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| The combined upper limit as a function of the Higgs boson mass between 100 and 200 GeV/c2
Solid black: observed limit/SM; Dashed black: median expected limit/SM. Colored bands: +-1, 2 sigma distributions around median expected limit. |
The combined upper limit as a function of the Higgs boson mass between 100 and 200 GeV/c2.
Solid lines indicate the observed upper limit for each channel and
combined result (dark red). Dashed lines indicate the median expected upper limit for each channel and the combined result (dark red). |
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| The summary table of observed and expected limits between 100 and 200 GeV/c2 for the combination of all CDF Higgs
search analyses. Limits are presented at the 95% CL. |
Limits for the H→bb channels. They are: lvbb, METbb, llbb, jjbb, and ttH. Limits are presented at the 95% CL. |
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| Events in all search channels, sorted by the s/b in the bins in which they are found. Signal and background totals are shown, stacked.
This plot is shown for mH=100 GeV/c2 |
Cumulative distributions of background, data and signal+background. The s/b distribution is integrated from the high s/b side downwards.
This plot is shown for mH=100 GeV/c2 |
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| Events in all search channels, sorted by the s/b in the bins in which they are found. Signal and background totals are shown, stacked.
This plot is shown for mH=115 GeV/c2 |
Cumulative distributions of background, data and signal+background. The s/b distribution is integrated from the high s/b side downwards.
This plot is shown for mH=115 GeV/c2 |
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| Events in all search channels, sorted by the s/b in the bins in which they are found. Signal and background totals are shown, stacked.
This plot is shown for mH=150 GeV/c2 |
Cumulative distributions of background, data and signal+background. The s/b distribution is integrated from the high s/b side downwards.
This plot is shown for mH=150 GeV/c2 |
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| Events in all search channels, sorted by the s/b in the bins in which they are found. Signal and background totals are shown, stacked.
This plot is shown for mH=165 GeV/c2 |
Cumulative distributions of background, data and signal+background. The s/b distribution is integrated from the high s/b side downwards.
This plot is shown for mH=165 GeV/c2 |
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Background-subtracted data distributions for events in all channels, sorted and collected by s/b. The background is fit to the data.
The error bars on the background-subtracted data points are the square roots of the best-fit background rates in those bins.
The blue histograms show the remaining uncertainty on the background rates after the fit. The shaded histogram shows the expected signal
yield for a 115 GeV/c2 Higgs boson. |
Background-subtracted data distributions for events in all channels, sorted and collected by s/b. The background is fit to the data.
The error bars on the background-subtracted data points are the square roots of the best-fit background rates in those bins.
The blue histograms show the remaining uncertainty on the background rates after the fit. The shaded histogram shows the expected signal
yield for a 165 GeV/c2 Higgs boson. |
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| Projected median expected upper limits on the SM Higgs boson cross section, scaling CDF performance to twice the luminosity.
The solid lines are 1/sqrt(L) projections, as functions of integrated luminosity per experiment.
The top of the orange band corresponds to the Summer 2007 performance expected limit divided by 1.5, and the bottom
of the orange band corresponds to the Summer 2007 performance expected limit divided by 2.25.
This plot is shown for mH=115 GeV/c2 |
Projected median expected upper limits on the SM Higgs boson cross section, scaling CDF performance to twice the luminosity.
The solid lines are 1/sqrt(L) projections, as functions of integrated luminosity per experiment.
The top of the orange band corresponds to the Summer 2007 performance expected limit divided by 1.5, and the bottom
of the orange band corresponds to the Summer 2007 performance expected limit divided by 2.25.
This plot is shown for mH=160 GeV/c2 |
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Probability of seeing a 2σ excess as a function of mH for analyzed integrated luminosities of 5 fb-1 and
10 fb-1 per experiment, assuming CDF and D0 perform the same. Two scenarios are shown, in which channels have the same performance
as for the Winter 2009 combination (solid lines), and for the case with another factor of 1.5 in the sensitivity (dashed lines).
The current observations are not taken into account, only expected sensitivities are shown. Sensitivities are expected to scale with sqrt(L).
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Probability of seeing a 3σ excess as a function of mH for analyzed integrated luminosities of 5 fb-1 and
10 fb-1 per experiment, assuming CDF and D0 perform the same. Two scenarios are shown, in which channels have the same performance
as for the Winter 2009 combination (solid lines), and for the case with another factor of 1.5 in the sensitivity (dashed lines).
The current observations are not taken into account, only expected sensitivities are shown. Sensitivities are expected to scale with sqrt(L).
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