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Data Challenge I Shameless Advertising for the DC1 Closeout Meeting

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Title: Data Challenge I Shameless Advertising for the DC1 Closeout Meeting


1
Data Challenge IShameless Advertising for
theDC1 Closeout Meeting
  • Tracy UsherGLAST All-Hands MeetingFebruary 11,
    2004

2
Purposes of the Data Challenges(Steve Ritz)
  • End-to-end testing of analysis software.
  • Familiarize team with data content, formats,
    tools and realistic details of analysis issues
    (both instrumental and astrophysical).
  • If needed, develop additional methods for
    analyzing LAT data, encouraging alternatives that
    fit within the existing framework.
  • Provide feedback to the SAS group on what works
    and what is missing from the data formats and
    tools.
  • Uncover systematic effects in reconstruction and
    analysis.

Support readiness by launch time to do all
first-year science.
See Richard Dubois January All-Hands Talk for
details
3
Data Challenge Plans
See Richard Dubois January All-Hands Talk for
details
4
Goal for Data Challenge IData for Analyses
  • Original Goal One days input to the onboard
    filter
  • Including background 400 Million Events
  • Backgrounds not (yet) necessary
  • Replace real backgrounds, cuts to approximate
    effect
  • Produced one day all-sky survey. Generated E gt 20
    MeV

Egt100 MeV with some other cuts for illustration
Courtesy Julie McEnery
5
DC1 Extra!Additional 5 Days Data
660k gs pass cutsCourtesy Seth Digel
6
Goals for Data Challenge IThe Desired
Results(Steve Ritz)
  • A minimum set of plots and tables, including 
  • Table 1 Found sources ranked by flux (Egt100
    MeV).
  • The table will contain the following columns
  • Reconstruction location and error circle
  • Flux (Egt100 MeV) and error
  • Significance
  • 3EG identification (yes/no) NOTE Don't assume
    DC1 sky is THE 3EG Catalog!
  • Extra Credit
  • Include flux below 100 MeV
  • Spectral indices of the brightest sources
  • Comparison of 3EG position and flux
    characteristics with GLAST analysis 
  • Figure 1 LogN-Logs plot of Table 1 
  • Table 2 List of transients detected, columns
    are
  • location and error circle
  • flux (E gt100 MeV) and error
  • significance
  • duration 
  • Figure 2 Light Curve
  • Extra Credit Figure 2a spectra 

7
Data Challenge I Schedule
  • Concept
  • Spring 2003
  • Organizing the Science Analysis Software Troops
  • July 2003 Ground Software Workshop
  • http//www-glast.slac.stanford.edu/software/Worksh
    ops/July03Workshop/coverpage.htm
  • Data Challenge I Kickoff
  • September 2003
  • Followed the Rome Collaboration Meeting
  • Getting the Users Involved
  • December 2003 DC1 Workshop
  • http//www-glast.slac.stanford.edu/software/Worksh
    ops/Dec03DC1Workshop/coverpage.htm
  • 50 attendees!
  • Closeout meeting
  • February 12-13
  • So far 50 people have indicated they are coming!

8
http//www-glast.slac.stanford.edu/software/DataCh
allenges/DC1/DC1_StatusAndInfo.htm
  • Documentation
  • Users Guide
  • Data Description
  • Likelihood Tutorial

DC-1 Discussion List
Analysis Codeand data download ftp site
Wiki page forsharing results!
9
http//www-glast.stanford.edu/cgi-prot/wiki?DataCh
allenge1
10
Jim Chiang A cursory study of the Galactic
Centerhttp//www.slac.stanford.edu/jchiang/GC_a
nalysis/main.html
11
Sean Robinson Some Results on my Wavelet
Methodhttp//d0.phys.washington.edu/srobinsn/m
emo/DC1AnalysisPerformanceJan04.htm
12
DC-1 Closeout Meeting
  • Starts Tomorrow!
  • All day Thursday
  • Half day Friday
  • Thursday Agenda
  • 15 Analysis Talks!
  • Monte Carlo Truth unveiled after talks
  • User feedback session to work on improving tools
  • For more Information go to the DC1 Closeout
    Meeting web page located at http//www-glast.sla
    c.stanford.edu/software/Workshops/Feb04DC1CloseOut
    /coverpage.htm

13
DC-1 Closeout Meeting
  • Friday Agenda
  • Update on Filter and Background Rejection
  • Recap of SAS upgrades for DC-1
  • Lessons learned, immediate plans and where to go
    next

14
DC-1 Closeout Meeting
  • This weeks meeting represents the culmination of
    a nearly 9 month project to tie together the
    various pieces of Science Analysis Software
  • Simulation reconstruction
  • Science Tools
  • Support software
  • Documentation
  • Etc.
  • For most it is the first time using the Science
    Tools to look at GLAST data
  • Long list of short analysis talks on various
    topics
  • Its not too late to sign up!
  • Registration starts tomorrow, 830 am in the SLAC
    Orange Room
  • See http//www-glast.slac.stanford.edu/software/W
    orkshops/Feb04DC1CloseOut/coverpage.htm
  • Come to the meeting!!

15
Riccardo Rando A Few Examples of the Likelihood
Tool http//sirad.pd.infn.it/glast/ground_sw/ri
ckObs.html
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