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Overview of ATLAS Distributed Analysis
Nurcan Ozturk
University of Texas at Arlington
Grid User Training for Local Community
TUBITAK ULAKBIM, Ankara, Turkey
April 5 - 9, 2010
Outline
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User’s Work-flow for Data Analysis
ATLAS Distributed Data Analysis System
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What Type of Data You Can Run On
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What Type of Jobs You Can Run
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How to Find Your Input Data
 AMI
 dq2 end-user tools
 ELSSI - Event Level Selection Service Interface
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Tips for Submitting Your Jobs
 How To Check Status of ATLAS Releases
 How to Check Status of Installation of Releases at Sites

Tips for Retrieving Your Outputs

Tips of Debugging Failures

User Support

Pathena Example on 7 TeV Collision Data
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User’s Work-flow for Data Analysis
Setup the analysis code
Locate the data
Setup the analysis job
Submit to the Grid
Retrieve the results
Analyze the results
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ATLAS Distributed Data Analysis System
3-layers:
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User
interface
Gateways
to resources
Execution
infrastructure
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What Type of Data You Can Run On
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RAW: raw data from DAQ system
ESD – Event Selection Data: output of reconstruction of RAW data
AOD – Analysis Object Data: condensed version of ESD
D1PD – Primary Derived Physics Data: ESD or AOD with:
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certain event removed (skimming)
some data objects within an event removed (thinning)
certain data members within object removed (slimming)
Commissioning DPD and Performance DPD (made from ESD’s)
Physics DPD (made from AOD’s)
DnPD, n-th Derived Physics Data (D2PD, D3PD): Specific format defined by
physics/performance groups or users
TAG: event tags which are event thumbnails with pointers to the full event in the AOD –
fast access to specific events (file-based or database-based)
Monte Carlo data
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EVNT – Event generator data: output of event generation
HITS – output of detector simulation (uses EVNT as input)
RDO – Raw Data Object: output of digitization (uses HITS as input) – MC equivalent of raw data
AOD and DPD
All of the above. However RAW/HITS/RDO are on tape, you need to request
for DDM replication to disk storage.
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What Type of Jobs You Can Run
 Athena jobs with official production transformations:
 Event generation, Simulation, Pileup, Digitization, Reconstruction, Merge
 General jobs (non-Athena type analysis):
 ROOT(CINT, C++, pyRoot)
 ARA (AthenaRootAccess)
 Python, user's executable, shell script, etc.
 Jobs with multiple-input streams (e.g. reco trf)
 Cavern, Minimumbias, BeamHalo , BeamGas input
 TAG selection jobs
 Jobs with nightly builds
 Jobs with arbitrary DBRelease
 Database release contains Conditions, Geometry and Trigger data
 More info about DBReleases is in backup slides
 etc.
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How to Find Your Input Data
 AMI
 dq2 end-user tools
 ELSSI (Event Level Selection Service Interface)
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What is AMI
 ATLAS Metadata Interface.
 A generic cataloging framework:
 Dataset discovery tool
 Tag Collector tool (release management tool)
 Where does AMI get its data:
 From real data : DAQ data from the Tier 0
 From Monte Carlo and reprocessing
 Pulled from the Task Request Database : Tasks, dataset names, Monte Carlo
and reprocessing config tags
 Pulled from the Production Database : Finished tasks – files and metadata
 From physicists
 Monte Carlo input files needed for event generation
 Monte Carlo Dataset number info, physics group owner,…
 Corrected cross sections and comments.
 DPD tags
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AMI Portal Page - http://ami.in2p3.fr
There is also a read-only server at CERN: http://atlas-ami.cern.ch
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7 TeV Datasets
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AMI Tutorial Page
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AMI Fast Tutorial Page
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Simple Search in AMI –
search by name
type here to
search for
latest 7 TeV
collision
dataset:
data10_7TeV%physics%MinBias%AOD%
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Simple Search in AMI –
various useful links
Group
by
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Apply
filter
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Simple Search in AMI –
DQ2 link
By clicking on the DQ2 link:
Use always merge datasets ending with /
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Simple Search in AMI –
PANDA link
By clicking on the PANDA link:
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Simple Search in AMI interpretation of tags (1)
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Simple Search in AMI –
Interpretation of tags (2)
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Simple Search in AMI –
Run Summary
By clicking on the Run_Summary link:
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Simple Search in AMI –
Run Queries
By clicking on the Run_Query link:
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dq2 End-User Tools (1)
 User interaction with DDM system:
 via dq2 end-user tools: querying, retrieving, creating datasets
 requesting dataset replication, dataset deletion, etc.
