NonCollisionBackgroundPublicResults < AtlasPublic

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---+!! <nop>%TOPIC%
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---+Introduction
This page shows public plots from the Non-Collision Background group

---++ Results from Run 2

---+++ Beam Induced Background Identification in ATLAS detector by Tracking System

These Plots illustrate the information on BIB characteristics at different locations in the SCT barrel and endcaps. Unpaired isolated bunches are studied using Beam Condition Monitor (BCM) unpaired triggers within the ATLAS Run-II dataset. Events are selected by the BCM trigger active on unpaired isolated bunches and to remove the electronic noise, they are required to have at least 80 hits in the Pixel detector. The Beam 1(2) which is rotating clockwise (anti-clockwise), crossing ATLAS from side A to C (C to A) are identified using BCM trigger. 
<table class="twikiTable" width="100%" bgcolor=#f5f5fa  border=1 cellpadding=10 cellspacing=10>

<tr>
<td bgcolor=#eeeeee>
<b> SCT barrel hit occupancy as a function of the detector layer for beam 1 and beam 2  for events with exactly one primary vertex (&#119899;_&#119875;&#119881;=1) and events with no PV or more than one (&#119899;_&#119875;&#119881;&#8800;1), in 2018 data. The hit occupancy is defined as the number of hits in a certain layer divided by the total number of strips in that layer. The histograms with &#119899;_&#119875;&#119881;&#8800;1 are BIB without contamination from ghost collisions, while the histograms with &#119899;_&#119875;&#119881;=1 are dominated by the ghost collision events. As expected for BIB events, the hit occupancy diminishes as the radius of the barrel layers increases. The BIB events have lower hit occupancy than the ghost collision events. The statistical uncertainties are negligible and not visible.
</td>
<td align="right">
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCT_Barrel_Hitoccupancy.png][<img width="300" alt="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCT_Barrel_Hitoccupancy.png" src="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCT_Barrel_Hitoccupancy.png"></img>]]<br>
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCT_Barrel_Hitoccupancy.eps][eps file]]
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCT_Barrel_Hitoccupancy.pdf][pdf file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee>
<b> SCT average cluster size as a function of the detector layer for beam 1  and beam 2  for events with exactly one primary vertex (&#119899;_&#119875;&#119881;=1 ) and events with no PV or more than one (&#119899;_&#119875;&#119881;&#8800;1), in part of 2018 data. The SCT cluster size is defined as the number of adjacent strips that record a hit when a particle crosses the active area. 
The histograms with &#119899;_&#119875;&#119881;&#8800;1 are BIB without contamination from ghost collisions, while the histograms with &#119899;_&#119875;&#119881;=1 are dominated by the ghost collision events. As expected for BIB events, the average cluster size diminishes as the radius of the barrel layers increases. The BIB events have lower average cluster size than the ghost collision events. The statistical uncertainties are included.
</td>
<td align="right">
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCTavaragecluster_barrel.png][<img width="300" alt="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCTavaragecluster_barrel.png" src="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCTavaragecluster_barrel.png"></img>]]<br>
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCTavaragecluster_barrel.eps][eps file]]
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCTavaragecluster_barrel.pdf][pdf file]]
</td>
</tr>

<td bgcolor=#eeeeee>
<b> The z-asymmetry is defined to quantify the difference in the in-time hits in downstream and upstream endcaps as the difference between the number of SCT hits in a certain disk in the endcap side A and C.  The z-asymmetry in the SCT endcap disk 1  for hits produced by beam 1 (dashed-line) and beam 2 (solid-line) in 2018 data are shown. To suppress the contamination from ghost collisions, only events with &#119899;_&#119875;&#119881;&#8800;1 are considered. Since the hits generated by BIB are expected to be predominantly recorded in regions downstream from the nominal collision point, an asymmetry in the number of hits is expected between the regions upstream and downstream of the incoming beam. The separation between beam 1 and beam 2 distributions depends on the endcap disk position and increases for outer disks, since with increasing distance from interaction point the time difference also increases, it becomes less likely that collision products fake an asymmetry in outer disks. The statistical uncertainties are negligible and not visible.
</td>
<td align="right">
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_sct_disk1.png][<img width="300" alt="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCTavaragecluster_barrel.png" src="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_sct_disk1.png"></img>]]<br>
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_sct_disk1.eps][eps file]]
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_sct_disk1.pdf][pdf file]]
</td>
</tr>


<td bgcolor=#eeeeee>
<b> 
The z-asymmetry is defined to quantify the difference in the in-time hits in downstream and upstream endcaps as the difference between the number of SCT hits in a certain disk in the endcap side A and C. The z-asymmetry in the SCT endcap  disk 8 for hits produced by beam 1 (dashed-line) and beam 2 (solid-line) in 2018 data are shown. To suppress the contamination from ghost collisions, only events with &#119899;_&#119875;&#119881;&#8800;1  are considered. Since the hits generated by BIB are expected to be predominantly recorded in regions downstream from the nominal collision point, an asymmetry in the number of hits is expected between the regions upstream and downstream of the incoming beam. The separation between beam 1 and beam 2 distributions depends on the endcap disk position and increases for outer disks, since with increasing distance from interaction point the time difference also increases, it becomes less likely that collision products fake an asymmetry in outer disks. The statistical uncertainties are negligible and not visible.

</td>
<td align="right">
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_sct_disk8.png][<img width="300" alt="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCTavaragecluster_barrel.png" src="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_sct_disk8.png"></img>]]<br>
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_sct_disk8.eps][eps file]]
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_sct_disk8.pdf][pdf file]]
</td>
</tr>


<td bgcolor=#eeeeee>
<b> 
The z-asymmetry defined as the difference between the number of SCT in-time hits in side A and side C of a certain section in a barrel layer, is shown here. The SCT barrel layers are divided into 12 sections, split between A and C side: 6 in the positive z direction (0-125, 125-250, 250-375, 375-500, 500-625 and 625-800 mm) paired with the corresponding 6 ones in the negative z direction. The z-asymmetry in the SCT barrel layer 3 - section 4  for hits produced by beam 1 (dashed-line) and beam 2 (solid-line) in 2018 data are shown. To suppress the contamination from ghost collisions, only events with &#119899;_&#119875;&#119881;&#8800;1 are considered. The statistical uncertainties are negligible and not visible.
</td>
<td align="right">
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_SCT_Barrel_3_sec4.png][<img width="300" alt="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCTavaragecluster_barrel.png" src="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_SCT_Barrel_3_sec4.png"></img>]]<br>
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_SCT_Barrel_3_sec4.eps][eps file]]
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_SCT_Barrel_3_sec4.pdf][pdf file]]
</td>
</tr>


<td bgcolor=#eeeeee>
<b> 
The z-asymmetry defined as the difference between the number of SCT in-time hits in side A and side C of a certain section in a barrel layer, is shown here. The SCT barrel layers are divided into 12 sections, split between A and C side: 6 in the positive z direction (0-125, 125-250, 250-375, 375-500, 500-625 and 625-800 mm) paired with the corresponding 6 ones in the negative z direction.  The z-asymmetry in the SCT barrel layer 5 - section 6  for hits produced by beam 1 (dashed-line) and beam 2 (solid-line) in 2018 data are shown. To suppress the contamination from ghost collisions, only events with &#119899;_&#119875;&#119881;&#8800;1 are considered. The statistical uncertainties are negligible and not visible.
</td>
<td align="right">
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_SCT_Barrel_5_sec6.png][<img width="300" alt="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCTavaragecluster_barrel.png" src="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_SCT_Barrel_5_sec6.png"></img>]]<br>
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_SCT_Barrel_5_sec6.eps][eps file]]
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_SCT_Barrel_5_sec6.pdf][pdf file]]
</td>
</tr>


<td bgcolor=#eeeeee>
<b> The z-asymmetry is defined to quantify the difference in the in-time hits in downstream and upstream endcaps as the difference between the number of SCT hits in a certain disk in the endcap side A and C. The z-asymmetry in the SCT endcap layers for hits produced by beam 1 (filled markers) and beam 2 (open markers) in 2018 data is shown. To suppress the contamination from ghost collisions, only events with &#119899;_&#119875;&#119881;&#8800;1 are considered. The z-asymmetry is more pronounced in the outermost regions as expected. The statistical uncertainties are negligible and not visible.
</td>
<td align="right">
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_SCTEndcaps.png][<img width="300" alt="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCTavaragecluster_barrel.png" src="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_SCTEndcaps.png"></img>]]<br>
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_SCTEndcaps.eps][eps file]]
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_SCTEndcaps.pdf][pdf file]]
</td>
</tr>


