
Compressed Zip archivetgz dists20090302.tgz r1 manage 18.4 K 2009-03-02 - 14:24 AmnonHarel source codes
Compressed Zip archivetgz jet_ratio_null_macros_20090305.tgz r1 manage 18.2 K 2009-03-05 - 14:12 AmnonHarel source codes with first binom implementation
PNGpng june14_data_check.png r1 manage 11.1 K 2010-06-16 - 19:25 AmnonHarel Simple check (fitting a constant to sideband region) of June14 (afternoon) data
PNGpng min_stat_opt.png r2 r1 manage 17.0 K 2010-05-25 - 18:51 AmnonHarel Optimizing the choice of the minimal statistical uncertainty @ 100nb-1
PNGpng min_stat_opt_mqs500.png r2 r1 manage 18.9 K 2010-05-29 - 13:48 AmnonHarel  
PNGpng plot_ci_100nb.png r1 manage 19.7 K 2010-05-23 - 17:34 AmnonHarel  
PNGpng plot_ci_jes.png r1 manage 20.7 K 2010-06-20 - 10:57 AmnonHarel Visualization of JES systematics in lambda=500 contact interactions
PNGpng plot_ci_model.png r7 r6 r5 r4 r3 manage 19.1 K 2010-09-05 - 23:39 AmnonHarel Contact interaction models @3pb
Unknown file formatroot plot_ci_model.root r1 manage 20.2 K 2010-06-22 - 20:31 AmnonHarel contact interaction models
PNGpng plot_fg.png r10 r9 r8 r7 r6 manage 17.7 K 2010-09-12 - 16:15 AmnonHarel feel good statistic for NLOcorr @ 3pb-1
Unknown file formatroot plot_fg.root r7 r6 r5 r4 r3 manage 17.3 K 2010-09-03 - 12:21 AmnonHarel canvas of "feel good" statistic plot
PNGpng plot_fg_flat.png r1 manage 21.6 K 2010-09-06 - 20:32 AmnonHarel feel good statistic for flat model @ 3pb-1
PNGpng plot_fg_kpyt.png r3 r2 r1 manage 21.6 K 2010-07-16 - 10:20 AmnonHarel feel good statistic @ 120nb-1 w.r.t. pythia with k-factor
PNGpng plot_fg_pyt.png r4 r3 r2 r1 manage 21.0 K 2010-09-06 - 20:32 AmnonHarel feel good statistic for Pythiar @ 3pb-1
PNGpng plot_qs_2shapes.png r1 manage 17.4 K 2010-04-20 - 18:14 AmnonHarel Test of q* interpolation
PNGpng plot_qs_jes.png r1 manage 20.5 K 2010-04-19 - 17:57 AmnonHarel Test of binned JES systematics used in q* models (rough models from 2010-Apr-18)
PNGpng plot_qs_model.png r2 r1 manage 22.9 K 2010-05-26 - 12:33 AmnonHarel Added 500 GeV (smoothed version from Dan, no tails), 100nb-1 plot
PNGpng plot_sm_jes.png r4 r3 r2 r1 manage 19.3 K 2010-09-09 - 11:45 AmnonHarel  
Unknown file formatroot plot_sm_jes.root r4 r3 r2 r1 manage 19.7 K 2010-09-09 - 11:45 AmnonHarel JES systematics in SM
PNGpng plot_sm_model.png r1 manage 23.6 K 2010-09-06 - 00:09 AmnonHarel SM models @3pb
PNGpng plot_smr_syst.png r4 r3 r2 r1 manage 24.6 K 2010-09-09 - 10:16 AmnonHarel Systematic variations of the SM ratio (update RooStats like code, 3pb-1 dataset)
Unknown file formatroot plot_smr_syst.root r2 r1 manage 20.6 K 2010-09-09 - 10:17 AmnonHarel Canvas of Systematic variations of the SM ratio (update RooStats like code, 3pb-1 dataset)
PNGpng plot_str_model.png r1 manage 23.5 K 2010-08-13 - 13:32 AmnonHarel String models
PNGpng ps10002I0_1.png r1 manage 17.3 K 2010-06-14 - 14:14 AmnonHarel LLR for lambda=1TeV, predictions mode
PNGpng ps10501I0_05.png r1 manage 19.1 K 2010-07-14 - 12:10 AmnonHarel LLR for lambda=1.05TeV, 50nb-1
