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Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration. Louie Corpe, Imperial College 1 31.08.16 Higgs Hunting 2016, Paris. Young Scientists Forum - Part 1 Public analysis summary: CMS-PAS-HIG-16-020

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Page 1: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV

Louie Corpe (Imperial College) on behalf of the CMS Collaboration.

Louie Corpe, Imperial College 1

31.08.16 Higgs Hunting 2016, Paris.

Young Scientists Forum - Part 1

Public analysis summary: CMS-PAS-HIG-16-020

Page 2: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Introduction

Louie Corpe, Imperial College 2

• H→ɣɣ: key role in discovery of the Higgs.

• Clean final state: two highly energetic photons. However, low branching fraction (~0.2%) and large irreducible background.

• In a nutshell: Look for ‘bump’ on diphoton invariant mass (mɣɣ) spectrum.

• General strategy: categorise events by resolution and production topology (using additional objects in the event).

• This talk presents first results with 12.9 fb-1

of prompt data collected by CMS in 2016 at √s=13 TeV.

• Increased Higgs cross-section (XS): similar statistical sensitivity to Run 1 analysis.

Run 1 result:Sig+Bkg fit, all

categories summed

Page 3: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

BDT score of the photon ID1− 0.8− 0.6− 0.4− 0.2− 0 0.2 0.4 0.6 0.8 1

Even

ts210

310

410

510

610

710

810DataSimulation:

4 = 125 GeV)x10H

(mγγ→Htotal background+stat.uncert.γ-γ

-jetγjet-jet

DataSimulation:

4 = 125 GeV)x10H

(mγγ→Htotal background+stat.uncert.γ-γ

-jetγjet-jet

DataSimulation:

4 = 125 GeV)x10H

(mγγ→Htotal background+stat.uncert.γ-γ

-jetγjet-jet

DataSimulation:

4 = 125 GeV)x10H

(mγγ→Htotal background+stat.uncert.γ-γ

-jetγjet-jet

DataSimulation:

4 = 125 GeV)x10H

(mγγ→Htotal background+stat.uncert.γ-γ

-jetγjet-jet

DataSimulation:

4 = 125 GeV)x10H

(mγγ→Htotal background+stat.uncert.γ-γ

-jetγjet-jet

(13 TeV)-112.9 fbCMS Preliminary

Vertex ID and photon/diphoton ID

Louie Corpe, Imperial College 3

Vertex ID

Photon ID and diphoton pairs• Photon ID selects prompt photons against π0/

η→ɣɣ and electrons. • Multivariate approach combining shower shape

and isolation variables. • A further BDT is used to identify signal-like

diphoton pairs: kinematics, high photon ID scores, correct vertex probability and good mass resolution.

• Vertex assignment important for mɣɣ resolution. |zchosen- ztrue|<1 cm ⇒ angular contribution negligible wrt energy resolution.

• Vertex ID uses Multivariate approach (BDT):exploits tracks recoiling from ɣɣ system and conversion tracks. Estimate of vertex probability extracted for use in diphoton classification.

α

Eɣ1

Eɣ2

Page 4: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

γ γTransformed BDT0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1

Even

ts/0

.02

1

10

210

310

410

510

610

710 Datajet jet jetγγ γ

MC stat. uncert.

ggHVBFVHttH

Preliminary CMS (13TeV)-112.9 fb

Simulation background =125 GeVH

, mγγ→SM H

Event categorisation

Louie Corpe, Imperial College 4

• Events with additional objects characteristic of specific production modes are tagged, and remaining events are categorised using BDTɣɣ.

• TTH: look for hadronic or leptonic decays of tops quarks.

• VBF: Distinctive 2-jet + 2-photon signature, use BDTs to identify VBF jets and split VBF Tags by mass resolution.

• Inclusive categories split by mass resolution using BDTɣɣ output.

TTH Leptonic

TTH Hadronic

VBF Tag 0

Untagged 0

VBF Tag 1

Untagged 1

Untagged 2

Untagged 3

}}

}Target ttH (~0.5 pb)

Events categorised by top decay

Target VBF (~3.8 pb). Events categorised by sensitivity

Inclusive categories, mostly populated by ggH (~49 pb)

and VH (~2 pb). Events categorised by sensitivity using BDT.