<td bgcolor=#eeeeee>
<b> 
The z-asymmetry as the difference between the number of SCT in-time hits in side A and side C of a certain section in a barrel layer is shown here. The SCT barrel layers are divided into 12 sections, split between A and C side: 6 in the positive z direction (0-125, 125-250, 250-375, 375-500, 500-625 and 625-800 mm) paired with the corresponding 6 ones in the negative z direction. The z-asymmetry in the SCT barrel layers per z section for hits produced by beam 1 (filled markers) and beam 2 (open markers) in 2018 data is shown. The B3 to B6 are the SCT barrel layers. To suppress the contamination from ghost collisions, only events with &#119899;_&#119875;&#119881;&#8800;1 are considered. The z-asymmetry is more pronounced in the outermost regions as expected. The statistical uncertainties are negligible and not visible.
</td>
<td align="right">
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_sctBarrel_Run2.png][<img width="300" alt="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/SCTavaragecluster_barrel.png" src="https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_sctBarrel_Run2.png"></img>]]<br>
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_sctBarrel_Run2.eps][eps file]]
[[https://twiki.cern.ch/twiki/pub/AtlasPublic/NonCollisionBackgroundPublicResults/zasymmetry_sctBarrel_Run2.pdf][pdf file]]
</td>
</tr>

</table>
---++ Public Plots Approved in Spring of 2020

---+++ Muon segment activity from non-collision backgrounds

These plots illustrate muon segment activity in unpaired and empty bunch crossings during Run 2 pp data-taking at
sqrt(s)=13 TeV. The reconstructed direction of muon segments in the plane transverse and parallel to the beam pipe are shown. To improve the reconstruction efficiency for out-of-time and non-pointing muon segments, the data have been reconstructed using the cosmic data-taking configuration. Events are selected using the J30 (empty) and J12 and J50 (unpaired) L1 triggers, are required to have no reconstructed primary vertex and must contain at least one jet with pT>60 GeV, residing within |eta|<2.4. To remove events due to coherent noise in the calorimeters, and HEC or presampler spikes, loose LLP (long-lived particle) jet cleaning is applied to the leading jet in the event. Events in which the maximum energy deposit of the leading jet resides in the presampler or LAr EM endcaps are also rejected.

<table class="twikiTable" width="100%" bgcolor=#f5f5fa  border=1 cellpadding=10 cellspacing=10>
<tr>
<td bgcolor=#eeeeee>
<b> Direction of muon segments in XY plane for events from empty bunch crossings </b><br>
Distribution of the reconstructed direction of muon segments in the plane transverse to the beam pipe. The data have been reconstructed using the cosmic ray data-taking configuration, which improves the reconstruction efficiency for out-of-time and non-pointing muon segments. Events are recorded in empty bunch crossings during 2015-2018 13 TeV pp data-taking, are required to have no reconstructed primary vertex and must have a jet with pT>60 GeV within |eta|<2.4. Data quality cleaning is applied, and events where the leading jet fails the loose LLP jet cleaning cuts for EM coherent noise and HEC spikes are rejected. Events in which the maximum energy deposit of the leading jet resides in the presampler or LAr EM endcaps are also rejected to further remove noise activity in the LAr calorimeter. Events induced by cosmic ray muons tend to contain downward pointing muon segments, whereas events due to beam-induced backgrounds tend to contain muon segments pointing parallel to the beam pipe.
</td>
<td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hCosmicCalo_preSel__MSpxpy.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hCosmicCalo_preSel__MSpxpy.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hCosmicCalo_preSel__MSpxpy.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hCosmicCalo_preSel__MSpxpy.eps][eps file]]
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hCosmicCalo_preSel__MSpxpy.pdf][pdf file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee>
<b> Direction of muon segments in ZY plane for events from empty bunch crossings </b><br>
Distribution of the reconstructed direction of muon segments in the plane parallel to the beam pipe. The data have been reconstructed using the cosmic ray data-taking configuration, which improves the reconstruction efficiency for out-of-time and non-pointing muon segments. Events are recorded in empty bunch crossings during 2015-2018 13 TeV pp data-taking, are required to have no reconstructed primary vertex and must have a jet with pT>60 GeV within |eta|<2.4. Data quality cleaning is applied, and events where the leading jet fails the loose LLP jet cleaning cuts for EM coherent noise and HEC spikes are rejected. Events in which the maximum energy deposit of the leading jet resides in the presampler or LAr EM endcaps are also rejected to further remove noise activity in the LAr calorimeter. Events induced by cosmic ray muons tend to contain downward pointing muon segments, whereas events due to beam-induced backgrounds tend to contain muon segments pointing parallel to the beam pipe. An asymmetry between segments pointing in the positive and negative z direction is consistent with there being a larger contribution from beam-induced muons from beam 2 (z=1 direction) than beam 1 (z=-1 direction).
</td>
<td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hCosmicCalo_preSel__MSpzpy.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hCosmicCalo_preSel__MSpzpy.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hCosmicCalo_preSel__MSpzpy.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hCosmicCalo_preSel__MSpzpy.eps][eps file]]
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hCosmicCalo_preSel__MSpzpy.pdf][pdf file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee>
<b> Direction of muon segments in XY plane for events from unpaired bunch crossings </b><br>
Distribution of the reconstructed direction of muon segments in the plane transverse to the beam pipe. The data have been reconstructed using the cosmic ray data-taking configuration, which improves the reconstruction efficiency for out-of-time and non-pointing muon segments. Events are recorded in unpaired bunch crossings during 2015-2018 13 TeV pp data-taking, are required to have no reconstructed primary vertex and must have a jet with pT>60 GeV within |eta|<2.4. Data quality cleaning is applied, and events where the leading jet fails the loose LLP jet cleaning cuts for EM coherent noise and HEC spikes are rejected. Events in which the maximum energy deposit of the leading jet resides in the presampler or LAr EM endcaps are also rejected to further remove noise activity in the LAr calorimeter. Events induced by cosmic ray muons tend to contain downward pointing muon segments, whereas events due to beam-induced backgrounds tend to contain muon segments pointing parallel to the beam pipe.
</td>
<td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hBackground_preSel__MSpxpy.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hBackground_preSel__MSpxpy.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hBackground_preSel__MSpxpy.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hBackground_preSel__MSpxpy.eps][eps file]]
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hBackground_preSel__MSpxpy.pdf][pdf file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee>
<b> Direction of muon segments in ZY plane for events from unpaired bunch crossings </b><br>
Distribution of the reconstructed direction of muon segments in the plane parallel to the beam pipe. The data have been reconstructed using the cosmic ray data-taking configuration, which improves the reconstruction efficiency for out-of-time and non-pointing muon segments. Events are recorded in UNPAIRED bunch crossings during 2015-2018 13 TeV pp data-taking, are required to have no reconstructed primary vertex and must have a jet with pT>60 GeV within |eta|<2.4. Data quality cleaning is applied, and events where the leading jet fails the loose LLP jet cleaning cuts for EM coherent noise and HEC spikes are rejected. Events in which the maximum energy deposit of the leading jet resides in the presampler or LAr EM endcaps are also rejected to further remove noise activity in the LAr calorimeter. Events induced by cosmic ray muons tend to contain downward pointing muon segments, whereas events due to beam-induced backgrounds tend to contain muon segments pointing parallel to the beam pipe.
</td>
<td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hBackground_preSel__MSpzpy.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hBackground_preSel__MSpzpy.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hBackground_preSel__MSpzpy.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hBackground_preSel__MSpzpy.eps][eps file]]
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/Run2/hBackground_preSel__MSpzpy.pdf][pdf file]]
</td>
</tr>
</table>

