LIGO-G050331-00-Z 17 August 20051 ETG Sensitivity and Efficiency to Simulations: BlockNormal and SLOPE Amber L. Stuver Penn State University.

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LIGO-G Z 17 August ETG Sensitivity and Efficiency to Simulations: BlockNormal and SLOPE Amber L. Stuver Penn State University

LIGO-G Z 17 August Background and Motivation ETGs are not fundamentally equivalent Signal properties that ETGs were sensitive to was not initially obvious (see LIGO-G050110) What, then, are the signal properties that each ETG favor? To determine specific signal sensitivities: »Simulate signals of different lengths and amplitudes and inject into a white noise background (zero mean and unit variance) »Compare efficiencies for various signals to a baseline efficiency using Gaussian modulated white noise bursts

LIGO-G Z 17 August Gaussian Modulated White Noise BlockNormal

LIGO-G Z 17 August Gaussian Modulated White Noise SLOPE

LIGO-G Z 17 August Baseline Observations The efficiencies of both ETGs are dominated by the amplitude of the burst as long as the duration is not “very short” (< ~0.025 sec) The A 50 is in about the same area (A rss = 0.4 – 0.8  ) for both ETGs. However, the efficiency increases faster, wrt A rss, for BlockNormal than SLOPE There is a much higher false rate for SLOPE than BlockNormal: Tuned False RateCurrent False Rate BlockNormal0.55 events/s1.52 events/s Slope0.56 events/s4.33 events/s

LIGO-G Z 17 August A 50 for Different Signals BlockNormal SLOPE

LIGO-G Z 17 August Sigmoid Slopes for Different Signals BlockNormal SLOPE

LIGO-G Z 17 August Measuring ETG Performance WRT a Population Convolve the efficiency surface with a population The integral of this gives a measure of and ETG’s performance WRT a population

LIGO-G Z 17 August ROUGH Measured Population Performances BlockNormal has fairly consistent performance over different signal types While SLOPE’s performance can be higher, it is not as reliable Disk (~ A -3 )Isotropic (~ A -4 ) BlockNormalSLOPEBlockNormalSLOPE White Noise * * SG16 Hz Hz BH 16 Hz Hz * Population values are normalized to this

LIGO-G Z 17 August Conclusions The overall shape of the efficiency sigmoid is more meaningful than just the A 50 for describing an ETG’s performance BlockNormal’s efficiency does not have a significant frequency dependence while SLOPE does. BlockNormal’s performance is relatively constant over different signals and frequencies. SLOPE can perform much better on some signals and much worse on others. The background noise largely effects the tuning performance of the ETGs.