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The FNAL

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Title: The FNAL


1
The FNAL LHC Physics CenterPreparing for CMS
Physics at Fermilab  
  • DOE Annual Program Review
  • Avi Yagil

2
A Talk within a Talk
  • Inside A presentation by Sarah during the Annual
    US-CMS collaboration mtg (Apr 06, Nebraska)
  • Wrapper My comments, observations
  • Will try to keep talk short
  • Please, guide it with your questions!

3
Brief History, Status
  • Motivation - why worry now?
  • Getting started - LPC
  • First discussion
  • Why do we cluster?
  • The plan
  • Status (1 slide)

4
Why worry now? Day-One
  • Commissioning
  • Complex detectors, environment
  • Took CDF 18 months (just for RunII startup!!)
  • Period to build credibility for future physics
    results
  • Partially instrumented detector (?)
  • No pixels ? Very different tracking strategy and
    capabilities. Study now!
  • Tracking always slower to mature, big impact
  • New Energy regime
  • Some (possibly exciting) physics is accessible
    with calorimetry only. Need to work on it now.
  • Really exploration machine! No paradigm, golden
    channels
  • Must be ready and prepared for anything
  • Do not waste time (money) on 17

5
LPC Founding Fathers Mothers, Adv Brd
First Discussion on Feb 12th 2004
  • Darin Acosta (Florida)
  • Claudio Campagneri (UCSB)
  • John Conway (Rutgers)
  • Sridhara Dasu (Wisconsin)
  • Regina Demina (Rochester)
  • Greg Landsberg (Brown)
  • Christoph Paus (MIT)
  • Chris Tully (Princeton)
  • John Womersley (FNAL)
  • Lothar Bauerdick (FNAL)
  • Bob Cousins (UCLA)
  • Dan Green (FNAL)
  • Sarah Eno (Maryland)
  • Avi Yagil (FNAL)
  • Since Added
  • Max Chertok (Davis)
  • Cecilia Gerber (UIC)

Julia Thom (Cornell) Bob Hirosky (Virginia) Mo
Swartz (JHU)
Recently rotate 1/3, new chair members
A bit more from that 1st mtg
6
Why do we cluster?
  • Detector location
  • Operations Shifts, Data validation, Maintenance
  • Computing Data reconstruction, Storage,
    Simulation
  • Critical mass for complex analyses
  • Experts (mainly tracking, calor, calib, sim...)
  • Presentations Meetings
  • New students post-docs education
  • Gossip and other social activities
  • In the end, our common goal is Physics output.
  • Can remote clustering be successful?

7
Agreed on a Plan
  • Establish the LHC Physics Center (LPC), so that
    we can
  • Build local low-level software expertise and
    infrastructure
  • Learn whats available (in CMS)? How good is it?
    What should we concentrate on?
  • Enable University participation by leveraging
    initial lab effort
  • Invite and encourage sharing of CDF/D0
    collaborations efforts (specifically of post-docs
    and students)
  • Establish skeleton local algorithm groups
  • Participate in CMS activities as a community
  • gt Sent letter to Mike that started the whole
    thing.

8
Where are we now?
  • We managed to build a strong foundation
  • Most points from the plan we made where
    actually and surprisingly achieved in an amazing
    short period.
  • Our working groups completed the study of the
    available
  • Some are major contributors to current
    developments (framework, tracking, Jet, Met, code
    management,)
  • Lab support has been and still is very strong
  • LPC is one of the best places (if not the best)
    in terms of low-level SW expertise in CMS
  • Examples
  • Six active working groups
  • Workshops, Schools, mtgs (a few highlights)
  • Hosted CMS Physics week
  • J-term
  • Hosted CMS Tracker/SW joint workshop
  • Initiated and will host the first joint FNAL/CERN
    HCSS
  • Recently started analysis oriented Physics
    effort
  • Remote Operation Center (ROC)

Became (literally) a model for imitation by CERN
and others
9
The FNAL LHC Physics Center
  • Sarah Eno, U. Maryland
  • US CMS Meeting
  • Apr. 7, 2006, Nebraska

10
LPC
Founded Feb 2004
Located on the 11th floor of the FNAL high rise,
the purpose of the LPC is to ensure the US gives
the strongest possible assistance to
international CMS in software preparations for
Day 1 and to enable physics analysis from within
the U.S.
  • a critical mass (clustering) of young people
    who are actively working on software
    (reconstruction, particle identification, physics
    analysis) in a single location (11th floor of the
    high rise),
  • a resource for University-based US CMS
    collaborators a place to find expertise in their
    time zone, a place to visit with their software
    and analysis questions,
  • a brick-and-mortar location for US-based physics
    analysis, with such physical infrastructure as
    large meeting rooms, video conferencing, large
    scale computing, and a water cooler for
    informal discussions of physics.