 
---++ Public Plots Approved in Spring of 2017

<table class="twikiTable" width="100%" bgcolor=#f5f5fa  border=1 cellpadding=10 cellspacing=10>
<tr>
<td bgcolor=#eeeeee><b> ATLAS BCM background rate in 2015 </b><br>
The plot shows the rate of LHC beam-induced background reaching ATLAS, as measured with the Beam Conditions Monitor during the proton-proton run in 2015. Each point represents the rate of BCM triggers at the start of an ATLAS run, averaged over the first ten minutes of stable beams. The BCM trigger rates are before prescale and are normalized by the 600s duration of the luminosity blocks used, and by the sum of bunch intensities in unpaired isolated bunches in each beam.
A systematically higher rate of Beam 1 than Beam 2 is observed in 2015 data and is consistent with previous studies. 
</td><td align="right" bgcolor=#eeeeee>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2017/2015BCM_RatesTime_Prel.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2017/2015BCM_RatesTime_Prel.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2017/2015BCM_RatesTime_Prel.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2017/2015BCM_RatesTime_Prel.png][eps file]]
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2017/2015BCM_RatesTime_Prel.pdf][pdf file]]
</td>
</tr>
<tr>
<td><b> ATLAS BCM background rate in 2016 </b><br>
The plot shows the rate of LHC beam-induced background reaching ATLAS, as measured with the Beam Conditions Monitor during the proton-proton run in 2016. Each point represents the rate of BCM triggers at the start of an ATLAS run, averaged over the first ten minutes of stable beams. The BCM trigger rates are before prescale and are normalized by the 600s duration of the luminosity blocks used, and by the sum of bunch intensities in unpaired isolated bunches in each beam.
A systematically higher rate of Beam 1 than Beam 2 is observed in 2016 data and is consistent with previous studies. An increased Beam 1 background due to the pressure bump test on 25/9/16 is apparent in subsequent LHC Fills 5332, 5337, 5338, 5339, and is thought to be due to slow out-gassing of the beam screen in the triplet. 
</td><td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2017/2016BCM_RatesTime_Prel.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2017/2016BCM_RatesTime_Prel.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2017/2016BCM_RatesTime_Prel.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2017/2016BCM_RatesTime_Prel.eps][eps file]]
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2017/2016BCM_RatesTime_Prel.pdf][pdf file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee><b> ATLAS Background rate evolution during an entire fill </b><br>
The plot shows the rate of LHC beam-induced background reaching ATLAS, as measured with the Beam Conditions Monitor during LHC proton Fill 5111 in 2016. Fill 5111 is selected by the LHC Beam Background Study group as a typical example, for comparison with background rates in the other LHC experiments for the IPAC conference. Each point represents the rate of BCM triggers in one ATLAS luminosity block. The BCM trigger rates are before prescale and are normalized by the duration of the luminosity block, and by the sum of bunch intensities in unpaired isolated bunches in each beam. The vertical line indicates the start of STABLE BEAMS. A systematically higher rate of Beam 1 than Beam 2 is observed in 2016 data and is consistent with previous studies. An increase in rate is observed during the LHC beam energy ramp, prior to stable beams, then falls off with the beam intensity over the duration of the fill, because the background rate is dominated by residual beam-gas interactions. 
</td><td align="right" bgcolor=#eeeeee>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2017/BCM_RatesTime_Prelim.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2017/BCM_RatesTime_Prelim.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2017/BCM_RatesTime_Prelim.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2017/BCM_RatesTime_Prelim.eps][eps file]]
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2017/BCM_RatesTime_Prelim.pdf][pdf file]]
</td>
</tr>
</table>


---++ Results for ICHEP 2016

<table class="twikiTable" width="100%" bgcolor=#f5f5fa  border=1 cellpadding=10 cellspacing=10>
<tr>
<td bgcolor=#eeeeee><b> Rate of on-track pixel clusters in 2016 </b><br>
The plots show the rate of on-track pixel clusters versus the azimuthal coordinate of the pixel cluster
in all unpaired isolated bunches (upper plots for unpaired isolated beam1, lower plots for unpaired
isolated beam 2), during the different pressure bumps at 150 m, 58 m, 19 m from ATLAS run 298771
(LHC Fill 4905). Beam1 indicates the beam circulating clockwise, and phi=0 points to the centre of
LHC. The distributions are normalized by the duration of the luminosity block slice, indicated in the
right hand side table. All triggers are used in the physics_Background stream. The main phi variation
indicates the influence of accelerator optics on the background reaching ATLAS. Background
originating at 19 m does not cross any LHC magnetic element, and therefore a uniform distribution is
expected. The fine structure is due to geometrical effects of module overlaps and ganged pixels. The
small dips are due to inoperable pixel modules in some layers.
</td><td align="right" bgcolor=#eeeeee>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb260_270_clusphi_UPB1.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb260_270_clusphi_UPB1.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb260_270_clusphi_UPB1.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb260_270_clusphi_UPB1.eps][eps file]]
</td>
</tr>
<tr>
<td><b> Rate of on-track pixel clusters in 2016 </b><br>
The plots show the rate of on-track pixel clusters versus the azimuthal coordinate of the pixel cluster
in all unpaired isolated bunches (upper plots for unpaired isolated beam1, lower plots for unpaired
isolated beam 2), during the different pressure bumps at 150 m, 58 m, 19 m from ATLAS run 298771
(LHC Fill 4905). Beam1 indicates the beam circulating clockwise, and phi=0 points to the centre of
LHC. The distributions are normalized by the duration of the luminosity block slice, indicated in the
right hand side table. All triggers are used in the physics_Background stream. The main phi variation
indicates the influence of accelerator optics on the background reaching ATLAS. Background
originating at 19 m does not cross any LHC magnetic element, and therefore a uniform distribution is
expected. The fine structure is due to geometrical effects of module overlaps and ganged pixels. The
small dips are due to inoperable pixel modules in some layers.
</td><td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb260_270_clusphi_UPB2.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb260_270_clusphi_UPB2.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb260_270_clusphi_UPB2.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb260_270_clusphi_UPB2.eps][eps file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee><b> Rate of on-track pixel clusters in 2016 </b><br>
The plots show the rate of on-track pixel clusters versus the azimuthal coordinate of the pixel cluster
in all unpaired isolated bunches (upper plots for unpaired isolated beam1, lower plots for unpaired
isolated beam 2), during the different pressure bumps at 150 m, 58 m, 19 m from ATLAS run 298771
(LHC Fill 4905). Beam1 indicates the beam circulating clockwise, and phi=0 points to the centre of
LHC. The distributions are normalized by the duration of the luminosity block slice, indicated in the
right hand side table. All triggers are used in the physics_Background stream. The main phi variation
indicates the influence of accelerator optics on the background reaching ATLAS. Background
originating at 19 m does not cross any LHC magnetic element, and therefore a uniform distribution is
expected. The fine structure is due to geometrical effects of module overlaps and ganged pixels. The
small dips are due to inoperable pixel modules in some layers.
</td><td align="right" bgcolor=#eeeeee>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb310_320_clusphi_UPB1.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb310_320_clusphi_UPB1.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb310_320_clusphi_UPB1.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb310_320_clusphi_UPB1.eps][eps file]]
</td>
</tr>
<tr>
<td><b> Rate of on-track pixel clusters in 2016 </b><br>
The plots show the rate of on-track pixel clusters versus the azimuthal coordinate of the pixel cluster
in all unpaired isolated bunches (upper plots for unpaired isolated beam1, lower plots for unpaired
isolated beam 2), during the different pressure bumps at 150 m, 58 m, 19 m from ATLAS run 298771
(LHC Fill 4905). Beam1 indicates the beam circulating clockwise, and phi=0 points to the centre of
LHC. The distributions are normalized by the duration of the luminosity block slice, indicated in the
right hand side table. All triggers are used in the physics_Background stream. The main phi variation
indicates the influence of accelerator optics on the background reaching ATLAS. Background
originating at 19 m does not cross any LHC magnetic element, and therefore a uniform distribution is
expected. The fine structure is due to geometrical effects of module overlaps and ganged pixels. The
small dips are due to inoperable pixel modules in some layers.
</td><td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb310_320_clusphi_UPB2.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb310_320_clusphi_UPB2.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb310_320_clusphi_UPB2.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb310_320_clusphi_UPB2.eps][eps file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee><b> Rate of on-track pixel clusters in 2016 </b><br>
The plots show the rate of on-track pixel clusters versus the azimuthal coordinate of the pixel cluster
in all unpaired isolated bunches (upper plots for unpaired isolated beam1, lower plots for unpaired
isolated beam 2), during the different pressure bumps at 150 m, 58 m, 19 m from ATLAS run 298771
(LHC Fill 4905). Beam1 indicates the beam circulating clockwise, and phi=0 points to the centre of
LHC. The distributions are normalized by the duration of the luminosity block slice, indicated in the
right hand side table. All triggers are used in the physics_Background stream. The main phi variation
indicates the influence of accelerator optics on the background reaching ATLAS. Background
originating at 19 m does not cross any LHC magnetic element, and therefore a uniform distribution is
expected. The fine structure is due to geometrical effects of module overlaps and ganged pixels. The
small dips are due to inoperable pixel modules in some layers.
</td><td align="right" bgcolor=#eeeeee>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb360_365_clusphi_UPB1.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb360_365_clusphi_UPB1.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb360_365_clusphi_UPB1.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb360_365_clusphi_UPB1.eps][eps file]]
</td>
</tr>
<tr>
<td><b> Rate of on-track pixel clusters in 2016 </b><br>
The plots show the rate of on-track pixel clusters versus the azimuthal coordinate of the pixel cluster
in all unpaired isolated bunches (upper plots for unpaired isolated beam1, lower plots for unpaired
isolated beam 2), during the different pressure bumps at 150 m, 58 m, 19 m from ATLAS run 298771
(LHC Fill 4905). Beam1 indicates the beam circulating clockwise, and phi=0 points to the centre of
LHC. The distributions are normalized by the duration of the luminosity block slice, indicated in the
right hand side table. All triggers are used in the physics_Background stream. The main phi variation
indicates the influence of accelerator optics on the background reaching ATLAS. Background
originating at 19 m does not cross any LHC magnetic element, and therefore a uniform distribution is
expected. The fine structure is due to geometrical effects of module overlaps and ganged pixels. The
small dips are due to inoperable pixel modules in some layers.
</td><td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb360_365_clusphi_UPB2.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb360_365_clusphi_UPB2.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb360_365_clusphi_UPB2.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/run00298771_DataPrep_lb360_365_clusphi_UPB2.eps][eps file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee><b> Radial coordinate of CSC muon segments </b><br>
The plot shows the radial coordinate of CSC muon segments for LHC Fill 4905 (Atlas run
298771) in luminosity block intervals corresponding to the different increase of local pressure at 150 m, 58
m, 19 m from the interaction point and also for standard running (no bump). The distributions are
normalized by the duration of the luminosity block slice, indicated in the right hand side table. Events
without any primary vertex in unpaired bunches are selected. A cut on the difference
between the polar position and the polar direction of the muon segment is applied in order to select
segments produced by background muons travelling parallel to the beam axis.
</td><td align="right" bgcolor=#eeeeee>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p12.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p12.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p12.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p12.pdf][pdf file]]
</td>
</tr>

