Results from 2007-08 data unblinding on point source analysis with the EM algorithm
DiPhoton + MET: Towards Unblinding of the 5 fb -1 Analysis
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DiPhoton + MET: Towards Unblinding of the 5 fb-1 Analysis
• Reminder about 1 fb-1 analysis• New strategy: A B C analyses• Optimization• MET Blues• Background estimates• Unblinding of A, preparation for B unblinding
Bruce Schumm29 Feb 2012
1 fb-1 Analysis: Thumbnail Sketch
(First-order) signal selection straightforward:• 2 tight isolated photons with ET 25 GeV
• ETmiss 125 GeV
Optimization based only on ETmiss cut value
Optimization geared towards high-mass Gluino for broad range of bino masses (50 GeV to Mgluino)
Analysis Improvements
Overlap Criteria- Reverse /e overlap criterion (have medium e kill )- e fake rate goes from 0.049-0.168 to 0.025-0.075- 13% signal efficiency loss
Conversion pixel requirements- Conversion tracks can have no pixel hits- e backgrounds reduced by 43% (42% for events with one conversion; 61% for events with two conversions)- 13% signal efficiency loss
Conversion categories- Division into three conversion categories suggested- No benefit if background is ~0
Two scales characterize GMSB production/decay
• Missing energy (mostly bino mass; also bino boost) MET
• Total energy, including photons (sparticle mass) HT
Analysis A: High-mass sparticle, high-mass binoLarge MET, moderate HT
Analysis B: High-mass sparticle, low-mass binoModerate MET, large HT
Analysis C: SPS8 (direct gaugino production; sparticles too heavy)Moderate-to-large MET; NO HT (most like 1 fb-1 analysis)
Also: 1 fb-1 backgrounds observed to have photons close to MET (photon to MET) cut explored for A,B,C analsyes
Optimization: General Principles
C
Optimization of A, B, C Points: Results
Optimization results:All use photon ET > 50 GeV.
Figure of merit rather flat in use either 0.5 or no cut
Drop unjustified significant digits
Target Model
ETmiss HT
A (900,800) 200 600 0.5
B (900,50) 100 1100 ---
C SPS8 170 125 --- 0.5
Background: Definition of “QCD” Control Samples
We model the ETmiss distribution of selected events with
no intrinsic missing energy via two control samples: QCDg and QCDgg.
A “control photon” satisfies the loose, but not the tight, selection requirement for two shower quantities: the shower shape in the shower core {fracs1} and the shower width {weta1} in the first sampling of the electromagnetic calorimeter.
QCDg has one such control photon; QCDgg has two.
QCDg, QCDgg, and gg – MET_SimpRefFinal
2/16/2012 10
No resemblance of control sample eT
miss shape to that of the signal
QCDg, QCDgg, and gg – MET_LocHadTopo
2/16/2012 11 Propose to use LocHadTopo for ET
miss
N.B.: Studies with +Njets MC suggest high-ET
miss tails a bit larger for SimpMetRefFinal
BACKGROUNDS
QCDgControl Sample(DESY)
E- Control Sample(Penn)
Overlap ?(DESY)
Missed?(SCIPP)
EW Background from e- control sample Brig, Jack
N.B.: “Signal” is e-
Scale factors from Ze/ZeeMultiply these by “signal” numbers on previous page
Pseudo-photon control sample (Peter, Martin)
• QCDg distribution provides shape and tails
• scale to signal (gamma-gamma) in low-MET region (ET
miss<20 GeV)
SIGNAL BLINDED FOR MET > 100 GEV
SIGNAL BLINDED FOR MET > 100 GEV
SIGNAL BLINDED FOR MET > 100 GEV
Background Summary
QCD EW TOTA 0.10 0.10 0.03 0.03 0.13 0.13
B 0+0.38-0.0 0.03 0.03 0.03+0.41
-0.03
C 0.7 ? 1.2 ? 1.9 ?