11
2005
  • Moved into 11th floor in early 2005
  • create of ROC
  • planning of LHC_at_FNAL
  • international CMS physics week
  • 3 sessions of CMS101/ 4 sessions of software
    tutorials
  • J-Term
  • 2 week summer school (run by Dan Green)
  • over 50 summer visitors who stayed at least 2
    continguous weeks
  • Physics workshop
  • LHC the first one-two years mini workshop
  • All US CMS Meeting
  • Wine and cheese on LPC at FNAL
  • new working groups (tau, cosmic challenge/roc,
    physics)

12
Facilities
13
Resources 11th Floor
  • Meeting Rooms/Video Conferencing/Internet
  • terminals/printers/office supplies
  • secretarial and computer support
  • Coffee machines/Water cooler
  • Lockers for transient use

Currently 25 University employees permanently on
11th floor.
14
ROC
15th Sept. 05.
Kaori Maeshima, Alan Stone et al.
15
Weve got data!
(working in conjunction with the FNAL CMS Tier1
team)
16
Web Information
http//www.uscms.org/LPC/LPC.htm
17
Web
18
Computer Help
Patrick Gartung
  • system administration of the Linux PC's at the
    LPC and the ROC
  • all common login PC's and some university PC's
  • user support for
  • Windows and Linux laptops at the LPC
  • accessing the UAF resources from the LPC and
    universities
  • the video conference rooms at the LPC
  • running CMS software
  • setting up the PC's and video conference
    equipment in the ROC
  • developing software configurations for new Linux
    desktop installations

19
Inform/Educate
20
All US CMS Meeting
May 13 EDM report - Liz Sexton-Kennedy May 20
sLHC - Wesley Smith May 27 e/gamma - Yuri
Gerstein Jun 3 trigger - Sridhara Jun 10
jet/met - Rob Harris Jun 17 (cancel due to cms
week? Jun 24 (cancel due to cms annual
review?) Jul 1 The CMS Forward Pixel Project -
John Conway Jul 8 Making contact with theorist -
Steve Mrenna Jul 15 muon alignment - Marcus
Hohlmann Jul 22 LPC muon group - Eric James Jul
27 due to Dan's lecture series Aug 5 Authorship
list requirements - Dan Green Aug 12 Magnet
studies - Rich Smith Aug 19 Data bases for Cosmic
Ray test - Lee Lueking Aug 26 luminosity
preparation - Dan Marlow Sep 2 cosmic analysis in
the U.S. - Yurii Maravin Sep 9 cosmic
workshop Sep 16 ROC - Kaori Sep 23 CMS week Sep
30 Simulation Certification Project - Daniel
Elvira Oct 7 physics workshop Oct 14 (HCAL
meeting at FNAL) MET - Richard Cavanough Oct 21
Calorimetry Task Force - Jeremy Mans Oct 28 HCAL
calibration - Shuichi Kunori Nov 4 P420 Proposal
- Mike Albrow Nov 11 Nov 18 Tier 2's for me and
you - Ken Bloom
  • (almost) every Friday
  • well-attended both in person and via vrvs
  • Typical Agenda
  • News from Dan
  • News from Ian/Jon
  • Hardware News (Hadley/Maravin)
  • one topical talk

21
CMS101 Agenda
22
Tutorials Agenda
23
International CMS Physics Workshop/USCMS Meeting
24
Article on Mini-Workshop
25
Summer School Agenda
26
Summer 05
Over 50 University-based physicists visited the
LPC for at least 2 weeks this summer.
  • Summer school
  • CMS 101
  • tutorials

27
Inauguration of LPC Physics Effort -Workshop
_at_FNAL on Oct. 7, 2005
Goals
  • Get to know (communications is the name of the
    game!)
  • each other
  • who is doing what wrt Physics analysis
  • what level of support already exists at the LPC
    (computing,
  • software, algorithms, environment,)
  • Find out where one can fit in
  • Join one (or more) of the working groups
  • Allow newcomers to learn from the experience of
    those
  • already active in CMS analysis
  • Help in shaping up our future feedback, input
  • Begin to enjoy the road to the promised land

