Etmiss distribution of random events
Missing transverse energy distribution for random triggers (noise) Shown in red is the sum over all cell above noise and in blue the result of summing over all topological clusters (noise suppression using 4/2/0). Data are shown as markers. Overlayed is a Monte Carlo simulation where the noise is modeled as simple single Gaussian distribution Used are randomly triggered events from run 150541; taken the 23th of November 2009. no calibration is applied (em-scale). See this plot under "Public plots from collision data". | ||
Cell- and topocluster-based EXmiss and EYmiss distributions, showing a good control of the energy reconstruction in the 187000 cells of the Calorimeter. The topocluster-based distributions show better noise suppression than when using the cell-based method. eps version (x) eps version (y) | ||
ET also has the expected Gaussian shape, with a similar improvement of the topocluster-based evaluation compared to the cell-based one. A small shift (compared to the RMS of the distribution) of the cell-based ET is visible, and is being studied further. eps version | ||
Inclusive distributions of ETmiss for both methods are shown, showing again the better noise suppression of the topocluster method. Tails in the distribution (beyond 8 GeV for topocluster-based, and 16 GeV for cell-based, variables), contributing less than 0.1% of events, have been understood to come from coherent noise in a specific region of LAr presampler. eps version | ||
The expected ETmiss distribution obtained by a randomisation of the cell energy with a Gaussian noise of width noise, superimposed on the measured cell-based ETmiss distribution. A good description of the observed distribution is seen. Similar studies for the topocluster-based missing ET require an accurate description of the noise up to and beyond 4 : this work is in progress. eps version |
Deviation of the mean of the EXmiss distribution () from its average value <> (0.103 ± 0.005 GeV). Good stability is seen over the month and a half period. eps version |
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Deviation of the width of the EXmiss distribution () from its average value <> (1.000 ± 0.005 GeV). Good stability is seen over the month and a half period, with no significant change with time. eps version |
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Deviation of the mean of the EYmiss distribution () from its average value <> (0.023 ± 0.004 GeV). Good stability is seen over the month and a half period, with no significant change with time. eps version |
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Deviation of the width of the EYmiss distribution () from its average value <> (0.932 ± 0.003 GeV). Good stability is seen over the month and a half period, with no significant change with time. eps version |
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Deviation of the mean of the ET distribution (); from its average value <> (0.780 ± 0.014 GeV). Good stability is seen over the month and a half period: variations are observed, but are small compared to the width of the distribution (~1.4 GeV). eps version |
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Deviation of the width of the ET distribution () from its average value <> (1.372 ± 0.006 GeV). Good stability is seen over the month and a half period, with no significant change with time. eps version |