 How to set up (on lxplus):
 source /afs/cern.ch/atlas/offline/external/GRID/ddm/DQ2Clients/setup.sh
 voms-proxy-init --voms atlas
 More info on setup at:
 https://twiki.cern.ch/twiki/bin/view/Atlas/RegularComputingTutorial#Getting_
ready_to_use_the_Grid
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dq2 End-User Tools (2)
 How to use:
 List available MInBias datasets in DDM system (same search as in AMI) :
 dq2-ls 'data10_7TeV*physics*MinBias*‘
 Search for merged AOD’s in container datasets:
 dq2-ls 'data10_7TeV*physics*MinBias*merge*AOD*‘
 Find location of container datasets (groups of datasets, ending with a '/' ):
 dq2-list-dataset-replicas-container
data10_7TeV.00152489.physics_MinBias.merge.AOD.f241_p115/
 List files in container dataset:
 dq2-ls –f data10_7TeV.00152489.physics_MinBias.merge.AOD.f241_p115/
 Copy one file locally:
 dq2-get -n 1 data10_7TeV.00152489.physics_MinBias.merge.AOD.f241_p115/
 More info at:
 https://twiki.cern.ch/twiki/bin/view/Atlas/DQ2ClientsHowTo
 https://twiki.cern.ch/twiki/bin/view/Atlas/DQ2Tutorial
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DQ2ClientsHowTo
https://twiki.cern.ch/twiki/bin/view/Atlas/DQ2ClientsHowTo
Extensive
info here
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DQ2Tutorial
https://twiki.cern.ch/twiki/bin/view/Atlas/DQ2Tutorial
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ELSSI –
Event Level Selection Service Interface
https://voatlas18.cern.ch/tagservices/index.htm
Goal: Retrieve the TAG file from TAG
database
• Define a query to select runs, streams,
data quality, trigger chains,…
•.Review the query
• Execute the query and retrieve the TAG file
(a root file) to be used in Athena job
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Tips for Submitting Your Jobs
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Always test your job locally before submitting to the Grid
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Use the latest version of pathena/Ganga
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Submit your jobs on container datasets (merged)
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If your dataset is on tape, you need to request for data replication to a disk storage
first
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Do not specify any site name in your job submission, pathena/Ganga will choose the
best site available
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If you are using a new release that is not meant be used for user analysis, e.g.
cosmic data, Tier0 reconstruction, then it’ll not be available at all sites. In general you
can check release and installation status at:
 http://atlas-computing.web.cern.ch/atlas-computing/projects/releases/status/
 https://atlas-install.roma1.infn.it/atlas_install/
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How To Check Status of ATLAS Releases
http://atlas-computing.web.cern.ch/atlas-computing/projects/releases/status/
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How to Check Status of Installation of
Releases at Sites (1)
https://atlas-install.roma1.infn.it/atlas_install/
Choose here 15.6.8.2
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How to Check Status of Installation of
Releases at Sites (2)
https://atlas-install.roma1.infn.it/atlas_install/list.php?rel=15.6.8.2
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Tips for Retrieving Your Outputs
 If everything went fine, you need to retrieve your outputs from the Grid
 Where and how you will store your output datasets:
 request a data replication: your output files will stay as a dataset on Grid.
 You need to freeze your dataset before requesting for replication
 download onto your local disk using dq2-get: by default, user datasets are
created on _SCRATCHDISK at the site where the jobs run. All the datasets on
_SCRATCHDISK are to be deleted after a certain period (~ 30days). If you
see a possibility to use them on Grid, you should think about replication.
 No more than 30-40GB/day can be copied by dq2-get
Details at:
https://twiki.cern.ch/twiki/bin/view/Atlas/DQ2ClientsHowTo#AfterCreatingDataset
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Tips of Debugging Failures
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Try to understand if the error is job related or site related
 Job log files tell most of the time
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If the site went down during your jobs being executed, you can check its status
from the ATLAS Computer Operations Logbook:
 https://prod-grid-logger.cern.ch/elog/ATLAS+Computer+Operations+Logbook/
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If input files are corrupted at given site you can exclude the site (till they are
recopied) and notify DAST (Distributed Analysis Support Team)
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Look at the FAQ (Frequently Asked Questions) section of the pathena/Ganga
twiki pages for most common problems and their solutions:
 https://twiki.cern.ch/twiki/bin/view/Atlas/PandaAthena#FAQ
 https://twiki.cern.ch/twiki/bin/view/Atlas/DAGangaFAQ
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If you can not find your problem listed there, do a search in the archive of the
distributed-analysis-help forum in e-groups:
 https://groups.cern.ch/group/hn-atlas-dist-analysis-help/default.aspx
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If you still need help, send a message to the e-groups, DAST and other users
will help you: [email protected]
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Does your job require conditions database
access?