Great Success - 60 Participants at WH1W 20 VC
Connections
28
J-Term Intro to CMS at LPC
Attended by over 70 1st and 2nd year grad
students!
29
People/Working Groups
30
More than just furniture
  • Run by Avi Yagil, Sarah Eno
  • offline/edm Liz Sexton-Kennedy (FNAL), Hans
    Wenzel (FNAL)
  • tracking Kevin Burkett (FNAL), Steve Wagner
    (CO)
  • e/gamma Yuri Gershtein (FSU), Colin Jessup
    (Notre Dame)
  • muon Eric James (FNAL) , Michael Schmitt
    (Northwestern)
  • jet/met Rob Harris (FNAL), Marek Zielinski
    (Roch)
  • Tau Anna Goussiou (Notre Dame), Alexei Safonov
    (Texas AM)
  • simulation Daniel Elvira (FNAL), Harry Cheung
    (FNAL)
  • trigger Greg Landsberg (Brown) , Kaori Maeshima
    (FNAL)
  • Physics Boaz Klima (FNAL)

Colin
Eric
Steve
Michiel
Rob
Yuri
Daniel
Hans
Avi
Marek
Liz
Kevin
Anna
Heidi
Kaori
Greg
Boaz
Harry
Sarah
31
Thanks and Welcome!
Thanks!
Sasha
Martijn
Heidi
Sridhara
Welcome!
Anna
Steve
Michiel
Greg
Colin
Harry
32
Integration with CMS CPT Project for Computing,
Software, Physics Reconstruction and Selection
Frequently on 11th floor or on LPC advisory
council
Project Manager P.Sphicas
Project Office V.Innocente L.Taylor
Computing L. Bauerdick S. Belforte
Software L.Silvestris A.Yagil
EvF/DQM E. Meschi
Framework L. Sexton
Technical Program P.Elmer/S.Lacaprara
Heavy Ions B. Wyslouch
Reconstruction T. Boccali
Analysis Tools L. Lista
Integration Program S. Belforte/I. Fisk
Higgs S. Nikitenko
Calibr/alignment O. Buchmuller L. Malgeri
Operations Program L. Barone
Standard Model J. Mnich
ORCA for PTDR W. Adam
SUSY BSM L. Pape M. Spiropulu
Fast Simulation P. Janot
Simulation M. Stavrianakou Daniel Elvira
Facilities and Infrastructure N. Sinanis
Generator Tools F. Moortgat S. Slabospitsky
SW Devel Tools S. Argiro
Geometry M. Case
33
The LPC Universities
  • a postdoc who is stationed at FNAL working on
    both CMS and a Tevatron experiment can have a
    desk on the 11th floor and be near people from
    both experiments.
  • a CMS postdoc can be stationed at FNAL and
    benefit from having many people close by to
    interact with
  • a postdoc stationed at your university can come
    for a month, to get up to speed on analysis
    basics and to form personal connections that will
    help his/her later work
  • students can come for the summer to interact
    with a wide variety of experts and learn the
    basics on the CMS environment
  • Faculty can come every other week to keep their
    connections with the experimental community .
  • Faculty can come for a day for help with a
    particularly knotty software or analysis problem

Participation in the groups will both help them
do physics and allow them to serve the US and
International CMS
34
US University Involvement
Simulation FNAL, FSU, Kansas State, Kansas,
Louisiana Tech/Calumet, Maryland, Northwestern,
Notre Dame, Rutgers, UIC, SUNY Buffalo, Nanjin,
Ciemat, Tata, Puerto Rico, Mississippi,
Colorado Jet/Met FNAL, Rochester, MD, Rutgers,
Boston, Cal Tech, Florida, Rockefeller,
Princeton, Texas Tech, Iowa, Mississippi,
Minnesota, Santa Barbara, Northwestern Muon
FNAL, Carnegie Mellon, Florida, Florida Tech,
Purdue, Nebraska, Northwestern e/gamma FNAL,
Northwestern, FSU, Minnesota, MD, Brown, Notre
Dame, San Diego, Cal Tech, Cornell, Virginia,
Kansas State Tracking FNAL, Colorado, Cornell,
Nebraska, UC Davis, UCSB, UC Riverside, Kansas,
Calumet Trigger Wisconsin, Florida,
Northwestern, FNAL, Vanderbilt, Texas AM, Brown,
Maryland, LLNL, UIC Offline/edm FNAL, Cornell,
CalTech Physics all
35
11th Floor
25 permanent University employees on 11th
floor
Brown , Buffalo, CMU, Kansas State, MD, MN,
Northeastern, Puerto Rico, Rochester,
Rockefeller, Rutgers, Texas AM, UC Davis , UIC,
FSU
36
Plans for Coming Year
  • Commissioning of ROC / Cosmic slice test
  • Expansion onto 10th floor
  • Full house this summer
  • CMS101/Tutorials in June and September
  • LHC_at_FNAL
  • Strengthening of working groups, especially the
    brand-new physics group
  • Development of realistic run plan for early
    data taking
  • Working with detector groups