<tr>
<td><b> Spatial distributions of CSC muon segments </b><br>
Spatial distributions of CSC muon segments during LHC fill n. 4905 (Atlas run n. 298771) in the
luminosity block intervals corresponding to the local increase of the beam pipe pressure at 150 m (top
right), 58 m (bottom left), 19 m (bottom right). The top left plot corresponds to standard operating values of
the pressure. Events without any primary vertex in unpaired isolated (> 175ns) bunches are selected. A cut
on the difference between the polar position and the polar direction of the muon segment is
applied. The distributions are normalized by the duration of the luminosity block intervals.
</td><td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13a.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13a.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13a.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13a.pdf][pdf file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee><b> Spatial distributions of CSC muon segments </b><br>
Spatial distributions of CSC muon segments during LHC fill n. 4905 (Atlas run n. 298771) in the
luminosity block intervals corresponding to the local increase of the beam pipe pressure at 150 m (top
right), 58 m (bottom left), 19 m (bottom right). The top left plot corresponds to standard operating values of
the pressure. Events without any primary vertex in unpaired isolated (> 175ns) bunches are selected. A cut
on the difference between the polar position and the polar direction of the muon segment is
applied. The distributions are normalized by the duration of the luminosity block intervals.
</td><td align="right" bgcolor=#eeeeee>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13b.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13b.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13b.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13b.pdf][pdf file]]
</td>
</tr>
<tr>
<td><b> Spatial distributions of CSC muon segments </b><br>
Spatial distributions of CSC muon segments during LHC fill n. 4905 (Atlas run n. 298771) in the
luminosity block intervals corresponding to the local increase of the beam pipe pressure at 150 m (top
right), 58 m (bottom left), 19 m (bottom right). The top left plot corresponds to standard operating values of
the pressure. Events without any primary vertex in unpaired isolated (> 175ns) bunches are selected. A cut
on the difference between the polar position and the polar direction of the muon segment is
applied. The distributions are normalized by the duration of the luminosity block intervals.
</td><td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13c.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13c.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13c.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13c.pdf][pdf file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee><b> Spatial distributions of CSC muon segments </b><br>
Spatial distributions of CSC muon segments during LHC fill n. 4905 (Atlas run n. 298771) in the
luminosity block intervals corresponding to the local increase of the beam pipe pressure at 150 m (top
right), 58 m (bottom left), 19 m (bottom right). The top left plot corresponds to standard operating values of
the pressure. Events without any primary vertex in unpaired isolated (> 175ns) bunches are selected. A cut
on the difference between the polar position and the polar direction of the muon segment is
applied. The distributions are normalized by the duration of the luminosity block intervals.
</td><td align="right" bgcolor=#eeeeee>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13d.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13d.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13d.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p13d.pdf][pdf file]]
</td>
</tr>
<tr>
<td><b> Space distributions of CSC muon segments </b><br>
Space distributions of CSC muon segments during LHC fill n. 4905 (Atlas run n. 298771) when the beam
pipe pressure was increased at 150 m from the interaction point. Unpaired bunches from beam 1 (left
column) and beam 2 (right column) are selected. Upper row plots show the distributions of muon segments
from CSC End Cap C, while the bottom row shows the distributions for CSC End Cap A. Events without
any primary vertex are selected and a cut on the difference between the polar position and
the polar direction of the muon segment is applied. The distributions are normalized by the duration of the
luminosity block interval when the pressure was stable.
</td><td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14a.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14a.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14a.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14a.pdf][pdf file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee><b> Space distributions of CSC muon segments </b><br>
Space distributions of CSC muon segments during LHC fill n. 4905 (Atlas run n. 298771) when the beam
pipe pressure was increased at 150 m from the interaction point. Unpaired bunches from beam 1 (left
column) and beam 2 (right column) are selected. Upper row plots show the distributions of muon segments
from CSC End Cap C, while the bottom row shows the distributions for CSC End Cap A. Events without
any primary vertex are selected and a cut on the difference between the polar position and
the polar direction of the muon segment is applied. The distributions are normalized by the duration of the
luminosity block interval when the pressure was stable.
</td><td align="right" bgcolor=#eeeeee>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14b.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14b.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14b.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14b.pdf][pdf file]]
</td>
</tr>
<tr>
<td><b> Space distributions of CSC muon segments </b><br>
Space distributions of CSC muon segments during LHC fill n. 4905 (Atlas run n. 298771) when the beam
pipe pressure was increased at 150 m from the interaction point. Unpaired bunches from beam 1 (left
column) and beam 2 (right column) are selected. Upper row plots show the distributions of muon segments
from CSC End Cap C, while the bottom row shows the distributions for CSC End Cap A. Events without
any primary vertex are selected and a cut on the difference between the polar position and
the polar direction of the muon segment is applied. The distributions are normalized by the duration of the
luminosity block interval when the pressure was stable.
</td><td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14c.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14c.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14c.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14c.pdf][pdf file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee><b> Space distributions of CSC muon segments </b><br>
Space distributions of CSC muon segments during LHC fill n. 4905 (Atlas run n. 298771) when the beam
pipe pressure was increased at 150 m from the interaction point. Unpaired bunches from beam 1 (left
column) and beam 2 (right column) are selected. Upper row plots show the distributions of muon segments
from CSC End Cap C, while the bottom row shows the distributions for CSC End Cap A. Events without
any primary vertex are selected and a cut on the difference between the polar position and
the polar direction of the muon segment is applied. The distributions are normalized by the duration of the
luminosity block interval when the pressure was stable.
</td><td align="right" bgcolor=#eeeeee>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14d.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14d.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14d.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p14d.pdf][pdf file]]
</td>
</tr>