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If you are running at CERN or at Tier1’s, you may have not even noticed it. They provide
direct access to Oracle databases. You may have seen possible some overload problems
(errors in job logs).
What is stored in Oracle databases:
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LAr calibrations and InDet alignments are too large to be stored effectively in Oracle; they
are stored as POOL files and replicated to all Tier1’s (soon to Tier2’s)
If your job runs at Tier2/Tier3’s, remote access to Oracle databases is possible
Solution for users: provide the conditions DB releases together with the job:
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DB release is an extraction of the needed constants into a tar file that is copied to the worker node
and accessed locally. Avaiable as a dataset in DDM system.
--dbReleases NameofDataset (in pathena/Ganga)
Now in place: have user jobs to access Oracle database through FroNtier/Squid caches
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The geometry and most of the conditions data
Jobs can run anywhere w/o configuration changes
Solves latency problems with jobs running at Tier2/Tier3’s
More info about databases at:
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https://twiki.cern.ch/twiki/bin/view/Atlas/AtlasDBRelease
https://twiki.cern.ch/twiki/bin/view/Atlas/AthenaDBAccess
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ATLAS Computer Operations Logbook –
site/service problems reported
https://prod-grid-logger.cern.ch/elog/ATLAS+Computer+Operations+Logbook/
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pathena FAQ
https://twiki.cern.ch/twiki/bin/view/Atlas/PandaAthena#FAQ
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Ganga FAQ
https://twiki.cern.ch/twiki/bin/view/Atlas/DAGangaFAQ
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User Support (1)
https://twiki.cern.ch/twiki/bin/view/Atlas/AtlasDAST
DAST members
EU time zone
NA time zone
-----------------------------------------------------------------------Daniel van der Ster
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Mark Slater
Alden Stradling
Hurng-Chun Lee
Sergey Panitkin
Bjorn Samset
Kamile Yagci
Christian Kummer
Bill Edson
Maria Shiyakova
Wensheng Deng
Jaroslava Schovancova
Manuj Jha
Karl Harrison
Elena Oliver Garcia
-----------------------------------------------------------------------
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User Support (2)
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DAST started in September 2008 for a combined support of pathena and
Ganga users
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First point of contact for distributed analysis questions
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All kinds of problems are discussed, not just pathena/Ganga related ones
 Analysis tools related problems
 DDM related problems
 And athena related problems
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15 hours coverage with 2 people on shift (one in NA, one in EU time zones).
Plan is to have 2 people in each time zone.
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DAST helps directly by solving the problem or escalating to relevant experts
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More shifters and more user2user support needed
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Shift work counts to OTSMOU credit (Category-2 shifts currently)
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User feedback is extremely useful to debug the distributed analysis tools and
explore the features pathena/Ganga have to offer. So feel free to write to this
forum
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Pathena Example on 7 TeV Collision Data
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Everyone needs to complete this tutorial:
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Setup CMT and athena as explained above. You can use the latest release (production cache):
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athena SUSYD3PDMaker_topOptions.py
Setup pathena on lxplus, or install yourself as explained in pathena wiki page:
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dq2-get -n 1 data10_7TeV.00152489.physics_MinBias.merge.AOD.f241_p115/
Configure the job option file and run athena locally as explained in the SUSYD3PDMaker wiki page:
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Example: SUSYD3PDMaker package
https://twiki.cern.ch/twiki/bin/view/AtlasProtected/SUSYD3PDMaker
Get one file locally to test that athena runs fine:
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source cmthome/setup.sh -tag=15.6.8.2,AtlasProduction,setup,32
Use a ntuple (D3PD) making package to run on AOD’s:
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https://twiki.cern.ch/twiki/bin/view/Atlas/RegularComputingTutorial
source /afs/cern.ch/atlas/offline/external/GRID/DA/panda-client/latest/etc/panda/panda_setup.sh
https://twiki.cern.ch/twiki/bin/view/Atlas/DAonPanda
Submit your job to Grid with pathena:
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pathena –inDS data10_7TeV.00152489.physics_MinBias.merge.AOD.f241_p115/
--outDS user10.NurcanOzturk.trgrid.test SUSYD3PDMaker_topOptions.py
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Monitor your job on Panda monitor or using pbook (bookkeeping tool for pathena). Once your job is
completed, get your output (root files and log files) to your local machine:
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dq2-get user10.NurcanOzturk.trgrid.test
Open Root and plot some histograms to see how the real data looks like
Use analysis codes (D3PD readers) to do more detailed analysis on ntuples. Codes can be based C++
(example in SUSYD3PDMaker wiki page), python (for instance SPyRoot), etc.
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