Page 5: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

(GeV)Hm121 122 123 124 125 126 127 128 129

Acc

epta

nce

(%)

×Ef

ficie

ncy

36

38

40

42

44

Simulation Preliminary CMS TeV 13

γγ→H

A× εSignal model

syst. uncertaintyσ 1 ±

• Signal Model: For each category/process, fit sum of Gaussians to mɣɣ distribution, separately for:

• Vertex correctly identified: mass resolution dominated by energy resolution.

• Vertex incorrectly identified: mass resolution dominated by uncert. on vertex position.

• Smooth parametric model in each process/category. Interpolated between 7 mass points in the range 120-130 GeV.

• Background model: data-driven method. Sidebands used to determine background shape under signal peak in mɣɣ distribution.

• Treat choice of background function as discrete parameter in final minimisation.

Signal and Background Modelling

Louie Corpe, Imperial College 5

(GeV)γγm105 110 115 120 125 130 135 140

Even

ts /

( 0.5

GeV

)

0

10

20

30

40

50

60

70

80

FWHM = 3.58 GeV

All Categoriesγγ→H

Simulation

modelParametric

= 1.88 GeVeffσ

13 TeVCMS Simulation Preliminary

Page 6: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Diphoton mass spectrumAll categories summed

Louie Corpe, Imperial College 6

• Invariant mass spectrum. Background-only and signal-plus-background fits to the data are shown.

• Clear Higgs signal, visible by eye when background subtracted. Applying the weighting by sensitivity makes the peak even more obvious.

Even

ts /

GeV

0

1000

2000

3000

4000

5000

6000

7000

8000

9000

DataS+B fitB component

σ1 ±σ2 ±

All categories=0.95µ=126.0 GeV, Hm --

Preliminary CMS TeV) (13-1 12.9 fbγγ→H

(GeV)γγm100 110 120 130 140 150 160 170 180

100−

0

100

200 B component subtracted

S/(S

+B) W

eigh

ted

Even

ts /

GeV

0

1000

2000

3000

4000

5000

DataS+B fitB component

σ1 ±σ2 ±

S/(S+B) weightedAll categories=0.95µ=126.0 GeV, Hm

--

Preliminary CMS TeV) (13-1 12.9 fbγγ→H

(GeV)γγm100 110 120 130 140 150 160 170 180

100−

0

100

200 B component subtracted

Unweighted Weighted

Page 7: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

P-value and signal strength

Louie Corpe, Imperial College 7

• We report an observation with significance 5.6σ where 6.2σ was expected for the SM Higgs boson at mH=125.09 GeV. The maximum significance of 6.1σ is observed at 126 GeV.

• Best fit signal strength (XS*BR) relative to SM, for profiled MH, is found to be:

(GeV)Hm116 118 120 122 124 126 128 130 132 134

Loca

l p-v

alue

10−10

9−10

8−10

7−10

6−10

5−10

4−10

3−10

2−10

1−10

1σ1 σ2

σ3

σ4

σ5

σ6

Observed

Expected

= 125.09 GeVHmExpected

Preliminary CMSγγ→H

(13TeV)-112.9 fb

µ0.6 0.7 0.8 0.9 1 1.1 1.2 1.3 1.4 1.5

ln L

∆-2

0

1

2

3

4

5

6

0.18−0.21+ = 0.95 µ

Preliminary CMSγγ→H

TeV) (13-112.9 fb

ProfiledHm

Page 8: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Fiducial Cross-section measurement

Louie Corpe, Imperial College 8

(fb)fidσ30 40 50 60 70 80 90 100 110

ln L

∆-2

0

1

2

3

4

5

6

fb 22− 18+ = 69 fidσ

HXSWG YR4+ aMC@NLO

=125.09 GeVHm

Preliminary CMS

H, profiling mγγ→H

(13 TeV)-112.9 fb

(TeV)s7 8 9 10 11 12 13 14

(fb)

fid.