<tr>
<td><b> Distribution of the time of the leading calorimeter clusters vs. pseudorapidity </b><br>
Distribution of the time of the leading calorimeter clusters vs. pseudorapidity in runs taken
from May 12 to June 2nd in events from unpaired isolated bunches, without any primary
vertex and passing a trigger requiring a jet with pT> 12 GeV in unpaired isolated bunches.
The cut on the leading cluster pT is 20 GeV. Event cleaning is applied by removing the
events with at least one jet failing the loose jet cleaning cuts for EM coherent noise and
HEC spikes. The distributions for each run are normalized by the duration of the run in
seconds, and the plot represents the average over all the runs.
</td><td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p15.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p15.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p15.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p15.pdf][pdf file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee><b> Eta versus time distribution of leading calorimeter clusters </b><br>
Eta versus time distribution of leading calorimeter clusters in runs from May 12 to June 2nd, in
events from unpaired bunches in beam 1, without any primary vertex and passing a trigger a
trigger requiring a jet with pT> 12 GeV in unpaired isolated bunches. The cut on the leading
cluster pT is 20 GeV. Event cleaning is applied by removing the events with at least one jet
failing the loose jet cleaning cuts for EM coherent noise and HEC spikes. The distributions for
each run are normalized by the duration of the run in seconds, and the plot represents the
average over all the runs.
</td><td align="right" bgcolor=#eeeeee>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p16.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p16.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p16.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p16.pdf][pdf file]]
</td>
</tr>
<tr>
<td><b> Eta versus time distribution of leading calorimeter clusters, beam 2 </b><br>
Eta versus time distribution of leading calorimeter clusters in runs from May 12 to June 2nd,
in events from unpaired bunches in beam 2, without any primary vertex and passing a
trigger requiring a jet with pT> 12 GeV in unpaired isolated bunches. The cut on the
leading cluster pT is 20 GeV. Event cleaning is applied by removing the events with at least
one jet failing the loose jet cleaning cuts for EM coherent noise and HEC spikes. The
distributions for each run are normalized by the duration of the run in seconds, and the plot
represents the average over all the runs.
</td><td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p17.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p17.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p17.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p17.pdf][pdf file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee><b> Distribution in space of the CSC muon segments </b><br>
Distribution in space of the CSC muon segments in ATLAS runs from May 12 to June
2nd , in events from unpaired bunches, without any primary vertex. A cut
on the difference between the polar position and the polar direction of the muon segment
is applied. The distributions for each run are normalized by the duration of the run in
seconds, and the plot represents the average over all the runs.
</td><td align="right" bgcolor=#eeeeee>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p18.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p18.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p18.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p18.pdf][pdf file]]
</td>
</tr>
<tr>
<td><b> Distribution in space of the CSC muon segments </b><br>
Distribution in space of the CSC muon segments in runs from May 12 to June 2nd , in events
from unpaired bunches, without any primary vertex and passing a trigger requiring a jet with
pT > 12 GeV in unpaired isolated bunches. A cut on the difference between the
polar position and the polar direction of the muon segment is applied. The distributions for
each run are normalized by the duration of the run in seconds, and the plot represents the
average over all the runs.
</td><td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p19.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p19.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p19.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p19.pdf][pdf file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee><b> Distribution in the transverse plane of the CSC muon segments </b><br>
Distribution in the transverse plane of the CSC muon segments in EndCap C, in runs
from May 12 to June 2nd in events from unpaired bunches in beam 1, without any
primary vertex and passing a trigger requiring a jet with pT> 12 GeV in unpaired isolated
bunches. A cut on the difference between the polar position and the polar
direction of the muon segment is applied. The distributions for each run are normalized
by the duration of the run in seconds, and the plot represents the average over all the
runs.
</td><td align="right" bgcolor=#eeeeee>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p20.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p20.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p20.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p20.pdf][pdf file]]
</td>
</tr>
<tr>
<td><b> Distribution in the plane transverse to the beam pipe of CSC muon segments </b><br>
Distribution in the plane transverse to the beam pipe of the CSC muon segments in
!EndCap A, in runs from May 13 to June 2nd, in events from unpaired bunches in beam 1,
without any primary vertex and passing a trigger requiring a jet with pT> 12 GeV in
unpaired isolated bunches. A cut on the difference between the polar
position and the polar direction of the muon segment is applied. The distributions for
each run are normalized by the duration of the run in seconds, and the plot represents the
average over all the runs.
</td><td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p21.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p21.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p21.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p21.pdf][pdf file]]
</td>
</tr>
<tr>
<td bgcolor=#eeeeee><b> Distribution of the CSC muon segments in the transverse plane for !EndCap C </b><br>
Distribution of the CSC muon segments in the transverse plane for !EndCap C, from May
13 to June 2nd 2016, in events from unpaired bunches in beam 2, without any primary
vertex and passing a trigger requiring a jet with pT> 12 GeV in unpaired isolated
bunches. A cut on the difference between the polar position and the polar
direction of the muon segment is applied. The distributions for each run are normalized
by the duration of the run in seconds, and the plot represents the average over all the
runs.
</td><td align="right" bgcolor=#eeeeee>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p22.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p22.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p22.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p22.pdf][pdf file]]
</td>
</tr>
<tr>
<td><b> Distribution of the CSC muon segments in the transverse plane for !EndCap A </b><br>
Distribution of the CSC muon segments in the transverse plane for !EndCap A in runs
from May 13 to June 2, in events from unpaired bunches in beam 2, without any primary
vertex and passing a trigger requiring a jet with pT> 12 GeV in unpaired isolated
bunches. A cut on the difference between the polar position and the polar
direction of the muon segment is applied. The distributions for each run are normalized
by the duration of the run in seconds, and the plot represents the average over all the
runs.
</td><td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p23.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p23.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p23.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2016/ICHEP/ATL-COM-DAPR-2016-011_p23.pdf][pdf file]]
</td>
</tr>
</table>


---+ Results from Run 1

Below are the public results from the Non-Colliding Backgrounds group in Run 1.

---++ 2012 data preliminary plots

---+++ 25ns vs 50ns bunch spacing comparison

The following plots show comparisons of beam backgrounds in standard 50 ns runs of 2012 and of the short 25 ns run at the very end of 2012. For the 50 ns runs we only use data before Technical Stop 3 (TS3, starting 17. September), because conditions early in the year were better comparable to those during the 25 ns run. In particular we observed a significant - unexplained - rise of ghost charge after TS3, while ghost charge interactions were largely absent due to the better isolation of unpaired bunches in the 25 ns run. Also, some instrumental noise in the BCM detector disturbed the data late in 2012, but was absent during the 25 ns run and in all runs prior to TS3. In normal 50 ns running the bunch pattern included three unpaired isolated and three non-isolated bunches per beam. For the 25 ns beam 12 isolated bunches per beam are used for these plots. The requirement for a bunch to be isolated is that there is no bunch in the other beam within 150 ns.
In all following plots, the lower x-axis labels indicate the BCIDs in the 50 ns run, while the upper labels give those in the 25 ns run.

<table class="twikiTable" width="100%" bgcolor=#f5f5fa  border=1 cellpadding=10 cellspacing=10>
<td bgcolor=#eeeeee><b> Beam background rate from BCM </b><br>
Beam background rate measured by the L1 BCM AC CA UNPAIRED ISO trigger. This trigger selects events with an early signal on one side and an in-time signal on the other, characteristic of beam background tracks. Standard runs with 50 ns bunch spacing and 1368 colliding bunches taken before TS3 are compared to a run with 25 ns bunch spacing that was taken during fill 3453. The fills with 1368 colliding bunches had a short train at the beginning containing 3 unpaired isolated bunches in each beam. Two trains with unpaired bunches only are shown from the bunch pattern in fill 3453. Entries are normalised by the bunch intensity. Only events from luminosity blocks passing general quality requirements are considered.
</td>
<td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/25ns/beamgas-BCM-25ns.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/25ns/beamgas-BCM-25ns.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/25ns/beamgas-BCM-25ns.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/25ns/beamgas-BCM-25ns.eps][eps file]]
</td>
</tr>

<table class="twikiTable" width="100%" bgcolor=#f5f5fa  border=1 cellpadding=10 cellspacing=10>
<td bgcolor=#eeeeee><b> Ghost charge interaction rate </b><br>
Ghost charge interaction rate measured by the L1 BCM Wide UNPAIRED ISO and L1 BCM Wide UNPAIRED NONISO trigger. These triggers select events with an in-time coincidence on both sides, characteristic of collision an the interaction point. Ghost charge is due to a part of the LHC beam having spread into nominally empty BCIDs such that they can produce collisions with unpaired bunches in the other beam. Standard runs with 50 ns bunch spacing and 1368 colliding bunches taken before TS3 are compared to a run with 25 ns bunch spacing that was taken during fill 3453. The fills with 1368 colliding bunches had a short train at the beginning consisting of 6 unpaired bunches for each beam. Two trains with unpaired bunches only are shown from the bunch pattern in fill 3453. The rate of ghost charge interactions rises with decreasing bunch isolation (in the 25 ns run all bunches are well isolated). Entries are normalised by the bunch intensity. Only events from luminosity blocks passing general quality requirements are considered.
</td>
<td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/25ns/ghostBCM_25ns.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/25ns/ghostBCM_25ns.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/25ns/ghostBCM_25ns.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/25ns/ghostBCM_25ns.eps][eps file]]
</td>
</tr>
</table>