1 fb-1 0.8 0.7 3.1 1.5 4.1 1.7*
*Includes a 0.2 event contribution from “irreducible” backgrounds (two real photons) that are negligible in A
and B regions; needs to be checked for C
Missed/Overlapped backgrounds study: No significant corrections suggested (up to smallish uncertainties)
A:ggm_900_800 -> LL: 142.4, sig: 16.9, #S: 21.3, #B 0.01ggm_1000_800 -> LL: 39.8, sig: 8.9, #S: 7.1, #B 0.01ggm_1100_800 -> LL: 10.8, sig: 4.7, #S: 2.4, #B 0.01ggm_1200_800 -> LL: 3.4, sig: 2.6, #S: 0.9, #B 0.01
C:sps8_170 -> LL: 22.2, sig: 6.7, #S: 11.9, #B 0.9sps8_180 -> LL: 14.5, sig: 5.4, #S: 8.9, #B 0.9sps8_200 -> LL: 6.6, sig: 3.6, #S: 5.3, #B 0.9sps8_220 -> LL: 2.7, sig: 2.3, #S: 3.0, #B 0.9sps8_240 -> LL: 1.2, sig: 1.5, #S: 1.8, #B 0.9
B:ggm_900_50 -> LL: 45.1, sig: 9.5, #S: 10.3, #B 0.05ggm_1000_50 -> LL: 13.6, sig: 5.2, #S: 4.0, #B 0.05ggm_1100_50 -> LL: 2.7, sig: 2.3, #S: 1.2, #B 0.05ggm_1200_50 -> LL: 0.4, sig: 0.85, #S: 0.3, #B 0.05
A word on the 5 fb-1 reach (not fully-optimal analyses)
Limits for 1 fb-1 about 820 GeV
for analysis-A-like scenario and ~145
TeV for SPS8 trajectory
Unblinding Procedures
1) Obtain Ed-Board approval (done 2/21/12)
2) Examine HT sidebands to build confidence in background modeling, especially without the cut (B analysis)
3) Since B sidebands (up to HT=1100 GeV) are almost A signal region (HT > 600 GeV) explore and unblind A before exploring B sidebands
HT Sidebands for Analysis A: 200 < HT < 400
MET Cut
Includes cut
HT Sidebands for Analysis A: 400 < HT < 600
MET Cut
Includes cut
Analysis A Unblinded
No signal for MET > 200;Should set strong limit for high Bino mass (note that 200 GeV cut has avoided one background event)
Includes cut
Analysis B Blinded
HT > 1100No cut
HT Sidebands for Analysis B: 500 < HT < 800
500 < HT < 800 No cut
HT Sidebands for Analysis B: 800 < HT < 1100
800< HT < 1100No cut
How well do we understand these backgrounds? Should
we fear not using the cut?
e- Control Sample (EW Bkgds); No Cut
Scale by e rate to get expected background
e- Control Sample (EW Bkgds); No Cut
Scale by e rate to get expected background
MET 50-75 75-100 100-200 > 200
EW 6.6 1.6 2.2 0.15
QCD 60.0 5.9 1.8 0.26
Exp. Bkgd 66.6 7.5 4.0 0.41
events 64 5 3 0
200 < HT < 1100 Sideband: Expected (assuming no signal) vs. Observed Rates
With cut
MET 50-75 75-100 100-200 > 200
EW 7.2 2.0 2.5 0.18
QCD 84.4 7.7 2.6 0.31
Exp. Bkgd 91.5 9.6 5.1 0.49
events 82 8 3 2
cut removed
200 < HT < 1100 Sideband: Expected (assuming no signal) vs. Observed Rates
Summary
Three analyses geared towards high&low mass bino, SPS8
High-mass bino analysis: 0 signal events
Low-mass bino ready to unblind; SPS8 requires further background studies (underway)
Verbatim 2011 analysis applied to 5 fb-1 150-200 GeV increase in limits
2012 analysis improvements 250-400 GeV increase
CMS did better than ATLAS with 1 fb-1 because of• More favorable interpretation of GGM model• Luck
but per fb-1, our analysis was more sensitive
BACKUP
Also: Limit of > 145 TeV set on SPS8 SUSY Breaking scale
Analysis background-limited; sparticle cross section goes as ~M-9
reoptimize!
Photon Et Optimization (1 fb-1 Analysis) Helenka
Choose Cut of50/50
Cross-check with MET distribution from Zee (background real ?)
No QCDg above 100 GeV Less than 1 event at 95% CL
Martin
Overlap Between QCDg and EW backgrounds
Missed Backgrounds (?)
• Since our “QCD” backgrounds are estimated by normalizing control samples (QCDg, Zee) to low-MET signal, they should be comprehensively accounted for
• “EW” (W,top) backgrounds estimated via e- control sample Assumes all W,top contributions have at least one e fake
• Is this true? If not, what is character of the “missed” component?
• Might the “missed” component in fact be incorporated into the QCD control sample (pseudo-photon) estimate?
Dan
According to MC, what fraction of EW background is due to e fakes?
MC
Of the 25% that is “missed”No e With e
+ 18.9 0.0
+ jet 47.5 5.0
+ 3.0 2.9
+ W l 22.9 0.0
18.9% + 47.5% = 66.4% 2/3 is expected to be reflected in the pseudo-photon sampleThis 2/3 may well be the source of the “EW-contamination” in the pseudo-photon sample (cross-check underwayThis component is neither missed nor double-counted! Add “QCD” and “EW” backgrounds linearly (values and errors)