LIGO-G010065-00-Z Detector Characterization Software Tools - 2001.3.14K. Riles - University of Michigan 1 Detector Characterization Software Tools Keith.

Slides:



Advertisements
Similar presentations
GWDAW-8 (December 17-20, 2003, Milwaukee, Wisconsin, USA) Search for burst gravitational waves with TAMA data Masaki Ando Department of Physics, University.
Advertisements

Patrick Krejcik LCLS April 16-17, 2007 Breakout Session: Controls Controls Commissioning Experience.
LIGO Reduced Data Sets E7 standard reduced data set RDS generation for future runs decimation examples LIGO-G Z Isabel Leonor (w/ Robert Schofield)
NSF : Nov. 10, LIGO End to End simulation overview  Time domain simulation written in C++  Like MATLAB with Interferometer toolbox  Major physics.
LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 1 Summary of Detector Characterization Sessions Keith.
ALLEGRO G Z LSC, Livingston 23 March, Calibration for the ALLEGRO resonant detector -- S2 and S4 Martin McHugh, Loyola University New Orleans.
LIGO-G Z NSF Review LIGO Scientific Collaboration - University of Michigan 1 The LSC Role in Detector Characterization Keith Riles.
Burst noise investigation for cryogenic GW detector TITECH NAOJ Daisuke TATSUMI 2nd Symposium ‐ New Development in Astrophysics through Multi-messenger.
LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 1 Summary of Detector Characterization Activities Keith.
LIGO-G Z NSF Review LIGO Scientific Collaboration - University of Michigan 1 LSC Participation in Initial LIGO Detector Characterization.
LIGO-G DM. Landry – Amaldi5 July 9, 2003 Laser Interferometer Gravitational Wave Observatory Monitoring LIGO Data During the S2 Science Run Michael.
Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut) Institut für Atom- und Molekülphysik Detector Characterization of GEO 600 during.
LIGO-G Z Detector characterization for LIGO burst searches Shourov K. Chatterji for the LIGO Scientific Collaboration 10 th Gravitational Wave.
1/25 Current results and future scenarios for gravitational wave’s stochastic background G. Cella – INFN sez. Pisa.
S4/S5 Calibration The Calibration team G Z.
June 27, 2002 EK 1 Data Analysis Overview Erik Katsavounidis LIGO-MIT PAC12 – June 27, 2002 LIGO-G Z.
LIGO-G Z Detector Characterization NeedsK. Riles - University of Michigan 1 Detector Characterization Needs Keith Riles (University of Michigan)
LIGO-G Z Detector Characterization SummaryK. Riles - University of Michigan 1 Summary of Detector Characterization Sessions Keith Riles (University.
LIGO-G Z Peter Shawhan, for the LIGO Scientific Collaboration APS Meeting April 25, 2006 Search for Gravitational Wave Bursts in Data from the.
Displacement calibration techniques for the LIGO detectors Evan Goetz (University of Michigan)‏ for the LIGO Scientific Collaboration April 2008 APS meeting.
Novemebr 5, 2006LSC meeting1 Virgo Update Prospects on detector performance and running schedules B. Mours.
Squeezed light and GEO600 Simon Chelkowski LSC Meeting, Hannover.
LIGO Z LIGO Scientific Collaboration -- UWM 1 LSC Data Analysis Alan G. Wiseman (LSC Software Coordinator) LIGO Scientific Collaboration.
Glitch Group S5 Activities Laura Cadonati for the Glitch Working Group LSC meeting, Hanford March 21, 2006 G Z.
LIGO-G Z Detchar Introduction (8/16/06)K. Riles - University of Michigan 1 StrainBandsMon and SixtyHertzMon Keith Riles (University of Michigan)
LIGO-G D Global Diagnostics and Detector Characterization 9 th Marcel Grossmann Meeting Daniel Sigg, LIGO Hanford Observatory.
G R LSC UL 13 Aug 011 Detector Characterization; Triggers, code infrastructure; Followup Analysis for the UL groups Nelson Christensen, Szabi.
Status of the Advanced LIGO PSL development LSC Virgo meeting, Caltech, March 2008 LIGO G Z Benno Willke for the PSL team.
LIGO-G Z 3/15/01Penn State1 The datacondAPI Sam Finn, for the datacondAPI Team: W. Anderson, K. Blackburn, P. Charlton, P. Ehrens, A. Gonzalez,
LIGO- G Z August 16, 2006August 2006 LSC Meeting - DetChar 1 Spectral Line Working Group Report Keith Thorne, Chair.
LIGO- G D Burst Search Report Stan Whitcomb LIGO Caltech LSC Meeting LIGO1 Plenary Session 18 August 2003 Hannover.
LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 1 Status Report on CW Discriminator Work Keith.