σ20

30

40

50

60

70

80

90

100Preliminary CMS

(13 TeV)-1 (8 TeV) + 12.9 fb-119.7 fb

γγ→H)Hbest-fit mData (

syst. uncertainty)=125.09 GeVHmSM (

- norm. LHC Higgs XSWG YR4MC@NLOA- acc.

• Measurement of fiducial cross section using different categorisation scheme.

• Consistency with SM observed.

Page 9: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

µ2− 0 2 4 6 8

-1.2+1.5 1.91

ttHµ

-0.8+0.9 1.61

VBFµ

-0.23+0.25 0.77

ggHµ

0.18−0.21+ = 0.95

combinedµ

ProfiledHm

σ 1±Combined

σ 1±Per category

SMµ=µ

Preliminary CMS

γγ→H

TeV) (13-1 12.9 fb

= 1VHµ

Production rate modifier

Louie Corpe, Imperial College 9

• Best fit signal strength split into bosonic and fermionic production modes:

• Also split the signal strength by individual production mode: consistent with SM.

ggH,ttHµ

0.5− 0 0.5 1 1.5 2 2.5 3

VBF,

VHµ

0

0.5

1

1.5

2

2.5

3

3.5

4Best Fit

SM

σ1

σ2

Preliminary CMSγγ→H

TeV) (13-112.9 fb

ProfiledHm

Page 10: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Vκ0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2

1−

0.5−

0

0.5

1

1.5

2

2.5

3 ) fκ, Vκq(

0

2

4

6

8

10

Best Fitσ1σ2

SM

Preliminary CMS TeV) (13-112.9 fb

γγ→H ProfiledHm

γκ0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2

gκ0

0.2

0.4

0.6

0.8

1

1.2

1.4

1.6

1.8

2 ) gκ, γκq(

0

2

4

6

8

10

Best Fitσ1σ2

SM

Preliminary CMS TeV) (13-112.9 fb

γγ→H ProfiledHm

Coupling strength modifiers

Louie Corpe, Imperial College 10

• 𝞳ɣ, 𝞳g, 𝞳V, 𝞳f measure strength of Higgs coupling to particles relative to SM. For Higgs couplings via loops, an effective coupling is defined.

• Results consistent with SM expectation.

Page 11: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Summary and Conclusions

Louie Corpe, Imperial College 11

• CMS has prepared its first results using the 2016 13 TeV dataset with 12.9 fb-1. Roughly equivalent to Run 1 dataset in terms of sensitivity.

• We report an observation of the Higgs boson with over 5σ significance in the diphoton decay channel.

• The measured signal strength is consistent with the SM expectation, with overall uncertainty of ~20%:

• Fiducial XS measurement performed - in line with SM expectation. • Consistency with SM when splitting signal strength into production modes. • Best-fit values of Higgs coupling strength modifiers for gluons, photons, vector

bosons and tops are found to be consistent with SM expectation. • Higgs physics: begin transitioning from discovery to precision

measurement era.

Page 12: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

BACKUP

Louie Corpe, Imperial College 12

BACKUP

Page 13: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

The CMS detector

HF Calorimeter

Hadron Calorimeter

Silicon Tracker

Preshower

Muon Detectors

EMCalorimeter

Louie Corpe, Imperial College 13

Solenoid Magnet 3.8T

Page 14: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Vertex ID

Louie Corpe, Imperial College 14

• Inputs to the vertex ID BDT.

• ptasym

• ptbal

• sumpt2

• pull

• correct vertex (dZ<1cm)

• incorrect vertex (dZ >1cm)

Page 15: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Photon ID

Louie Corpe, Imperial College 15

• Inp

• Distribution of BDTɣ ID score for signal and background. • Comparison of Distribution of BDTɣ ID score in data and MC using Z→ee events

where electrons are reconstructed as photons.

Page 16: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Energy Reconstruction

Louie Corpe, Imperial College 16

• data vs MC comparison for invariant mass of Z→ee electrons reconstructed as photons.

• Events split into |η| and R9 categories. (R9 is the ratio of the amount of energy in a 3x3 array of ECAL crystals around the seed divided by the total energy in the supercluster. High R9 (>0.94) photons are likely to be unconverted, while Low R9 photons are likely to have undergone ɣ→e+e-).

