TWiki
>
ILCTPC Web
>
Analysis
>
JamboreeRecommendations
(2007-01-26,
PeterWienemann
)
(raw view)
E
dit
A
ttach
P
DF
---++ Guidelines for Result Comparisons The information given below is taken from the conclusions of the [[http://ilcagenda.linearcollider.org/conferenceDisplay.py?confId=desya0591][first ILC Analysis Jamboree]], held at DESY on February 13-15, 2006. In order to avoid comparing apples and oranges, a couple of rules should be obeyed: ---+++++ Setup and Data Set Provide the following information: * pad pitch and layout * gas used (preferably P5 as a reference) * magnetic field * gain * noise level (for instance r.m.s. in ADC counts) * detector acceptance (phi and theta distribution, intercept x_0, z_0) * charge deposition of a row (a hit) to show the amount of saturation and noise ---+++++ Selection To avoid biasing the results by selecting very specific tracks, the selection cuts should be reduced to a minimum and justified. However fiducial cuts to ensure a good data quality are recommended if needed. Effect of cutting or keeping saturated hits has to be assessed. An estimate of the selection efficiency has to be given. ---+++++ Resolution Show residual distributions (for instance at a given z) to allow estimating the tails and the shape. To define the resolution, use * RMS of residual distibution, after cutting outliers, not less than 5*RMS cut (iterative process) * the geometric mean of fits with and without the test row (the preferred method) to avoid a bias from the track extrapolation error. Also simple methods like the triplet method or the extrapolation between adjacent rows are correct, provided the right statistical factor is used. * for cosmics, a phi cut at +-0.1 rad (recommended), for sake of comparison without cutting too much statistics. However, depending on trigger and aspect ratio, one can have to change this. The best, if statistics allows, is to show phi dependence of the resolution. The same is true for theta, here a cut at 0.2 rad is indicated. Provide the following information: * fraction of 1-pad, 2-pad, 3-pad hits (especially if one of these categories is rejected) * fit of the resolution with a sigma0 and a Neff for large enough drift distance that a parabolic dependence can be fitted: sigma = sqrt(sigma0**2+(CD**2/Neff)*z) * bias plots (residuals vs position in the pad) * probability of the chi^2 (if one uses such a fit) or pull distribution -- Main.PeterWienemann - 26 Jan 2007
E
dit
|
A
ttach
|
Watch
|
P
rint version
|
H
istory
: r1
|
B
acklinks
|
V
iew topic
|
WYSIWYG
|
M
ore topic actions
Topic revision: r1 - 2007-01-26
-
PeterWienemann
Log In
ILCTPC
ILCTPC Web
Create New Topic
Index
Search
Changes
Notifications
Statistics
Preferences
Public webs
Public webs
ABATBEA
ACPP
ADCgroup
AEGIS
AfricaMap
AgileInfrastructure
ALICE
AliceEbyE
AliceSPD
AliceSSD
AliceTOF
AliFemto
ALPHA
ArdaGrid
ASACUSA
AthenaFCalTBAna
Atlas
AtlasLBNL
AXIALPET
CAE
CALICE
CDS
CENF
CERNSearch
CLIC
Cloud
CloudServices
CMS
Controls
CTA
CvmFS
DB
DefaultWeb
DESgroup
DPHEP
DM-LHC
DSSGroup
EGEE
EgeePtf
ELFms
EMI
ETICS
FIOgroup
FlukaTeam
Frontier
Gaudi
GeneratorServices
GuidesInfo
HardwareLabs
HCC
HEPIX
ILCBDSColl
ILCTPC
IMWG
Inspire
IPv6
IT
ItCommTeam
ITCoord
ITdeptTechForum
ITDRP
ITGT
ITSDC
LAr
LCG
LCGAAWorkbook
Leade
LHCAccess
LHCAtHome
LHCb
LHCgas
LHCONE
LHCOPN
LinuxSupport
Main
Medipix
Messaging
MPGD
NA49
NA61
NA62
NTOF
Openlab
PDBService
Persistency
PESgroup
Plugins
PSAccess
PSBUpgrade
R2Eproject
RCTF
RD42
RFCond12
RFLowLevel
ROXIE
Sandbox
SocialActivities
SPI
SRMDev
SSM
Student
SuperComputing
Support
SwfCatalogue
TMVA
TOTEM
TWiki
UNOSAT
Virtualization
VOBox
WITCH
XTCA
Cern Search
TWiki Search
Google Search
ILCTPC
All webs
Copyright &© 2008-2021 by the contributing authors. All material on this collaboration platform is the property of the contributing authors.
or Ideas, requests, problems regarding TWiki? use
Discourse
or
Send feedback