LSC Meeting, 19 March 2003 Shawhan, Leonor, MarkaLIGO-G D Introduction to Hardware Signal Injections Peter Shawhan, Isabel Leonor, Szabi Márka.
Nov 3, 2008 Detection System for AdV 1/8 Detection (DET) Subsystem for AdV  Main tasks and requirements for the subsystem  DC readout  Design for: the.
LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 1 Summary of Detector Characterization Sessions Keith.
LSC Meeting: 3/14/01Inspiral Upper Limit - Detector Characterization 1 Inspiral Upper Limit: Detector Characterization Needs Nelson Christensen Carleton.
LIGO-G Z Instrum. Lines and Blind CW Search K. Riles - University of Michigan 1 Status Report on Instrumental Line Catalog and Blind.
LIGO- G M Paths to Improving Detector Performance Rainer Weiss, David Shoemaker NSF Review Caltech, 30 April 2001.
LSC Meeting at LHO LIGO-G E 1August. 21, 2002 SimLIGO : A New LIGO Simulation Package 1. e2e : overview 2. SimLIGO 3. software, documentations.
Gabriele Vajente ILIAS WG1 meeting - Frascati Noise Analysis Tools at Virgo.
LIGO-G Z Detchar Introduction (8/16/06)K. Riles - University of Michigan 1 SixtyHertzMon Update Junyi Zhang & Keith Riles (University of Michigan)
LIGO-G Z DMT Status for UL Analysis K. Riles - University of Michigan 1 DMT Monitors -- Status Update for Upper Limits Analysis.
May 29, 2006 GWADW, Elba, May 27 - June 21 LIGO-G0200XX-00-M Data Quality Monitoring at LIGO John Zweizig LIGO / Caltech.
Status of Virgo GWDAW12 Status of Virgo GWDAW Dec Leone B. Bosi INFN and University of Perugia (Italy) On behalf of the Virgo Collaboration.
1 Locking in Virgo Matteo Barsuglia ILIAS, Cascina, July 7 th 2004.
LIGO-G Z Detector Characterization SummaryK. Riles - University of Michigan 1 Summary of Detector Characterization Sessions Keith Riles (University.
Magnetic Field Stability Measurements Joe DiMarco 23Oct07.
S.Klimenko, March 2003, LSC Burst Analysis in Wavelet Domain for multiple interferometers LIGO-G Z Sergey Klimenko University of Florida l Analysis.
LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 1 Introduction to Detector Characterization Sessions.
Stochastic Background Data Analysis Giancarlo Cella I.N.F.N. Pisa first ENTApP - GWA joint meeting Paris, January 23rd and 24th, 2006 Institute d'Astrophysique.
LIGO-G Z Introd. to Detect. Charact. Sessions K. Riles - University of Michigan 1 Introduction to the Detector Characterization.
Detector Characterisation and Optimisation David Robertson University of Glasgow.
LIGO-G Z Detector Characterization Summary K. Riles - University of Michigan 1 Summary of the Detector Characterization Sessions Keith.
Joshua Smith August Identifying and eliminating limiting noise sources of GEO600 LSC Meeting, Hanford WA, August `04 Joshua Smith for the GEO team.
S.Klimenko, LSC March, 2001 Line Noise Investigation l Outline Ø Line Noise Investigation task Ø E2 data, line monitoring Ø Documentation Ø Lines observed.
LIGO-G E S2 Data Quality Investigation John Zweizig Caltech/LIGO.
LIGO-G Z 23 October 2002LIGO Laboratory NSF Review1 Searching for Gravitational Wave Bursts: An Overview Sam Finn, Erik Katsavounidis and Peter.
LIGO-G Z Report on E3/E4 Lock Losses K. Riles - University of Michigan 1 Report on E3/E4 Lock Losses David Chin, Dick Gustafson Keith.
LIGO-G Z Report on the S2 RunK. Riles / S. Whitcomb 1 Report on the S2 Run Keith Riles (University of Michigan) Stan Whitcomb (LIGO–Caltech)
S.Klimenko, LSC meeting, March 2002 LineMonitor Sergey Klimenko University of Florida Other contributors: E.Daw (LSU), A.Sazonov(UF), J.Zweizig (Caltech)
LIGO-G Z Report on E2 Lock Losses K. Riles - University of Michigan 1 Report on E2 Lock Losses David Chin, Dick Gustafson Keith Riles.
The Proposed Holographic Noise Experiment Rainer Weiss, MIT On behalf of the proposing group Fermi Lab Proposal Review November 3, 2009.
LIGO-G Z March 21, 2007 March 2007 LIGO/Virgo Meeting - DetChar 1 S5 Spectral Line Cataloguing Keith Thorne for the Spectral Line Working Group.
The Proposed Holographic Noise Experiment
Detector Characterization
Status of Virgo GWDAW Dec 13-16
Summary of the iKAGRA Run
Planning for the S4 Run Keith Riles (University of Michigan)
Summary of the iKAGRA Run
LIGO Scientific Collaboration - University of Michigan
Presentation transcript:

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 1 Detector Characterization Software Tools Keith Riles University of Michigan

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 2 Elements of Detector Characterization Commissioning Online Diagnostics Environmental Monitoring (hardware) Offline Data Monitoring »Performance Characterization »Transient Analysis (subgroup chair: Fred Raab) Data Set Reduction (subgroup chair: Jim Brau) Data Set Simulation »Parametrized simulation (subgroup chair: Sam Finn) »End-to-End Model

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 3 Some Goals of the Working Group Quantify “Steady-State” Behavior of IFO’s »Monitor instrumental & environmental noise »Measure channel-to-channel correlations »Quantify IFO sensitivity to standard-candle GW sources »Characterization includes both description & correction Identify transients due to instrument or environment »Avoid confusion with astrophysical sources »Identify & correct contamination in data stream »Diagnose and fix recurring disturbances

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 4 Examples of Ambient Noise Seismic Violin modes Internal mirror resonances Laser frequency noise Electrical mains (60 Hz & harmonics) Coupling of orientation fluctuations into GW channel Electronics noise (RF pickup, amplifiers, ADC/DAC)

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 5 Examples of Transients Earthquakes, Trains, Airplanes, Wind Gusts Army tanks firing (!) Machinery vibration Magnetic field disturbances Wire slippage Violin mode ringdown Flickering optical modes Electronic saturation (analog / digital) Servo instability Dust in beam

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 6 Characterization Methods Measured optical, RF, geometrical parameters Calibration curve Statistical trends & analysis (outliers, likelihood) Power spectra Time-frequency analysis »Band-limited RMS »Wavelets Principal value decomposition Non-linear couplings measurement Matched filters

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 7 Evolution of LSC Detector Characterization Efforts Initial work: »Developing infrastructure of online characterization tools: –Data Monitor Tool (DMT -- J. Zweizig) –Diagnostic Test Tool (DTT -- D. Sigg) »Developing software tools & monitors for DMT (broad effort) Moving toward 2nd phase - two-pronged approach: »Investigations focussed on engineering runs –15 teams formed for E2 (Nov 2000) –13 teams formed for E3 (March 2001) –Prelim reports from all E2 teams given at monthly DetChar telecons –Final presentations & written reports due at March LSC meeting »Participation in four Upper Limits Working Groups for E6 –Special session at March LSC meeting to identify where help needed

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 8 Software Developed for the Data Monitor Tool (DMT)

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 9 Getting Information Downstream Detector characterization used online for diagnosis / warnings and offline for interpreting data Characterization conveyed downstream to LDAS via meta-database and frame-contained constants Meta-database entries (examples) »Calibration constants and power spectra »Environmental noise measures »Cross-coupling coefficients »Line noise strength and phase »Triggers (for veto or “handle with care”): –Environmental disturbances –Excess noise or unstable conditions

