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S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

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Page 1: S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

S5 BNS Inspiral Update

Duncan BrownCaltech

LIGO-G060265-00-Z

Page 2: S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

Introduction

• Talk divided into two parts:

• S5 Online Analysis» Runs all the time at LHO and LLO

» Single detector search, only generates trigger SNR

» Displayed by InspiralMon and daily glitch pages

• S5 First Epoch BNS search» Start of run (11/4/05) to start of LHO commissioning (02/06/06)

» Standard 1 - 3 Msun 2pN inspiral templates

» Full search pipeline (filter, signal based vetoes, coincidence)

Page 3: S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

S5 Online Analysis

• Runs with latency ~ 20 mins at LHO and LLO• Results displayed in control room via InspiralMon

• Not much to say…• Other than the occasional brief downtime, this has been running well

Page 4: S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

S5 BNS Glitch Pages

• Display top 10 loudest single IFO triggers with SNR > 25

Triggers with noknown DQ flag

Triggers withknown DQ flag

Page 5: S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

S5 BNS Glitch Pages

• Scimons encouraged to look at glitches with no current DQ explanation» Glitch group have been working with these triggers

• Experts encouraged to create DQ flags for glitches that are “obvious” but are not currently flagged

• To do:» Time cluster triggers with 10 sec window (real soon now!)

» Random sampling of triggers in SNR range 6 - 25 for scimons and glitch group to follow up

Page 6: S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

S5 Hardware Injection Analysis

• Script that looks at hardware injections using online triggers (Fairhurst)

Currently run by hand. Plan is to automate generation

and add to scimon checklist

Page 7: S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

S5 First Epoch Analysis

Distance to optimally oriented 1.4,1.4 solar mass BNS at = 8

First S5 EpochNov 4, 2005 -Feb 6, 2006

Page 8: S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

S5 Accidental Coincidencesand Simulated Signals

• Tune pipeline using background, playground (10% of data) and injections• Measure background by applying time slides before coincidence• Add simulated signals to detector data to evaluate analysis performance

Page 9: S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

Efficiency in Triple Coincident Data

Page 10: S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

Efficiency in Triple Coincident Data

These are injections found as H1H2 double coincidence,

but which have a large effective distance in LLO

(due to detector misalignment)

Apparent structurehere due to low number statistics

Page 11: S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

Histogram of Number of Galaxies

Page 12: S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

Histogram of Number of Galaxies

Current galaxy catalogruns out at 25 Mpc:

This should keep going up(needs to be fixed for S5)

Page 13: S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

Ball Park of S5 Epoch 1 Result

• Doing final tuning of vetoes before opening box» Group has been busy closing out S3/4 analyses…

• Total time in triple coincident data ~ 0.1 years

• The total luminosity ~ 300 L10 = 190 MWEG

• R90% ~ 0.08 yr-1 L10-1 = 0.13 yr-1 MWEG-1

• But would not quote this number outside this room…» Galaxy distribution incomplete (limit will go down)

» Efficiency computed at threshold, not loudest event (limit will go up)

» No consideration of background, errors, etc.

» Not reviewed!

Page 14: S5 BNS Inspiral Update Duncan Brown Caltech LIGO-G060265-00-Z

Future for S5 BNS

• Complete S5 first epoch upper limit (or detection?) for approval at August LSC meeting

• At August LSC meeting we will have S5 second epoch (end of LHO commissioning to start of LLO commissioning) in same state first epoch is now

• Setting up automated code to analyze data for BNS weekly for a detection/no detection statement

• Detection or final upper limit at end of S5…?