Page 17: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Diphoton MVA

Louie Corpe, Imperial College 17

• Distribution of BDTɣɣ score for signal and background. • Comparison of Distribution of BDTɣɣ score in data and MC using Z→ee events

where electrons are reconstructed as photons.

Page 18: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Diphoton Selection andEvent Classification

Louie Corpe, Imperial College 18

• Diphotons split into categories, exploiting different S/B ratios and mass resolution => maximum sensitivity:

• TTH categories: make cuts on photon quality and requirements on bTags, Jets and absence/presence of leptons .

• VBF categories: use an MVA to identify VBF-like events with dijets. A further MVA using the diphoton and dijet MVAs as inputs is used to classify VBF events by sensitivity into VBFTags 0 and 1.

• Untagged categories: mostly populated by ggH, bring the largest contribution to analysis’ sensitivity. Category boundaries defined by Diphoton MVA.

• Event tagging sequence is defined as follows:

ttHLeptonic ttHHadronic VBF0-1 Untagged0-3

Page 19: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Background Model Plots Unblinded

Louie Corpe, Imperial College 19

• Data and Signal + Background Fits shown, in the scenario where mH is profiled.

• Figures also show the Background-subtracted distributions.

• Uncertainty bands achieved by throwing toys from the post-Fit distributions and finding locations of relevant quantiles.

Page 20: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Background Model Plots Unblinded

Louie Corpe, Imperial College 20

• Data and Signal + Background Fits shown, in the scenario where mH is profiled.

• Figures also show the Background-subtracted distributions.

• Uncertainty bands achieved by throwing toys from the post-Fit distributions and finding locations of relevant quantiles.

Page 21: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Weighted S/S+B and P-Value

Louie Corpe, Imperial College 21

• Shown here is the total invariant mass distribution where we reweight using the factor S/(S+B) in a 1GeV window around the point.

Unweighted Weighted

Page 22: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Signal Model

Louie Corpe, Imperial College 22

Page 23: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Signal Model

Louie Corpe, Imperial College 23

(GeV)γγm105 110 115 120 125 130 135 140

Even

ts /

( 0.5

GeV

)

02468

1012141618202224

FWHM = 5.11 GeV

Untagged 3γγ→H

Simulation

modelParametric

= 2.44 GeVeffσ

13 TeVCMS Simulation Preliminary

(GeV)γγm105 110 115 120 125 130 135 140

Even

ts /

( 0.5

GeV

)

0

5

10

15

20

25

FWHM = 3.45 GeV

Untagged 2γγ→H

Simulation

modelParametric

= 1.70 GeVeffσ

13 TeVCMS Simulation Preliminary

(GeV)γγm105 110 115 120 125 130 135 140

Even

ts /

( 0.5

GeV

)

0

2

4

6

8

10

12

14

16

18

20

FWHM = 2.83 GeV

Untagged 1γγ→H

Simulation

modelParametric

= 1.35 GeVeffσ

13 TeVCMS Simulation Preliminary

(GeV)γγm105 110 115 120 125 130 135 140

Even

ts /

( 0.5

GeV

)

0

0.2

0.4

0.6

0.8

1

1.2

1.4

1.6

1.8

2

2.2

FWHM = 2.42 GeV

Untagged 0γγ→H

Simulation

modelParametric

= 1.18 GeVeffσ

13 TeVCMS Simulation Preliminary

Page 24: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Signal Model

Louie Corpe, Imperial College 24

(GeV)γγm105 110 115 120 125 130 135 140

Even

ts /

( 0.5

GeV

)

0

0.05

0.1

0.15

0.2

0.25

0.3

0.35

0.4

FWHM = 2.84 GeV

TTH Hadronic Tagγγ→H

Simulation

modelParametric

= 1.39 GeVeffσ

13 TeVCMS Simulation Preliminary

(GeV)γγm105 110 115 120 125 130 135 140

Even

ts /

( 0.5

GeV

)

