Pile-up Noise (2022) | |
Energy distribution in the Tile Calorimeter Layer A cells with 1.1<![]() ![]() ![]() ![]() ![]() ![]() Contact: Aliaksei Hrynevich aliaksei.hrynevich@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2022-059 Date: November, 2022 |
[PDF] [EPS] |
The Tile Calorimeter noise as a function of an average number of interactions per bunch crossing, ![]() ![]() ![]() ![]() ![]() Contact: Aliaksei Hrynevich aliaksei.hrynevich@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2022-059 Date: November, 2022 |
[PDF] [EPS] |
The Tile Calorimeter noise as a function of average number of interactions per bunch crossing, ![]() ![]() ![]() ![]() ![]() ![]() Contact: Aliaksei Hrynevich aliaksei.hrynevich@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2022-059 Date: November, 2022 |
[PDF] [EPS] |
Pile-up Noise MC Only (2022) | |
Energy distribution in the Tile Calorimeter Layer A cell with 1.1<![]() ![]() ![]() ![]() ![]() ![]() Contact: Aliaksei Hrynevich aliaksei.hrynevich@cernNOSPAMPLEASE.ch Date: August, 2022 |
[PDF] [EPS] |
The noise distributions in different Tile Calorimeter cells for a mixed sample of events from EPOS (jet ![]() ![]() ![]() Contact: Aliaksei Hrynevich aliaksei.hrynevich@cernNOSPAMPLEASE.ch Date: August, 2022 |
[PDF] [EPS] |
The Tile Calorimeter noise as a function of average number of interactions per bunch crossing, ![]() ![]() ![]() ![]() Contact: Aliaksei Hrynevich aliaksei.hrynevich@cernNOSPAMPLEASE.ch Date: August, 2022 |
[PDF] [EPS] |
The Tile Calorimeter noise as a function of average number of interactions per bunch crossing, ![]() ![]() ![]() ![]() ![]() Contact: Aliaksei Hrynevich aliaksei.hrynevich@cernNOSPAMPLEASE.ch Date: August, 2022 |
[PDF] [EPS] |
Pile-up Noise (2016) | |
Energy distribution for data collected in 2016 in the zero-bias stream with 25 ns bunch spacing at a centre-of-mass energy of 13 TeV (runs 310247, 310249, 310341, 310370) and Pythia 8 Monte Carlo simulation with A3 Minimum Bias tune for the layer A cell with ![]() ![]() ![]() ![]() Contact: Aliaksei Hrynevich aliaksei.hrynevich@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2017-007 Date: February, 2017 |
[PDF] [EPS] |
The noise distributions in different Tile Calorimeter cells are represented as a function of ![]() ![]() Contact: Aliaksei Hrynevich aliaksei.hrynevich@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2017-007 Date: February, 2017 |
[PDF] [EPS] |
The Tile Calorimeter noise dependence with the average number of interactions per bunch crossing, ![]() ![]() ![]() Contact: Aliaksei Hrynevich aliaksei.hrynevich@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2017-007 Date: February, 2017 |
[PDF] [EPS] |
The Tile Calorimeter noise dependence with the average number of interactions per bunch crossing, ![]() ![]() ![]() Contact: Aliaksei Hrynevich aliaksei.hrynevich@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2017-007 Date: February, 2017 |
[PDF] [EPS] |
Pile-up Noise (2012) | |
The noise distribution in different TileCal cells is represented as a function of |![]() ![]() Contact: Juan Pedro Araque juan.pedro.araque.espinosa@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2011-022 | ![]() [pdf] [eps] |
The noise distribution in different TileCal cells is represented as a function of |![]() ![]() Contact: Juan Pedro Araque juan.pedro.araque.espinosa@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2011-022 | ![]() [pdf] [eps] |
The noise in D5 and D6 cells of the Tile calorimeter, located at the outermost layer with 0.9 < |η| < 1.3, is plotted against the average number of interactions per event. The dashed line shows the electronic noise contribution estimated from special pedestal runs.
The noise was estimated as the RMS of the energy deposited in the cell in zero bias data in collisions with a center-of-mass energy of 8 TeV and bunch spacing of 25 ns. The data beam parameters and structure were simulated in the Monte-Carlo events. The data points refer to the D5 and D6 cells of the Extended Barrel modules EBA39 and EBC39 because they were powered by the new generation low noise Low Voltage Power Supplies, which are going to be used in the whole calorimeter in Run 2.
