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Fits to W final states

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A global likelihood fit can take this into account ... (mainly suppress the kink) Compare with shapes obtained from full simulation ... – PowerPoint PPT presentation

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Title: Fits to W final states


1
Fits to W final states
L. R. Flores-Castillo, B. Mellado, S. Padhi, Sau
Lan Wu University of Wisconsin-Madison Exotics
Meeting
Feb 21st, 2007
2
Motivation
  • Computing the significance using a sliding cut
    strategy can overestimate it (look-elsewhere
    effect).
  • A global likelihood fit can take this into
    account see, e.g., talks by Y. Gao in the Higgs
    meeting.
  • Counting the number of events on a MT window does
    not take into account shape information
  • In the case of W, the MT distribution may also
    depend on tails on the missing ET reconstruction.
    A global fit can use them as sidebands, instead
    of relying on MC.
  • At 100 pb-1
  • How significant is this?

3
Samples, selection
  • Fortran Atlfast for
  • W?l nu
  • 5 samples to cover a large kinematic range
  • W ?l nu
  • 1,2,3,4,5,6 TeV
  • Selection
  • Exactly one lepton in ?
  • Pt(lepton)50GeV
  • 90 lepton rec. eff. applied
  • MET 50GeV
  • No cut on MT

4
Background model
  • The function exp( p0 - p1(mT)p2 ) does a good
    job over the full range (8 orders of magnitude).
  • Some variations due to the joining of background
    samples

5
Signal Model
Derivative discontinuity
p0 p1(mT)p2
Double exponential tail
  • The same model works fine for all m(W) values
  • The sharp peak needs to be softened
  • Related to resolution
  • Brings some headaches when fitting

6
Signal template. Fits
No need to model the turn on (completely
swallowed by the background)
7
Signal template. Fits
  • The highest-mass W samples (5, 6 TeV) have a
    negative slope before the drop this is still
    well described by the model, but brings a problem
    later.

8
Signal template. Parameterization
  • Once we have a model for each W mass value, we
    can find a model for each parameter as a function
    of the true mass of the W
  • Result a one-parameter family of functions that
    describes the shape of the transverse mass for
    each W mass

9
  • The previously mentioned negative slope of the
    highest two W masses produces a sign change in
    one parameter
  • The change is smooth (because the weight of the
    corresponding term vanishes), but it is not clear
    how to interpolate
  • For now, will use only up to 4TeV

10
Toy MC
  • Single experiment with a 2TeV W signal over the
    W background, corresponding to 100pb-1
  • Unbinned maximum likelihood fits
  • Left BG model, floating all three background
    parameters
  • Right SB model, floating also the mass of the
    W, and the fraction (dashed
    background component solid line total)

11
Delta Log Likelihood
  • Estimate the probability of a background-only
    experiment to produce a typical signal (one with
    a ?NLL in the median of the distribution).
  • Behaves as expected, but too low statistics
    (very slow fits in the bg-only case)
  • Still, seems unlikely that it would reach 5
    sigma
  • (fitter or look-elsewhere?)

12
Outlook and plans
  • Preliminary parameterization of the signal and
    background shapes for the W analysis.
  • First look at the delta log likelihood.
  • Machinery working, but too low statistics as of
    now
  • To do
  • Increase the statistics, refine the model
    (mainly suppress the kink)
  • Compare with shapes obtained from full simulation
  • Study the dependence of the parameters on
    instrumental uncertainties
  • Toy MC studies of Z significance

13
  • BACKUP

14
The remaining parameters
  • Only modeled up to 4TeV
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