37
LPC and MTCC
  • MTCC Magnet Test Cosmic Challenge
  • Start of test Detector close, June 6, 2006
  • Goals test and train magnet, integrate
    detectors.
  • Date has slipped. Summer visitors can now
    participate.
  • Data will be brought to FNAL for analysis.
  • Some (e.g. HCAL brightening data) will be kept
    and archived at Fnal.)
  • Also some real time monitoring will be done.
  • Specific plan for LPC analysis varies by group
    and is in formulation
  • (ECAL, EMU, HCAL, Tracker, Trigger)
  • Many periods without data taking, no shifts
    currently envisioned, brief daily meeting instead.

38
LPC and Test Beam
  • Test Beam planned for late summer.
  • ECAL, HCAL,
  • Data will be brought to FNAL (as was done for
    previous test beams)
  • ECAL and HCAL have LPC based analysis plans for
    this data.
  • Shift(s) at ROC and real time data monitoring
    planned
  • Shifts likely not 24/7
  • Nick
  • Yurii

39
This Summer
(Brown, Carnegie Mellon, Colorado, Cornell, FIT,
FSU, KS, MD, Mississippi, Northwestern, Ohio
State, Puerto Rico, Rochester, Rockefeller,
Rutgers, Buffalo, Texas AM, Florida, UC Davis,
UC Riverside, UIC, Virginia)
40
10th Floor
WH10 Sec-LPC
???
41
LHC_at_FNAL Location Layout
42
LHC_at_FNAL Current Status
  • LHC_at_FNAL layout endorsed by Fermilab Director
  • Conceptual Design Report completed and reviewed
  • Project Execution Plan written
  • Project Managers
  • Elvin Harms (FNAL-AD) construction
  • Erik Gottschalk (FNAL-PPD) consoles
  • Weekly meetings to prepare construction drawings
  • Presentation to US-CMS Collaboration (early
    April)
  • Presentation to LHC Accelerator Research Program
    (LARP) at its collaboration meeting (late April)
  • Construction complete by end of FY06

43
Conclusions
Hope to see you on the 11th floor!
44
Impact of LPC
  • Although not formally commissioned until early
    2005, LPC have already had a big impact on CMS
  • Review of software framework led to overhaul of
    CMS software from the bottoms up (new framework,
    event data model).
  • One of the two tracking packages CMS uses, has
    been developed and is supported by the LPC
    tracking group.
  • LPC Jet/Met group leads the implementation of Jet
    and Met reconstruction software in the new
    framework.
  • ROC is setting an example for remote
    participation/access (CMS is planning the CCAR).
  • To date, best place to pick up and get started on
    CMS.

45
Interaction terms - Key to success
  • The three legs
  • US-CMS SC
  • FNAL CD/PPD
  • LPC
  • There have been an early understanding of the
    potential benefits from coordination
  • Joint study groups (CDF/D0, CD experts, US-CMS
    colleagues)
  • Started with tracking --gt code distribution,
    framework
  • Utilizing CD consultancy time, huge impact!
    (critical during early stage)
  • Consolidating US-CMS SC efforts around few, well
    chosen projects
  • Instead of shipping individual effort across the
    Atlantic
  • Maintain constant project effort level (see Liz
    talk)
  • Push overall effort level. Enable physicists
    contributions, broader participation.
  • Tremendous cross-fertilization
  • Impact rather obvious

46
Summary
  • 2005 concentration on the physics-enabling
    environment and reconstruction tools. Aspects
    ranging from muon identification to trigger
    tables to jet calibration.
  • 2006 moving closer to physics analyses, via the
    path of understanding the detectors during the
    cosmic challenge and test beam. Starting to plan
    for commissioning, Day-1 Physics.
  • 2007
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