1. June 27, 2002 EK 1 Data Analysis Overview Erik Katsavounidis LIGO-MIT PAC12 – June 27, 2002 LIGO-G020293-00-Z

2. June 27, 2002 EK 2 Data Analysis Participation l All LIGO-MIT group members participate across all four LSC Data Analysis Working Groups l P. Fritschel/M. Zucker co-chair Stochastic/Continuous Wave Groups l Participation in the Inspiral group under the leadership of P. Brady and G. Gonzalez: »Mittleman, Mavalvala, Harry l Participation in the Stochastic group under the leadership of P. Fritschel and J. Romano: »Weiss, Regimbau, Katsavounidis l Participation in the Bursts group under the leadership of S. Finn and P. Saulson: »Zucker, Sylvestre, Shoemaker, Ottoway, Katsavounidis, Cadonati, Bayer, Ballmer, Adhikari »Operation of the Bursts group’s main analysis computing infrastructure »Direct contribution in algorithms, vetoes and pipeline integration of the E7 engineering run

3. June 27, 2002 EK 3 LDAS Cluster at MIT l Laboratory and LSC facility l Operational as of summer 2001 »Anderson, Blackburn, Lazzarini »Bayer, Thomas, Katsavounidis, Shoemaker l Additional DMT machines l Data Challenges: »September 2001, Bursts/Stochastic »May 2002, Bursts E7 dress rehearsal l Start up hardships- being worked on (CIT,CSR,MIT): »facilities »network

4. June 27, 2002 EK 4 Bursts Upper Limit Effort l Goal: search for transients of unmodeled (or not well modeled) gravitational radiation l Search filters »Slope (Arnaud et al, Daw) – slope of data in time domain »Excess power (Anderson et al) – power of the data above noise in time-frequency band »Time-Frequency clusters (Sylvestre) – thresholded spectrograms combined with clustering analysis »Externally triggered analysis: GRB’s, neutrinos via on/off IFO cross correlation (Finn et al)

5. June 27, 2002 EK E7 Bursts Search Pipeline Strain Data Aux Data (non GW) Quality Check Data split Burst Analysis Algorithms (DSO) Feature Extraction LDAS, DB (T, dT, SNR) Glitch Analysis Algorithms (DMT) Feature Extraction DB (T, dT, SNR) GW/Veto anticoincidence Event Analysis Tools … LLOLLO Aux Data (non GW) Strain Data Aux Data (non GW) Quality Check Data split Burst Analysis Algorithms (DSO) Feature Extraction LDAS, DB (T, dT, SNR) Glitch Analysis Algorithms (DMT) Feature Extraction DB (T, dT, SNR) GW/Veto anticoincidence Event Analysis Tools … LHOLHO Aux Data (non GW) IFO-IFO Coincidence And Clustering Million Sanity Checks Quantify Upper Limit Quantify efficiency Simulated data Based on Astrophysical Source Knowledge

6. June 27, 2002 EK 6 E7 Pipeline Implementation l E7 = Dec 28, 2001 – Jan 14, 2002 of which ~400 hours reflected LLO-4k/LHO-2k coincident data taking. l A complete pipeline analysis of E7 data was carried out by Julien Sylvestre for his PhD work – defended June 24. l A complementary approach was adopted and carried out in a synergetic way by the Bursts group: »select ~3 hours of ‘playground’ data over which pipeline optimization (‘tuning’) is going to be performed (filter thresholds, veto parameters) »prepare statistical tools and methods under a unified and commonly accepted platform »apply and confront multiple veto-defining methods and channels: purely time-domain, template-matching (IUL) on at least 4+4 auxiliary channels »study each of the bursts filters independently

7. June 27, 2002 EK 7 E7 Pipeline Implementation »perform analysis of single IFO and multi-IFO (coincidence) events »quantify Upper Limit by estimating the background via time- shifting and using confidence belt statistics »establish sensitivity to modeled sources via software injection (Monte Carlo by Alan Weinstein) l Redundant and complementary ways to look at the E7 burst data: luxury or necessity?

8. June 27, 2002 EK 8 What have we learnt? Instrument was bursty during E7 Are events coming from a random source? How varying are the amplitudes of the instrumental glitches?

9. June 27, 2002 EK 9 Where are we standing now? l Infrastructure to perform any Bursts pipeline analysis is in place and in multiple versions »finalize the tuning of vetoes l Define and integrate in pipeline post-(time) coincidence analysis strategies l Complete study of efficiency of search (DSO’s+vetoes) to benchmark sources l Proceed with the full set of E7 data l Express upper limit in astrophysical terms

10. June 27, 2002 EK E7 Stochastic Search Pipeline LHOLLO CLEAN DATA Environmental noise removal for each ~90 s stretch of data Datacond API FFT INJECTION Cross correlation statistic detector geometry Optimal filter: Whitening:  f   detector geometry and sensitivity Gaussian random generator ~16 min

11. June 27, 2002 EK 11 Looking at S1 and beyond l Ready to start looking at burst triggers and vetoes as they are coming in l A good number of new people brought online and ready to pursue instrument and search studies l S1 will give the opportunity to exercise the full path of most analyses via hardware-injected data (Alan Weinstein, Daniel Sigg, Szabi Marka) l Develop new methods for extracting bursts and their features via time-frequency decomposition beyond Fourier, e.g. wavelet bases (S. Ballmer’s thesis work) l Feasibility studies to bring up the search for bursts close to real-time