Contact: Vladimir Drugakov v.drugakov@cernNOSPAMPLEASE.ch
Reference: ATL-COM-TILECAL-2013-035![]() Date: 16 Aug 2013 |
![]() |
Energy distribution for data collected in 2012 in the zero-bias stream with 50 ns bunch spacing at a centre-of-mass energy of 8 TeV and
Monte Carlo simulation for the layer A cell with ![]() ![]() ![]() ![]() ![]() Contact: Aliaksei Hrynevich aliaksei.hrynevich@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2015-012 Date: March 10, 2015 |
![]() [PDF] |
Noise comparison as a function of the mean number of interactions per crossing between data
collected in 2012 in the zero-bias stream with 50 ns bunch spacing at a centre-of-mass energy of 8
TeV and Monte Carlo simulation for the cells in the layer A of the Tile Calorimeter. For data the runs
201555, 205112, 207397, 208781, 210302, 211973 have been used. The noise is derived as the
standard deviation of the energy distribution. In the region where data and Monte Carlo simulation
overlap a good agreement can be seen, with the highest different being of the order of ![]() Contact: Juan Pedro Araque jp.araque@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2015-012 Date: March 10, 2015 |
![]() [PDF] |
The energy distribution for the cell in the layer A with ![]() Contact: Juan Pedro Araque jp.araque@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2015-012 Date: March 10, 2015 |
![]() [PDF] |
Comparison between the RMS of the energy distribution scaled by a factor of 2 (dark yellow circle) and 4 (blue circle) and the
width of the regions that contains the 95.45% (filled dark yellow circle) and 99.99% (filled blue circle) of the events in the energy
distributions (solid circles) for the cell in the layer A with ![]() Contact: Juan Pedro Araque jp.araque@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2015-012 Date: March 10, 2015 |
![]() [PDF] |
Comparison between the RMS of the energy distribution scaled by a factor of 2 (dark yellow circle) and 4 (blue
circle) and the width of the regions that contains the 95.45% (filled dark yellow circle) and 99.99% (filled blue circle)
of the events in the energy distributions (solid circles) for the cell in the layer D with ![]() Contact: Juan Pedro Araque jp.araque@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2015-012 Date: March 10, 2015 |
![]() [PDF] |
Comparison between the RMS of the energy distribution scaled by a factor of 2 (hollow markers) and the width of the
regions that contains the 95.45% of the events in the energy distributions (filled markers) for the cell in the layer A
with ![]() ![]() ![]() ![]() Contact: Juan Pedro Araque jp.araque@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2015-012 Date: March 10, 2015 |
![]() [PDF] |
Pile-up Noise (2011) | |
The noise distribution in different TileCal cells is represented as a function of |![]() ![]() Contact: Susana Santos Susana.Patricia.Santos@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2011-022 | ![]() [pdf] [eps] |
The noise distribution in different TileCal cells is represented as a function of |![]() ![]() Contact: Susana Santos Susana.Patricia.Santos@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2011-022 | ![]() [pdf] [eps] |
The TileCal noise dependence with the actual number of interactions, ![]() Contact: Serguei Yanush Serguei.Yanush@cernNOSPAMPLEASE.ch Reference: ATL-COM-TILECAL-2011-022 | ![]() [pdf] [eps] |
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25ns_216416abs.eps | r1 | manage | 58.1 K | 2016-08-23 - 17:02 | PawelKlimek | |
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25ns_216416abs.pdf | r1 | manage | 23.4 K | 2016-08-23 - 17:02 | PawelKlimek | |
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25ns_216416abs.png | r1 | manage | 31.4 K | 2016-08-23 - 17:02 | PawelKlimek | |
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50ns_208781abs.eps | r1 | manage | 58.1 K | 2016-08-23 - 17:04 | PawelKlimek | |
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50ns_208781abs.pdf | r1 | manage | 23.3 K | 2016-08-23 - 17:04 | PawelKlimek | |
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50ns_208781abs.png | r1 | manage | 34.8 K | 2016-08-23 - 17:04 | PawelKlimek | |
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EnergyDep.eps | r1 | manage | 29.0 K | 2017-03-20 - 22:51 | AliakseiHrynevich | |
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EnergyDep.pdf | r2 r1 | manage | 23.1 K | 2017-03-20 - 22:51 | AliakseiHrynevich | |
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EnergyDep_2022.eps | r1 | manage | 14.5 K | 2022-08-18 - 22:45 | AliakseiHrynevich | |
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EnergyDep_2022.pdf | r1 | manage | 15.2 K | 2022-08-18 - 22:45 | AliakseiHrynevich | |
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EnergyDep_2022_wdata.eps | r1 | manage | 27.8 K | 2022-11-28 - 15:56 | AliakseiHrynevich | Update to the simulation only plots, but now with the data. |
