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Calibration of CMS detector using Particle Flow Objects Sunanda Banerjee Gobinda Majumder Swagata Mukherjee India CMS Meeting Saha Institute of Nuclear Physics, Kolkata 18 – 21 December , 2012

Calibration of CMS detector using Particle Flow Objectsindiacms/indiacms-meetings/december-2012/swagata... · Calibration of CMS detector using Particle Flow Objects Sunanda Banerjee

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Page 1: Calibration of CMS detector using Particle Flow Objectsindiacms/indiacms-meetings/december-2012/swagata... · Calibration of CMS detector using Particle Flow Objects Sunanda Banerjee

Calibration of CMS detector usingParticle Flow Objects

Sunanda Banerjee Gobinda Majumder

Swagata Mukherjee

India CMS MeetingSaha Institute of Nuclear Physics, Kolkata

18 – 21 December , 2012

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OutlineOutline

● Reason to introduce PF calibration● Scenario without HO● Scenario with HO● Future Plans

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What is Particle Flow and Why is it important ?

Aims to reconstruct all stable particles in an event and returns a single list of reconstructed particles → Photon, Charged Hadron, Neutral Hadron, Muon, Electron.

Particle Flow reconstruction provides a global pp-collision event description by using information from different sub-detectors and combining it in the best possible way

Higher level physics objects can be built from the particle list

Jets , Missing transverse Energy etc.

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Why is Particle Flow Calibration needed?Why is Particle Flow Calibration needed?✔ HCAL and ECAL are already calibrated. PF calibration is done

on top of it.

✔ Energy reconstructed in PF algorithm, by combining ECAL and HCAL RecHit energies, is far from the true energies of the hadrons.

✔ This is especially true for low energy hadrons → energy is underestimated due to noise and threshold conditions.

✔ Estimating scale factors separately for ECAL and HCAL energies →

• Better estimate of the reconstructed energy

• Improvement in the energy resolution

• A smooth transition from low energy regime to high energy regime

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Samples UsedSamples Used

✔ Hadron samples are used for this calibration work

➢ Events are generated using CMSSW version 6_0_0_pre3 with particle gun event generator

➢ Separate samples are created with K+, K-, KL

0 , neutrons,

protons, anti-neutrons, anti-protons, π+ and π- ➢ Flat energy spectra of particles between 10 GeV and 1 TeV

are generated in the range |η| < 1.5 using a flat η distribution ➢ More or less 600k events are generated for each particle type

Thanks to Salavat

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Scenario 1 : Without HOScenario 1 : Without HOFor a hadron we expect energy deposit in the HCAL along with MIP like or higher energy (early showers) in the ECAL.

● ETrue

is fitted by (a+b.EECal

+c.EHCal

) =(ECorr

, say)

● 'a' is independent of energy, supposed to correct for ECAL and HCAL thresholds. 'b' and 'c' depends on E

True .

● Coefficients 'b' and 'c' are calculated by minimizing

● σi for barrel :

● → Two equations involving 'b' and 'c'

‘abc ’ Fit

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Inverting the resulting linear equations ,

Coeff 'a' cannot be obtained this way : To be put by hand

● Take 'a=0' for simplicity (Not a good choice)● Non zero 'a' → ◮ a = 3.5GeV (for E

ECal ≠ 0, E

HCal ≠ 0 )

◮ a = 3.0GeV (for EECal

= 0 )

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Why include HO ?Why include HO ?

➢ Around April 2012 , a study of MET measurements prompted that energy measured in HO rings 0 and 1 will be used for physics analysis.

➢ We extended the original code used to get the scales for ECAL and HCAL to include those for HO.

➢ Ntuples are created containing the information of energy in EB, HB, HO (separately for rings 0,1,2), η and the true energy of the particle.

➢ Modified macro is used on this ntuple to produce the plots within the ROOT version in CMSSW 5_2_0_pre6.

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Onto the plots ...Onto the plots ...

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Energy Calibration Coefficients : Without HOEnergy Calibration Coefficients : Without HO

Case 1 : EECal

> 0 , EHCal

> 0

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Case 2 : EECal

> 0 , EHCal

= 0

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Case 3 : EECal

= 0 , EHCal

> 0

Now, Response can be calculated as :

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Response : Scatter Plots (without HO)Response : Scatter Plots (without HO)*

*

* An eta correction has been used. Details are in Back Up

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Response : Profile Histogram (without HO)Response : Profile Histogram (without HO)

* An eta correction has been used. Details are in Back Up

*

*

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What is the effect of the What is the effect of the ηη correction on the response ? correction on the response ?