---+++ BCM Background rates

<table class="twikiTable" width="100%" bgcolor=#f5f5fa  border=1 cellpadding=10 cellspacing=10>
<td bgcolor=#eeeeee><b> BCM Background rate per run </b><br>
Rate of BCM background-like Level 1 triggers in unpaired isolated bunches throughout 2012 in Stable Beams periods. Unpaired isolated bunches are required to have no bunch in the other beam within 150 ns. Each dot represents the average rate over an ATLAS run. Since the background is dominated by loss-processes which are proportional to beam intensity, the rates have been normalized to an intensity of 1011 protons in order to remove the effect of intensity variations. At the start of an LHC fill on 1st November unusually high backgrounds were observed, and the corresponding ATLAS run is seen as an outlier in this plot.
</td>
<td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/bcmbkgd-2012-upi-run.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/bcmbkgd-2012-upi-run.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/bcmbkgd-2012-upi-run.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/bcmbkgd-2012-upi-run.eps][eps file]]
</td>
</tr>

<tr>
<td bgcolor=#eeeeee><b> BCM Background rate per Luminosity Block </b><br>
Rate of BCM background-like Level 1 triggers in unpaired isolated bunches throughout 2012 in Stable Beams periods. Unpaired isolated bunches are required to have no bunch in the other beam within 150 ns. Each dot represents the average rate over one ATLAS luminosity block, corresponding to typically 60 seconds of data-taking. Since the background is dominated by loss-processes which are proportional to beam intensity, the rates have been normalized to an intensity of 1011 protons in order to remove the effect of intensity variations. At the start of an LHC fill on 1st November unusually high backgrounds were observed. This background came back to normal level within a hour. In the plot this background decay is seen as a vertical string of points above the normal level.
</td>
<td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/bcmbkgd-2012-upi-lb.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/bcmbkgd-2012-upi-lb.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/bcmbkgd-2012-upi-lb.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/NonCollisionBackground/2012/bcmbkgd-2012-upi-lb.eps][eps file]]
</td>
</tr>
</table>

---++ 2011 data preliminary plots
---+++ BCM Halo trigger rates

<table class="twikiTable" width="100%" bgcolor=#f5f5fa  border=1 cellpadding=10 cellspacing=10>
<td bgcolor=#eeeeee><b> BCM Halo rate vs LHC Fill</b><br>
Beam-induced background rates as measured by Beam Condition Monitor (BCM). The trigger rate is obtained from the L1_BCM_AC_CA trigger in Unpaired Isolated bunches (no proton bunches in the other beam within 75 ns).
The trigger rate for the 2011 data-taking period in is normalised to 10^11 protons.
</td><td align="right">
[[%ATTACHURLPATH%/BcmSpecificRatePaper_2011.png][<img width="500" alt="%ATTACHURLPATH%/BcmSpecificRatePaper_2011.png" src="%ATTACHURLPATH%/BcmSpecificRatePaper_2011.png"></img>]]<br>
[[%ATTACHURLPATH%/BcmSpecificRatePaper_2011.eps][eps file]]<br>
</td>
</tr>

<tr>
<td bgcolor=#eeeeee><b>BCM Halo rate during a single LHC Fill</b><br>
The BCM_AC_CA halo signal is formed by a coincidence of an early hit on one side
of the interaction point and and in-time hit on the other side. The time windows for accepting
a hit are 5.5 ns wide and centered around the expected incoming/outgoing time.
The Figure shows the BCM_AC_CA Halo rate during the start of an LHC fill for
unpaired isolated bunches (no bunch in the other beam within 75 ns). Also shown are the 
beam energy and the residual pressures in the vacuum pipe at z = 58 m and z = 22 m from the interaction point. 
The important phases: Injection (intensity increase), Ramp (energy increase), Adjust 
(bringing beams into collision) and Stable Beams (colliding) are indicated on top of the plot.
The pressure at 58 m correlates with the intensity increase, while that at 22 m rises
during the energy ramp. The plot shows that the background measured by the BCM halo monitor 
is mostly determined by the pressure at 22 m. The zero-point of the time axis is set to the start
of ATLAS data-taking in this LHC fill.
</td><td align="right">
[[%ATTACHURLPATH%/beamhalo.png][<img width="500" alt="%ATTACHURLPATH%/beamhalo.png" src="%ATTACHURLPATH%/beamhalo.png"></img>]]<br>
[[%ATTACHURLPATH%/beamhalo.eps][eps file]]<br>
</td>
</tr>
</table>


---+++ Beam Background Rejection
<table class="twikiTable" width="100%" bgcolor=#f5f5fa  border=1 cellpadding=10 cellspacing=10>
<!----------------- EXAMPLE BELOW
<td bgcolor=#eeeeee><b> First plot</b><br>
CAPTION HERE
</td><td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/2011/DataSummary/figs/TEST.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/2011/DataSummary/figs/TEST.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/2011/DataSummary/figs/TEST.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/2011/DataSummary/figs/TEST.eps][eps file]]<br>
</td>
</tr>
<tr>
<td bgcolor=#eeeeee><b>Second Plot</b><br>
CAPTION
</td><td align="right">
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/2011/DataSummary/figs/TEST.png][<img width="300" alt="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/2011/DataSummary/figs/TEST.png" src="https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/2011/DataSummary/figs/TEST.png"></img>]]<br>
[[https://atlas.web.cern.ch/Atlas/GROUPS/DATAPREPARATION/PublicPlots/2011/DataSummary/figs/TEST.eps][eps file]]<br>
</td>
</tr>
-->

<tr>
<td bgcolor=#eeeeee><b> Delta theta in CSC </b><br>
Difference between the reconstructed theta direction
and the theta position for the muon segments in CSC.
Data from unpaired (non-colliding) bunches (points) are cleaned from noise
and parasitic collisions by requiring no primary vertex.
There is an additional requirement of at least one jet in order to assure a calorimeter activity.
In this way, an almost pure sample of beam induced background is prepared.
Beam background events are compared to the physics collision events with muon triggers (filled histogram)
where also at least one jet is required.
Beam background data are characterised by a muon traversing the detector
in a direction parallel to the beam pipe.
Therefore, the expected value is ~ 11 degrees, for the CSC detector.
For muons coming from collisions, we expect delta theta ~ 0.
The tail for collision data may come from resolution, magnetic field or cavern background.
</td><td align="right">
[[%ATTACHURLPATH%/bb_thetaCSC.png][<img width="300" alt="%ATTACHURLPATH%/bb_thetaCSC.png" src="%ATTACHURLPATH%/bb_thetaCSC.png"></img>]]<br>
[[%ATTACHURLPATH%/bb_thetaCSC.eps][eps file]]<br>
</td>
</tr>

<tr>
<td bgcolor=#eeeeee><b> Delta theta in the inner MDT end-cap </b><br>
Difference between the reconstructed theta direction
and the theta position for the muon segments in the inner MDT end-cap.
Data from unpaired (non-colliding) bunches (points) are cleaned from noise
and parasitic collisions by requiring no primary vertex.
There is an additional requirement of at least one jet in order to assure a calorimeter activity.
In this way, an almost pure sample of beam induced background is prepared.
Beam background events are compared to the physics collision events with muon triggers (filled histogram)
where also at least one jet is required.
Beam background data are characterised by a muon traversing the detector
in a direction parallel to the beam pipe.
Therefore, the expected value is > 14 degrees, for the inner MDT end-cap.
For muons coming from collisions, we expect delta theta ~ 0.
The tail for collision data may come from resolution, magnetic field or cavern background.
</td><td align="right">
[[%ATTACHURLPATH%/bb_thetaMDT.png][<img width="300" alt="%ATTACHURLPATH%/bb_thetaMDT.png" src="%ATTACHURLPATH%/bb_thetaMDT.png"></img>]]<br>
[[%ATTACHURLPATH%/bb_thetaMDT.eps][eps file]]<br>
</td>
</tr>

