LIGO-G030394-00-Z Detector Characterization Summary - 2003.8.21K. Riles - University of Michigan 1 Summary of the Detector Characterization Sessions Keith.

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Presentation transcript:

LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 1 Summary of the Detector Characterization Sessions Keith Riles (University of Michigan) Daniel Sigg (LIGO–LHO) LIGO Scientific Collaboration Meeting Hannover University August 21, 2003

LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 2 S2 Analysis S2 investigation teams very active / productive  Many reports at this meeting Much improved communication with search groups  Quite effective glitch collaboration with burst / inspiral groups Data quality repository seems to be serving its purpose In general, things seem to be working better than for S1

LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 3 S2 Analysis BUT… Investigations / reports taking longer than hoped Delays tolerable only because search groups held up by finalization of S1 analyses Can’t assume this pattern will hold for S3 Need to be quicker for S3 (more later)

LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 4 Looking ahead to S3 - Schedule Mini-E-runs (single-site 6-hour evening runs): Sat Sept 13 at Hanford and Sat Sept 20 at Livingston Hardware/software freeze  ~Oct 1 – Start routine running of DMT monitors  Figures of merit once again prominently displayed Maxi-E-run: (1-week final shakedown at both sites): Fri Oct 17 (evening) – Fri Oct 24 (early morning) Tinkering to fix / improve hardware / software Fri Oct 24 – Thur Oct 30 Science Run S3 Fri Oct 31 – Mon Jan 5 (+ 1 month?)

LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 5 Looking ahead to S3 - Scimons Plan for S3 same as for S2: 24/7 shift staffing at both sites – 1 expert Three 8-hour shifts / day Training slots available for new persons But should have larger pool of experts now »More equitable burden on groups Allocation based once again on FTE counts »Please send updated FTE counts to Irena Will solicit request for group constraints / preferences with prompt response requested »Will accommodate requests within reason and where possible

LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 6 Looking ahead to S3 – Feedback Devoting one week to maxi-E-run to shake down software and to evaluate detector performance Cannot use “tinkering week” well without that evaluation: DMT diagnostics S3 investigations Search group quick-looks Be Prepared!

LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 7 One more issue- DMT evolution As reported Tuesday, new ITR proposal approved with funding for 2.25 FTE’s to assist in DMT infrastructure development ( PSU, MIT, UWM ) We are now discussing how best to make use of this new resource, but tentative strawman plan: Support linux porting of DMT with auto-installation tools Support “gridification”, i.e., automated remote submission of jobs and i/o handling at tier 2 centers (good progress PSU) Support small number of linux nodes at each observatory with immediate access to recent full data

LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 8 One more issue- DMT evolution More input requested: What else would you like to see in gridified DMT system? Examples: »Full support of GDS tree (DTT & other existing tools) »New graphical tools »Other new infrastructure that could help at the sites? »What do search groups want?

LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 9 Presentations in DC Sessions Can’t do justice to all of these in this brief summary Agenda Lots of interesting talks!