0

0.02

0.04

0.06

0.08

0.1

0.12

0.14

0.16

FWHM = 3.17 GeV

TTH Leptonic Tagγγ→H

Simulation

modelParametric

= 1.61 GeVeffσ

13 TeVCMS Simulation Preliminary

(GeV)γγm105 110 115 120 125 130 135 140

Even

ts /

( 0.5

GeV

)

0

0.2

0.4

0.6

0.8

1

1.2

FWHM = 3.12 GeV

VBF Tag 0γγ→H

Simulation

modelParametric

= 1.60 GeVeffσ

13 TeVCMS Simulation Preliminary

(GeV)γγm105 110 115 120 125 130 135 140

Even

ts /

( 0.5

GeV

)

0

0.2

0.4

0.6

0.8

1

1.2

1.4

1.6

1.8

2

2.2

FWHM = 3.28 GeV

VBF Tag 1γγ→H

Simulation

modelParametric

= 1.71 GeVeffσ

13 TeVCMS Simulation Preliminary

Page 25: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Fiducial XS measurement

Louie Corpe, Imperial College 25

(fb)fidσ30 40 50 60 70 80 90 100 110

ln L

∆-2

0

1

2

3

4

5

6

fb 22− 18+ = 69 fidσ

HXSWG YR4+ aMC@NLO

=125.09 GeVHm

Preliminary CMS

H, profiling mγγ→H

(13 TeV)-112.9 fb

(TeV)s7 8 9 10 11 12 13 14

(fb)

fid.

σ

20

30

40

50

60

70

80

90

100Preliminary CMS

(13 TeV)-1 (8 TeV) + 12.9 fb-119.7 fb

γγ→H)Hbest-fit mData (

syst. uncertainty)=125.09 GeVHmSM (

- norm. LHC Higgs XSWG YR4MC@NLOA- acc.

Page 26: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

μggH,ttH vs μVBF,VH Run1 vs Run2

Louie Corpe, Imperial College 26

ggH,ttHµ

0.5− 0 0.5 1 1.5 2 2.5 3VB

F,VH

µ0

0.5

1

1.5

2

2.5

3Best Fit

SM

σ1

σ2

Preliminary CMSγγ→H

TeV) (13-112.9 fb

ProfiledHm

Run 1

Figures shows with same axis ranges

Run 2

Page 27: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

𝞳g vs 𝞳ɣRun1 vs Run2

Louie Corpe, Imperial College 27

γκ0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2gκ

0

0.2

0.4

0.6

0.8

1

1.2

1.4

1.6

1.8

2 ) gκ, γκq(

0

2

4

6

8

10

Best Fitσ1σ2

SM

Preliminary CMS TeV) (13-112.9 fb

γγ→H ProfiledHm

Run 1 Run 2

Page 28: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

𝞳g vs 𝞳ɣRun1 vs Run2

Louie Corpe, Imperial College 28

Run 1 Run 2

Vκ0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2

1−

0.5−

0

0.5

1

1.5

2

2.5

3 ) fκ, Vκq(

0

2

4

6

8

10

Best Fitσ1σ2

SM

Preliminary CMS TeV) (13-112.9 fb

γγ→H ProfiledHm

Page 29: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Analysis Flowchart

Louie Corpe, Imperial College 29

Page 30: Observation of H→ɣɣ at CMS using 2016 data at s=13 TeV...Observation of H→ɣɣ at CMS using 2016 data at √s=13 TeV Louie Corpe (Imperial College) on behalf of the CMS Collaboration

Mass Measurement

Louie Corpe, Imperial College 30

• Observed best fit is at mH=126.0 GeV.• Obtained from prompt-reconstructed data. • Statistical uncertainty ~0.3 GeV. • Systematic uncertainty ~0.2-0.4 GeV. • Details of the systematic uncertainties on

the mass require further refinement and are still under study.

Even

ts /

GeV

0

1000

2000

3000

4000

5000

6000

7000

8000

9000

DataS+B fitB component

σ1 ±σ2 ±

All categories=0.95µ=126.0 GeV, Hm --

Preliminary CMS TeV) (13-1 12.9 fbγγ→H

(GeV)γγm100 110 120 130 140 150 160 170 180

100−

0

100

200 B component subtracted