PNGpng ps11001I0_05.png r1 manage 19.8 K 2010-07-14 - 12:09 AmnonHarel LLR for lambda=1.1TeV, 50nb-1
PNGpng ps15001F11.png r2 r1 manage 14.6 K 2010-05-25 - 19:26 AmnonHarel first bin #11
PNGpng ps15001F13I0.1.png r1 manage 14.6 K 2010-05-25 - 19:26 AmnonHarel first bin #13
PNGpng ps15001F5.png r2 r1 manage 14.6 K 2010-05-25 - 19:23 AmnonHarel first bin #5
PNGpng ps15001F7.png r2 r1 manage 14.6 K 2010-05-25 - 19:24 AmnonHarel first bin #7
PNGpng ps15001F9.png r2 r1 manage 14.6 K 2010-05-25 - 19:25 AmnonHarel first bin #9
PNGpng ps15001I0.1.png r1 manage 14.5 K 2010-05-25 - 18:53 AmnonHarel  
PNGpng ps4001I0_01.png r1 manage 15.2 K 2010-06-23 - 15:24 AmnonHarel LLR, lambda=400, 11.4nb-1
PNGpng ps4501I0_01.png r1 manage 15.0 K 2010-06-23 - 15:23 AmnonHarel LLR, lambda=450, 11.4nb-1
PNGpng ps500_1472_1I0_1F11.png r1 manage 15.3 K 2010-05-29 - 13:09 AmnonHarel LLR dists, mq*=500, 100nb-1, first bin=11
PNGpng ps500_1472_1I0_1F3.png r1 manage 13.9 K 2010-05-29 - 13:48 AmnonHarel LLR dists, mq*=500, 100nb-1, first bin=3
PNGpng ps500_1472_1I0_1F5.png r1 manage 14.4 K 2010-05-29 - 11:46 AmnonHarel LLR dists, mq*=500, 100nb-1, first bin=5
PNGpng ps500_1472_1I0_1F7.png r1 manage 13.9 K 2010-05-29 - 13:08 AmnonHarel LLR dists, mq*=500, 100nb-1, first bin=7
PNGpng ps500_1472_1I0_1F9.png r1 manage 14.5 K 2010-05-29 - 11:46 AmnonHarel LLR dists, mq*=500, 100nb-1, first bin=9
PNGpng ps500_1472_1I0_1_S10_1.png r1 manage 14.9 K 2010-05-29 - 14:59 AmnonHarel LLR distributions, mqs*500, shifting uncertainty at 0 (first bin #3)
PNGpng ps500_1472_1I0_1_S10_1_1_3.png r1 manage 15.0 K 2010-05-29 - 14:58 AmnonHarel LLR distributions, mqs*500, shifting uncertainty at 1.3% (absolute)
PNGpng ps500_1472_2I0_1.png r2 r1 manage 16.4 K 2010-05-29 - 11:45 AmnonHarel LLR dists, mq*=500, 100nb-1, first bin=9, without systematics
PNGpng ps6001I0_01.png r1 manage 17.7 K 2010-06-23 - 15:15 AmnonHarel LLR, lambda=600, 11.4nb-1
PNGpng psd10002I0_1_t3012.png r1 manage 15.4 K 2010-06-15 - 10:37 AmnonHarel LLR for lambda=1TeV, data mode, fake data statistics happen to be low (3012 events)
PNGpng psd10002I0_1_t3426.png r1 manage 15.5 K 2010-06-15 - 10:38 AmnonHarel LLR for lambda=1TeV, data mode, fake data statistics happen to be high (3426 events)
PNGpng psd17001I0_12.png r1 manage 17.2 K 2010-07-19 - 16:15 AmnonHarel LLR dists, mq*=1700, 120nb-1 dataset
Unknown file formatroot psd17001I0_12.root r1 manage 16.0 K 2010-07-19 - 16:14 AmnonHarel LLR dists, mq*=1700, 120nb-1 dataset
PNGpng psd18501I0_12.png r1 manage 17.8 K 2010-07-19 - 16:15 AmnonHarel LLR dists, mq*=1850, 120nb-1 dataset
Unknown file formatroot psd18501I0_12.root r1 manage 16.0 K 2010-07-19 - 16:13 AmnonHarel LLR dists, mq*=1850, 120nb-1 dataset
PNGpng psd20001I0_12.png r1 manage 18.3 K 2010-07-19 - 16:15 AmnonHarel LLR dists, mq*=2000, 120nb-1 dataset
Unknown file formatroot psd20001I0_12.root r1 manage 16.1 K 2010-07-19 - 16:13 AmnonHarel LLR dists, mq*=2000, 120nb-1 dataset