Magenta : No η correctionBlue : η Corrected

η Correction doesn't really help much

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Energy Resolution Plots (without HO)Energy Resolution Plots (without HO)

* An eta correction has been used. Details are in Back Up

*

*

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Scenario 2 : With HOScenario 2 : With HO

● ETrue

is fitted with (a + b.EECal

+ c.EHCal

+ d.EHO

)

● Coefficients 'b' , 'c' and 'd' are calculated by minimizing

● Where σi =

● → Three equations involving

'b' , 'c' and 'd'

‘abcd’ Fit

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Inverting the resulting linear equations ,

Value of 'a' is taken same as before

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Plots after including Ring 0 only

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Energy Calibration Coefficients : Energy Calibration Coefficients : With HO Ring 0With HO Ring 0

Case 1 : EECal

> 0 , EHCal

> 0 , EHO

> 0

Large fluctuation in HO coefficient while true energy is less than 100 GeV

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Case 2 : EECal

> 0 , EHCal

> 0 , EHO

= 0

With HO Ring 0With HO Ring 0

Coefficients are almost constant beyond 100 GeV

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Case 4 : EECal

= 0 , EHCal

> 0 , EHO

> 0

With HO Ring 0With HO Ring 0

Coefficient is almost constant throughout the whole energy range

Some fluctuations in low energy (< 100 GeV)

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Response : Profile Histogram (with HO Ring 0)Response : Profile Histogram (with HO Ring 0)

* An eta correction has been used. Details are in Back Up

*

*

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Energy Resolution Plots (with HO Ring 0)Energy Resolution Plots (with HO Ring 0)

* An eta correction has been used. Details are in Back Up

*

*

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But ...But ...

Is there any improvement in Energy Resolution after including Ring 0 ?

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Blue : Without HOMagenta : With Ring 0

Here all the particles in the η range-1.479 to +1.479 has been taken

What if I take only those particles which lies What if I take only those particles which lies in the in the ηη range -0.34 to +0.34 ? range -0.34 to +0.34 ?

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Plots after including Ring 0+1*

* Plots of Energy Calibration Coefficients, Response and Resolution are in Back Up.

Let's take a look only at the Resolution Comparison plotResolution Comparison plot

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Blue : Without HOMagenta : With Ring 0Green : With Ring 0+1

All the particles in the η range -1.479 to +1.479 has been taken

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Resolution Comparison Plot after including Resolution Comparison Plot after including Ring 0+1+2 Ring 0+1+2 *

Blue : Without HOMagenta : With Ring 0Green : With Ring 0+1Black : With Ring 0+1+2

Blue : Without HOMagenta : With Ring 0Green : With Ring 0+1Black : With Ring 0+1+2

* Other plots are in Back Up

All the particlesin the η range-1.479 to +1.479has been taken

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Summary & OutlookSummary & Outlook

● Energy scale factors are computed for the PF algorithm with energies from ECAL, HB and HO

● Inclusion of energy measurements from HO improves energy resolution of single particles

● Ring 2 has very little effect on the improvements

● Verify these factors in jets

● Calculate the scale factors using dijet events and gamma+jet events.

● We plan to use the scale factors in real data

Thank You

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Back Up SlidesBack Up Slides

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Plots after including Ring 0+1

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Energy Calibration CoefficientsEnergy Calibration Coefficients

Case 1 : EECal

> 0 , EHCal

> 0 , EHO

> 0

With HO Ring 0+1With HO Ring 0+1

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Case 2 : EECal

> 0 , EHCal

> 0 , EHO

= 0

Case 3 : EECal

> 0 , EHCal

= 0 , EHO

= 0

With HO Ring 0+1With HO Ring 0+1

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Case 4 : EECal

= 0 , EHCal

> 0 , EHO

> 0

Case 5 : EECal

= 0 , EHCal

> 0 , EHO

= 0

With HO Ring 0+1With HO Ring 0+1

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Response : Scatter Plots (with HO Ring 0+1)Response : Scatter Plots (with HO Ring 0+1)

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Response : Profile Histogram (with HO Ring 0+1)Response : Profile Histogram (with HO Ring 0+1)

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Energy Resolution Plots (with HO Ring 0+1)Energy Resolution Plots (with HO Ring 0+1)

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Plots after including Ring 0+1+2

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Energy Calibration CoefficientsEnergy Calibration Coefficients

Case 1 : EECal

> 0 , EHCal

> 0 , EHO

> 0

With HO Ring 0+1+2With HO Ring 0+1+2

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Case 2 : EECal

> 0 , EHCal

> 0 , EHO

= 0

Case 3 : EECal

> 0 , EHCal

= 0 , EHO

= 0

With HO Ring 0+1+2With HO Ring 0+1+2

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Case 4 : EECal

= 0 , EHCal

> 0 , EHO

> 0

Case 5 : EECal

= 0 , EHCal

> 0 , EHO

= 0

With HO Ring 0+1+2With HO Ring 0+1+2

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Response : Scatter Plots (with HO Ring 0+1+2)Response : Scatter Plots (with HO Ring 0+1+2)

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Response : Profile Histogram (with HO Ring 0+1+2)Response : Profile Histogram (with HO Ring 0+1+2)

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Energy Resolution Plots (with HO Ring 0+1+2)Energy Resolution Plots (with HO Ring 0+1+2)

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η correction of reconstructed energyη correction of reconstructed energy

The following angular correction has been used :

We have also tried the following types of angular corrections, which gave more or less similar results.

Coefficients are calculated by minimizing

→ Type_0 (say)

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Plots for Plots for ηη coefficients coefficients

→ Without HO

With HO Ring 0 ←

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Weight Factors of Different Hadrons

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Snippets from our Snippets from our ππ+ + ntuplentuple

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2D plots of “Energy in ECAL” vs “Energy in HO” when true energy is less than 100 GeV(With π+ ntuple )