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EnergyDep_2022_wdata.pdf | r1 | manage | 24.3 K | 2022-11-28 - 15:56 | AliakseiHrynevich | Update to the simulation only plots, but now with the data. |
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NoiseEta_F2.eps | r1 | manage | 42.0 K | 2016-08-23 - 17:02 | PawelKlimek | |
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NoiseEta_F2.pdf | r1 | manage | 20.7 K | 2016-08-23 - 17:02 | PawelKlimek | |
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NoiseEta_F2.png | r1 | manage | 409.6 K | 2016-08-23 - 17:02 | PawelKlimek | |
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NoiseEta_M2.eps | r1 | manage | 42.1 K | 2016-08-23 - 17:02 | PawelKlimek | |
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NoiseEta_M2.pdf | r1 | manage | 20.7 K | 2016-08-23 - 17:02 | PawelKlimek | |
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NoiseEta_M2.png | r1 | manage | 411.0 K | 2016-08-23 - 17:02 | PawelKlimek | |
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NoiseMu.eps | r1 | manage | 19.5 K | 2016-08-23 - 17:02 | PawelKlimek | |
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NoiseMu.pdf | r1 | manage | 15.7 K | 2016-08-23 - 17:02 | PawelKlimek | |
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NoiseMu.png | r1 | manage | 498.1 K | 2016-08-23 - 17:02 | PawelKlimek | |
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NoiseVsEta.eps | r1 | manage | 18.3 K | 2022-08-18 - 22:45 | AliakseiHrynevich | |
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NoiseVsEta.pdf | r1 | manage | 18.5 K | 2022-08-18 - 22:45 | AliakseiHrynevich | |
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NoiseVsMu_EBA_2022.eps | r1 | manage | 39.9 K | 2022-08-18 - 22:45 | AliakseiHrynevich | |
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NoiseVsMu_EBA_2022.pdf | r1 | manage | 26.2 K | 2022-08-18 - 22:45 | AliakseiHrynevich | |
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NoiseVsMu_EBA_2022_wdata.eps | r1 | manage | 55.1 K | 2022-11-28 - 15:56 | AliakseiHrynevich | Update to the simulation only plots, but now with the data. |
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NoiseVsMu_EBA_2022_wdata.pdf | r1 | manage | 32.3 K | 2022-11-28 - 15:56 | AliakseiHrynevich | Update to the simulation only plots, but now with the data. |
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NoiseVsMu_LBA_2022.eps | r1 | manage | 33.4 K | 2022-08-18 - 22:45 | AliakseiHrynevich | |
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NoiseVsMu_LBA_2022.pdf | r1 | manage | 23.5 K | 2022-08-18 - 22:45 | AliakseiHrynevich | |
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NoiseVsMu_LBA_2022_wdata.eps | r1 | manage | 45.6 K | 2022-11-28 - 15:56 | AliakseiHrynevich | Update to the simulation only plots, but now with the data. |
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NoiseVsMu_LBA_2022_wdata.pdf | r1 | manage | 28.4 K | 2022-11-28 - 15:56 | AliakseiHrynevich | Update to the simulation only plots, but now with the data. |
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PileupEtaDep.eps | r1 | manage | 22.1 K | 2017-03-20 - 22:51 | AliakseiHrynevich | |
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PileupEtaDep.pdf | r2 r1 | manage | 24.2 K | 2017-03-20 - 22:51 | AliakseiHrynevich | |
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PileupMuDep_EBA.eps | r1 | manage | 59.7 K | 2017-03-20 - 22:51 | AliakseiHrynevich | |
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PileupMuDep_EBA.pdf | r2 r1 | manage | 53.0 K | 2017-03-20 - 22:51 | AliakseiHrynevich | |
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PileupMuDep_LBA.eps | r1 | manage | 52.1 K | 2017-03-20 - 22:51 | AliakseiHrynevich | |
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PileupMuDep_LBA.pdf | r2 r1 | manage | 46.4 K | 2017-03-20 - 22:51 | AliakseiHrynevich | |
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energy2030.png | r1 | manage | 46.8 K | 2016-08-23 - 17:02 | PawelKlimek | |
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energymu.png | r1 | manage | 31.1 K | 2016-08-23 - 17:02 | PawelKlimek | |
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noise_D5D6_8TeV_25ns_newLVPS_v2.eps | r1 | manage | 8.6 K | 2016-08-23 - 17:02 | PawelKlimek | |
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noise_D5D6_8TeV_25ns_newLVPS_v2.png | r1 | manage | 26.6 K | 2016-08-23 - 17:02 | PawelKlimek | |
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quantA.png | r1 | manage | 43.7 K | 2016-08-23 - 17:02 | PawelKlimek | |
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quantAD.png | r1 | manage | 42.8 K | 2016-08-23 - 17:02 | PawelKlimek | |
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quantD.png | r1 | manage | 45.4 K | 2016-08-23 - 17:02 | PawelKlimek | |
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quantshapes.png | r1 | manage | 42.2 K | 2016-08-23 - 17:02 | PawelKlimek |