<tr>
<td bgcolor=#eeeeee><b> CSC time </b><br>
Reconstructed time of the CSC muon segments in the beam background data.
A cut on the difference between the reconstructed position and the reconstructed direction > 5 degrees is applied in order to select muon candidates
going in a direction parallel to the beam-pipe.
Data from unpaired (non-colliding) bunches (points) are cleaned from noise
and parasitic collisions by requiring no primary vertex.
There is an additional requirement of at least one jet in order to assure a calorimeter activity.
In this way, an almost pure sample of beam induced background is prepared.
Beam background events are compared to the physics collision events with muon triggers (filled histogram)
where also at least one jet is required.
In the beam background events, one expects in-time muon segments (peak at 0 ns) for
the beam halo muons leaving the detector.
If the muon leaves a segment on the way into the detector, the expected time is ~ 50 ns
(twice the time-of-flight between the interaction point and the CSC position).
In the collision events, we always expect in-time muon segments.
The peaks at +-50 ns correspond to the out-of-time pile-up (50 ns bunch spacing).
</td><td align="right">
[[%ATTACHURLPATH%/bb_timeCSC.png][<img width="300" alt="%ATTACHURLPATH%/bb_timeCSC.png" src="%ATTACHURLPATH%/bb_timeCSC.png"></img>]]<br>
[[%ATTACHURLPATH%/bb_timeCSC.eps][eps file]]<br>
</td>
</tr>

<tr>
<td bgcolor=#eeeeee><b> CSC time difference between side A and C </b><br>
Time difference of the muon segments on side A and C that are matched to a calorimeter cluster.
A cut on the difference between the reconstructed position and the reconstructed direction
is applied in order to select muon candidates
going in a direction parallel to the beam-pipe.
Data from unpaired (non-colliding) bunches (points) are cleaned from noise
and parasitic collisions by requiring no primary vertex.
There is an additional requirement of at least one jet in order to assure a calorimeter activity.
In this way, an almost pure sample of beam induced background is prepared.
The muon segments are matched to a calorimeter cluster by comparing their phi and R position.
The idea is to select events where a halo muon leaves hits in the muon chambers on both sides
and also deposits energy in the calorimeter.
</td><td align="right">
[[%ATTACHURLPATH%/bb_timeDiffAC.png][<img width="300" alt="%ATTACHURLPATH%/bb_timeDiffAC.png" src="%ATTACHURLPATH%/bb_timeDiffAC.png"></img>]]<br>
[[%ATTACHURLPATH%/bb_timeDiffAC.eps][eps file]]<br>
</td>
</tr>

<tr>
<td bgcolor=#eeeeee><b> Position of the CSC segments </b><br>
Position of the muon segments in the beam background events.
A cut on the difference between the reconstructed position and the reconstructed direction
is applied in order to select muon candidates
going in a direction parallel to the beam-pipe.
Data from unpaired (non-colliding) bunches (points) are cleaned from noise
and parasitic collisions by requiring no primary vertex.
There is an additional requirement of at least one jet in order to assure a calorimeter activity.
In this way, an almost pure sample of beam induced background is prepared.
The arrow indicates the direction towards the centre of the LHC ring (positive x-axis).
Units correspond to the number of entries per bin.
</td><td align="right">
[[%ATTACHURLPATH%/bb_xySeg.png][<img width="300" alt="%ATTACHURLPATH%/bb_xySeg.png" src="%ATTACHURLPATH%/bb_xySeg.png"></img>]]<br>
[[%ATTACHURLPATH%/bb_xySeg.eps][eps file]]<br>
</td>
</tr>

<tr>
<td bgcolor=#eeeeee><b> LAr cluster time as a function of z position </b><br>
Cluster time plotted as a function of z position in the LAr calorimeter.
Data from unpaired (non-colliding) bunches are cleaned from noise
and parasitic collisions by requiring no primary vertex.
There is an additional requirement of at least one jet in order to assure a calorimeter activity.
In this way, an almost pure sample of beam induced background is prepared.
Furthermore, beam halo muon candidates are selected by demanding
a segment in CSC or the inner MDT end-cap with a direction parallel to the beam-pipe.
Only the clusters with E > 10 !GeV that are matched in phi and R
to such muon segments are plotted.
The two bands show the expected time for the clusters in 1 < R < 2 m
coming from beam halo muons going in the AC or CA direction.
Units correspond to the number of entries per bin.
</td><td align="right">
[[%ATTACHURLPATH%/bb_ztLar.png][<img width="300" alt="%ATTACHURLPATH%/bb_ztLar.png" src="%ATTACHURLPATH%/bb_ztLar.png"></img>]]<br>
[[%ATTACHURLPATH%/bb_ztLar.eps][eps file]]<br>
</td>
</tr>

<tr>
<td bgcolor=#eeeeee><b> Tile cluster time as a function of z position </b><br>
Cluster time plotted as a function of z position in the Tile calorimeter.
Data from unpaired (non-colliding) bunches are cleaned from noise
and parasitic collisions by requiring no primary vertex.
There is an additional requirement of at least one jet in order to assure a calorimeter activity.
In this way, an almost pure sample of beam induced background is prepared.
Furthermore, beam halo muon candidates are selected by demanding
a segment in CSC or the inner MDT end-cap with a direction parallel to the beam-pipe.
Only the clusters with E > 10 !GeV that are matched in phi and R
to such muon segments are plotted.
The two bands show the expected time for the clusters in 2 < R < 4.25 m
coming from beam halo muons going in the AC or CA direction.
Units correspond to the number of entries per bin.
</td><td align="right">
[[%ATTACHURLPATH%/bb_ztTile.png][<img width="300" alt="%ATTACHURLPATH%/bb_ztTile.png" src="%ATTACHURLPATH%/bb_ztTile.png"></img>]]<br>
[[%ATTACHURLPATH%/bb_ztTile.eps][eps file]]<br>
</td>
</tr>

<tr>
<td bgcolor=#eeeeee><b> Leading jet phi </b><br>
Phi of the leading jet in the beam background events (points)
and physics collision data (filled histogram).
Data from unpaired (non-colliding) bunches are cleaned from noise
and parasitic collisions by requiring no primary vertex.
There is an additional requirement of at least one jet in order to assure a calorimeter activity.
In this way, an almost pure sample of beam induced background is prepared.
Beam background events are compared to the physics collision events with muon triggers
where also at least one jet is required.
</td><td align="right">
[[%ATTACHURLPATH%/bb_jet1Phi.png][<img width="300" alt="%ATTACHURLPATH%/bb_jet1Phi.png" src="%ATTACHURLPATH%/bb_jet1Phi.png"></img>]]<br>
[[%ATTACHURLPATH%/bb_jet1Phi.eps][eps file]]<br>
</td>
</tr>

<tr>
<td bgcolor=#eeeeee><b> Leading jet time </b><br>
Time of the leading jet in the beam background events (points)
and physics collision data (filled histogram).
Data from unpaired (non-colliding) bunches are cleaned from noise
and parasitic collisions by requiring no primary vertex.
There is an additional requirement of at least one jet in order to assure a calorimeter activity.
In this way, an almost pure sample of beam induced background is prepared.
Beam background events are compared to the physics collision events with muon triggers
where also at least one jet is required.
</td><td align="right">
[[%ATTACHURLPATH%/bb_jet1Time.png][<img width="300" alt="%ATTACHURLPATH%/bb_jet1Time.png" src="%ATTACHURLPATH%/bb_jet1Time.png"></img>]]<br>
[[%ATTACHURLPATH%/bb_jet1Time.eps][eps file]]<br>
</td>
</tr>

<tr>
<td bgcolor=#eeeeee><b> Leading jet in the eta-phi plane </b><br>
Leading jets in the eta-phi plane in the beam background data.
Data from unpaired (non-colliding) bunches are cleaned from noise
and parasitic collisions by requiring no primary vertex.
There is an additional requirement of at least one jet in order to assure a calorimeter activity.
In this way, an almost pure sample of beam induced background is prepared.
Units correspond to the number of entries per bin.
</td><td align="right">
[[%ATTACHURLPATH%/bb_jet1EtaPhi.png][<img width="300" alt="%ATTACHURLPATH%/bb_jet1EtaPhi.png" src="%ATTACHURLPATH%/bb_jet1EtaPhi.png"></img>]]<br>
[[%ATTACHURLPATH%/bb_jet1EtaPhi.eps][eps file]]<br>
</td>
</tr>