PNGpng psd5001I0_01.png r1 manage 15.1 K 2010-06-21 - 00:35 AmnonHarel LLR lambda=500, w.syst,11.4nb
PNGpng pso10002I0_1.png r1 manage 15.7 K 2010-06-14 - 14:13 AmnonHarel LLR for lambda=1TeV, "old style"=NP hypothesis used for total counts
PDFpdf ratio10.pdf r2 r1 manage 80.9 K 2010-08-05 - 13:46 AmnonHarel Draft of talk for EXO-multijet working meeting
Compressed Zip archivetgz rj_macros_20100622.tgz r1 manage 111.9 K 2010-06-23 - 00:01 AmnonHarel Statistical analysis macros
Compressed Zip archivetgz rj_macros_20100623b.tgz r1 manage 113.8 K 2010-06-23 - 15:35 AmnonHarel Statistical analysis macros (added CLs)
Compressed Zip archivetgz rj_macros_20100629.tgz r1 manage 115.0 K 2010-06-29 - 10:28 AmnonHarel Statistical analysis
Compressed Zip archivetgz rj_macros_20100819.tgz r1 manage 125.7 K 2010-08-31 - 18:04 AmnonHarel Statistical analysis (cleaned up + string resonances)
Compressed Zip archivetgz rjetAN1.1plotters.tgz r1 manage 1.2 K 2009-09-30 - 16:23 AmnonHarel Plotting macros ofr AN
Compressed Zip archivetgz rjetAN1.2.tgz r3 r2 r1 manage 144.7 K 2009-10-12 - 12:25 AmnonHarel Draft of internal AN (latex and eps source, version C)
Texttxt sideband_fit_50nb.txt r1 manage 1.5 K 2010-07-13 - 10:00 AmnonHarel  
PNGpng sideband_fit_man.png r1 manage 11.2 K 2010-07-13 - 10:00 AmnonHarel Automated sideband fit output with 50nb-1
PNGpng sm_ratio_man.png r2 r1 manage 11.2 K 2010-06-16 - 14:17 AmnonHarel SM ratio (1st try at NLO fits in stat. code)
PDFpdf strings_at_LHC_luest.pdf r1 manage 5293.8 K 2009-10-14 - 19:21 AmnonHarel Luest's talk on "String at LHC"
Unknown file formatroot tf1_fitResults_dataMC_june17.root r1 manage 167.8 K 2010-06-21 - 00:11 AmnonHarel Jim's latest data summary
Compressed Zip archivetgz toDan20100412.tgz r1 manage 13.5 K 2010-04-12 - 18:04 AmnonHarel Tar file for Dan - for qstar models
Unknown file formatroot total_counts_120inb.root r1 manage 13.4 K 2010-07-18 - 22:11 AmnonHarel data total for 120nb-1 dataset
Unknown file formatroot total_syst_qcd.root r1 manage 7.2 K 2010-06-21 - 00:12 AmnonHarel Jim's systematics summary (for the feel_good statistic)
PNGpng xlim0.71_1K.png r1 manage 15.5 K 2010-05-17 - 08:35 AmnonHarel x-section limits summary for 700GeV q* @ 100nb-1
PNGpng xlim0_52_1KI0_3.png r1 manage 17.2 K 2010-05-27 - 14:35 AmnonHarel limits on 500GeV q* @ 300nb-1, without systematics
PNGpng xlim0_52_400I0_3.png r1 manage 17.0 K 2010-05-27 - 13:58 AmnonHarel Very rough 1st look at limits on 500GeV q*
PNGpng xlim0_71_1KI0_3.png r1 manage 16.5 K 2010-05-26 - 14:23 AmnonHarel x-sec limits for 700GeV q* @ 300nb-1
PNGpng xlim0_71_1Kz0_4I0_3.png r1 manage 18.4 K 2010-05-26 - 14:24 AmnonHarel x-sec limits for 700GeV q* @ 300nb-1, zoomed in
PNGpng xlim0_72_1KI0_3.png r1 manage 17.1 K 2010-05-27 - 13:33 AmnonHarel x-sec limits for 700GeV q* @ 300nb-1, no syst
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Topic revision: r121 - 2010-09-12 - AmnonHarel
 
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