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 10 Other Detector Characterization Software Tools Data Set Reduction: »Wavelet methods (lossless & lossy) -- Sergey Klimenko (Florida) »Data set summary -- Benoit Mours (Annecy/CIT) et al »Data channel selection -- David Strom (Oregon) Data Set Simulation - Parametrized »SimData package -- Sam Finn (Penn State) –Time domain simulation tool (shot noise, radiation pressure, thermal substrates, suspensions, seismic) –Integrated into End-to-End Model

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 11 Engineering Run Investigations (E2 - November 2000)

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 12 Engineering Run Investigations (E2 - November 2000)

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 13 Engineering Run Investigations (E3 - March 2001)

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 14 Engineering Run Investigations (E3 - March 2001)

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 15 DMT Example: Seismic Noise Monitoring

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 16 Engineering Run Results (Calibration studies) Scale set by absolute calibration Visible calibration lines (“c”) 30% calibration accuracy c c c c

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 17 Engineering Run Results (Line noise monitoring) AC Power line monitor: Phase of 60 Hz:

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 18 Engineering Run Results (Line noise monitoring) Tracking strength of injected calibration lines: (One arm stable; the other degrading with time in lock)

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 19 Engineering Run Results (Line noise monitoring) Non-linearity signature - sidebands on calibration lines:

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 20 Engineering Run Results (Lock losses) Tidal correction disabled - periodic saturation of coils

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 21 Engineering Run Results (Tidal modelling) Comparison of tidal derivative prediction with data (one free parameter): Differential Mode

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 22 Engineering Run Results (Tidal modelling) Comparison of tidal derivative prediction with data (one free parameter): Common Mode

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 23 Engineering Run Results (Transients) Airplane seen in E1 run: (seismometer time/freq plot)

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 24 Back to the Data Monitor Tool...

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 25 How to make all of this useful downstream? Power spectra / transfer functions: Technical details to decide - but straightforward Quality flagging: Some things obvious and easy, others will require running experience - but straightforward Environmental / Instrumental Transients: Much work to do - but straightforward

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 26 How to make all of this useful downstream? Quasi-stationary data characterization and correction: Not necessarily straightforward What is needed beyond nominal power spectrum & calibration curve? How exactly will it be used? Data correction: Regression of cross-channel correlations Line removal

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 27 How to make all of this useful downstream? Regression of linear cross-channel correlations: Will know most important correlations But how to remove? Various schemes possible One already in DMT (A. Ottewill) Another on the way in LDAS data cond. API How do we systematically verify no harm done? Bilinear couplings: Prototype online DMT monitor exists Do we dare try to correct for these?

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 28 How to make all of this useful downstream? Line removal: Two line trackers in the DMT (allow removal) At least one other in LAL now (allows removal) Another on the way in LDAS data cond. API (?) Again, how do we verify no harm done?

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 29 Bringing things together... How do we coordinate ongoing diagnostics development with needs of upper limits groups? Suggestions: Designate Detector Characterization liaison (or two) in each U.L. group to ensure communication Talk directly to DMT monitor authors to ensure useful information gets to database or trends (or ?) Identify overlapping needs among U.L. groups and consolidate efforts

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 30 Bringing things together... Emphasis to date on defining standardized background monitors in 24/7 operation - Time to think about the user! Existing Interactive Tools for Data Exploration: Data Viewer - Works well but limited and inflexible Diagnostic Test Tool - Great for power spectra, correlations, inspecting time series w/o aliasing Data Monitor Tool - Allows for interactive data exploration via root interface and DMT classes. Lots of potential but not yet exploited much. Some stand- alone root-based GUI’s exist (e.g., Sylvestre’s TID). Matlab - Lots of tools already available, data input supported (at some bandwidth).

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 31 Bringing things together... Event-driven (database or local trigger) analysis using root environment under study by D. Sigg for burst upper limits group - probably relevant to all UL groups (and to operations).

LIGO-G Z Detector Characterization Software Tools K. Riles - University of Michigan 32 Bringing things together... Hope: Specific physics goals will improve focus of online/offline data monitoring Hard deadlines will concentrate the minds...