<tr>
<td bgcolor=#eeeeee><b> Time of the leading jet as a function of eta </b><br>
Time of the leading jet as a function of eta in the beam background data.
Only the events identified by the One-sided loose method are shown.
This method requires a muon segment in CSC or the inner MTD end-cap with
a direction parallel to the beam-pipe. This segment has to be matched in phi and R
to a calorimeter cluster with E > 10 !GeV and time corresponding
to a particle going in the AC or CA direction.
The direction is reconstructed from the muon segment time and position measurement.
Units correspond to the number of entries per bin.
</td><td align="right">
[[%ATTACHURLPATH%/bb_jet1EtaTime.png][<img width="300" alt="%ATTACHURLPATH%/bb_jet1EtaTime.png" src="%ATTACHURLPATH%/bb_jet1EtaTime.png"></img>]]<br>
[[%ATTACHURLPATH%/bb_jet1EtaTime.eps][eps file]]<br>
</td>
</tr>

</table>

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   * [[%ATTACHURL%/zasymmetry_sctBarrel_Run2.eps][zasymmetry_sctBarrel_Run2.eps]]: zasymmetry_sctBarrel_Run2.eps</verbatim>

   * [[%ATTACHURL%/zasymmetry_SCTEndcaps.eps][zasymmetry_SCTEndcaps.eps]]: zasymmetry_SCTEndcaps.eps</verbatim>
Attachments
Topic attachments
I	Attachment	History	Action	Size	Date	Who	Comment
eps	BcmSpecificRatePaper_2011.eps	r1	manage	14.2 K	2011-11-01 - 17:06	LucaFiorini	2011 plot with UISO only by Fill eps
png	BcmSpecificRatePaper_2011.png	r1	manage	40.1 K	2011-11-01 - 17:05	LucaFiorini	2011 plot with UISO only by Fill
eps	SCT_Barrel_Hitoccupancy.eps	r1	manage	13.6 K	2023-02-24 - 12:12	MarziehBahmani	Run2 results for SCT
pdf	SCT_Barrel_Hitoccupancy.pdf	r1	manage	14.5 K	2023-02-24 - 12:36	MarziehBahmani
png	SCT_Barrel_Hitoccupancy.png	r1	manage	46.1 K	2023-02-24 - 12:36	MarziehBahmani
eps	SCTavaragecluster_barrel.eps	r1	manage	12.9 K	2023-02-24 - 12:12	MarziehBahmani	Run2 results for SCT
pdf	SCTavaragecluster_barrel.pdf	r1	manage	14.3 K	2023-02-24 - 12:37	MarziehBahmani
png	SCTavaragecluster_barrel.png	r1	manage	41.2 K	2023-02-24 - 12:37	MarziehBahmani
eps	bb_jet1EtaPhi.eps	r1	manage	66.1 K	2011-11-02 - 16:21	DavidSalek
png	bb_jet1EtaPhi.png	r1	manage	14.7 K	2011-11-02 - 16:18	DavidSalek
eps	bb_jet1EtaTime.eps	r1	manage	21.0 K	2011-11-02 - 16:20	DavidSalek
png	bb_jet1EtaTime.png	r1	manage	14.4 K	2011-11-02 - 16:19	DavidSalek
eps	bb_jet1Phi.eps	r1	manage	10.5 K	2011-11-02 - 16:20	DavidSalek
png	bb_jet1Phi.png	r1	manage	20.2 K	2011-11-02 - 16:19	DavidSalek
eps	bb_jet1Time.eps	r1	manage	10.9 K	2011-11-02 - 16:20	DavidSalek
png	bb_jet1Time.png	r1	manage	20.6 K	2011-11-02 - 16:19	DavidSalek
eps	bb_thetaCSC.eps	r1	manage	14.8 K	2011-11-02 - 16:21	DavidSalek
png	bb_thetaCSC.png	r1	manage	28.1 K	2011-11-02 - 14:08	DavidSalek
eps	bb_thetaMDT.eps	r1	manage	15.6 K	2011-11-02 - 16:22	DavidSalek
png	bb_thetaMDT.png	r1	manage	28.4 K	2011-11-02 - 16:19	DavidSalek
eps	bb_timeCSC.eps	r1	manage	13.0 K	2011-11-02 - 16:23	DavidSalek
png	bb_timeCSC.png	r1	manage	27.1 K	2011-11-02 - 14:16	DavidSalek
eps	bb_timeDiffAC.eps	r1	manage	11.9 K	2011-11-02 - 16:22	DavidSalek
png	bb_timeDiffAC.png	r1	manage	17.6 K	2011-11-02 - 16:17	DavidSalek
eps	bb_xySeg.eps	r1	manage	154.7 K	2011-11-02 - 16:22	DavidSalek
png	bb_xySeg.png	r1	manage	21.5 K	2011-11-02 - 16:17	DavidSalek
eps	bb_ztLar.eps	r1	manage	30.0 K	2011-11-02 - 16:22	DavidSalek
png	bb_ztLar.png	r1	manage	21.2 K	2011-11-02 - 16:18	DavidSalek
eps	bb_ztTile.eps	r1	manage	30.4 K	2011-11-02 - 16:22	DavidSalek
png	bb_ztTile.png	r1	manage	22.4 K	2011-11-02 - 16:18	DavidSalek
eps	beamhalo.eps	r1	manage	14.0 K	2011-11-02 - 17:33	MikaHuhtinen
png	beamhalo.png	r1	manage	41.9 K	2011-11-02 - 17:33	MikaHuhtinen
eps	zasymmetry_SCTEndcaps.eps	r1	manage	10.7 K	2023-02-24 - 13:16	MarziehBahmani
pdf	zasymmetry_SCTEndcaps.pdf	r2 r1	manage	13.5 K	2023-02-24 - 12:39	MarziehBahmani
png	zasymmetry_SCTEndcaps.png	r1	manage	12.5 K	2023-02-24 - 12:39	MarziehBahmani
eps	zasymmetry_SCT_Barrel_3_sec4.eps	r2 r1	manage	12.6 K	2023-02-24 - 13:07	MarziehBahmani	Run2 results for SCT
pdf	zasymmetry_SCT_Barrel_3_sec4.pdf	r2 r1	manage	15.7 K	2023-02-24 - 13:07	MarziehBahmani
png	zasymmetry_SCT_Barrel_3_sec4.png	r2 r1	manage	40.3 K	2023-02-24 - 13:09	MarziehBahmani
eps	zasymmetry_SCT_Barrel_5_sec6.eps	r1	manage	14.3 K	2023-02-24 - 12:11	MarziehBahmani	Run2 results for SCT
pdf	zasymmetry_SCT_Barrel_5_sec6.pdf	r1	manage	16.5 K	2023-02-24 - 12:38	MarziehBahmani
png	zasymmetry_SCT_Barrel_5_sec6.png	r1	manage	41.9 K	2023-02-24 - 12:38	MarziehBahmani
eps	zasymmetry_sctBarrel_Run2.eps	r1	manage	12.6 K	2023-02-24 - 13:16	MarziehBahmani
pdf	zasymmetry_sctBarrel_Run2.pdf	r1	manage	14.7 K	2023-02-24 - 12:39	MarziehBahmani
png	zasymmetry_sctBarrel_Run2.png	r1	manage	20.0 K	2023-02-24 - 12:39	MarziehBahmani
eps	zasymmetry_sct_disk1.eps	r1	manage	12.8 K	2023-02-24 - 12:08	MarziehBahmani	Run2 results for SCT
pdf	zasymmetry_sct_disk1.pdf	r1	manage	15.3 K	2023-02-24 - 12:38	MarziehBahmani
png	zasymmetry_sct_disk1.png	r1	manage	39.2 K	2023-02-24 - 12:38	MarziehBahmani
eps	zasymmetry_sct_disk8.eps	r1	manage	12.9 K	2023-02-24 - 12:09	MarziehBahmani	Run2 results for SCT
pdf	zasymmetry_sct_disk8.pdf	r1	manage	15.4 K	2023-02-24 - 12:38	MarziehBahmani
png	zasymmetry_sct_disk8.png	r1	manage	39.2 K	2023-02-24 - 12:38	MarziehBahmani
Topic revision: r17 - 2023-10-09 - HeatherGray
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