status of the hough cw search code - plans for s2 -

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Status of the Hough CW search code - Plans for S2 - A.M. Sintes, B. Krishnan, M.A. Papa Universitat de les Illes Balears, Spain Albert Einstein Institut, Germany LSC Meeting Hannover, August 2003 LIGO-G030517-00-Z

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Status of the Hough CW search code - Plans for S2 -. A.M. Sintes, B. Krishnan, M.A. Papa Universitat de les Illes Balears, Spain Albert Einstein Institut, Germany. LSC Meeting Hannover, August 2003 LIGO-G030517-00-Z. Outline. The hierarchical Hough search. Pipeline for S2 - PowerPoint PPT Presentation

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Page 1: Status of the Hough CW search code - Plans for S2 -

Status of the Hough CW search code- Plans for S2 -

A.M. Sintes, B. Krishnan, M.A. Papa

Universitat de les Illes Balears, Spain

Albert Einstein Institut, Germany

LSC Meeting

Hannover, August 2003

LIGO-G030517-00-Z

Page 2: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Outline

The hierarchical Hough search. Pipeline for S2

Statistics of the Hough maps. Frequentist analysis

Code statusResults on simulated & H1 data

Page 3: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

The concept of the Hough transform

– The idea is to perform a search over the total observation time using an incoherent (sub-optimal) method:

We propose to search for evidence of a signal whose frequency is changing over time in precisely the pattern expected for some one of the parameter sets

– The method used is the Hough transform

t

f

{,,f0,fi}

Page 4: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Hierarchical Hough transform strategy

Set upper-limit

Pre-processing

Divide the data set in N chunks

raw data GEO/LIGO

Construct set of short FT (tSFT)

Coherent search (,fi)

in a frequency band

Template placing

Incoherent search

Hough transform(f0, fi)

Peak selection in t-f plane

Candidates

selection

Candidates

selection

Page 5: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

The time-frequency pattern

• SFT data

• Demodulated data

Time at the SSB for a given sky position

) ˆ ˆ ( ) ( ) ( ) (0N n t t F t f

kk

Nk tTfftF )()( ˆ00

c

NtxttT

N

ˆ)()(ˆ

kkk Fff N̂

kF

kf

c

txtTkF

c

tvtTFtFt

k

kNk

k

kNk

)()(

)()()()(

1

ˆˆ0

nc

t vt f t f t fˆ

) () ( ) ( ) (0 0

Page 6: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Incoherent Hough search:Pipeline for S2

Set upper-limit

Pre-processing

Divide the data set in N chunksraw data

GEO/LIGO

Construct set of short FT (tSFT<1800s)

Incoherent search

Hough transform(f0, fi)

Peak selection in t-f plane

Candidates

selection

Page 7: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Peak selection in the t-f plane

Input data: Short Fourier Transforms (SFT) of time series (Time baseline: 1800 sec, calibrated)

For every SFT, select frequency bins i such

exceeds some threshold

time-frequency plane of zeros and ones

p(|h, Sn) follows a 2 distribution with 2 degrees of freedom:

The false alarm and detection probabilities for a threshold are

SFTin

i

i

ii )T(fS

)(fx

)(fn

)(fx 2

2

2 |~|

|~|

|~|

SFTin

i

SFTin

ii )T(fS

)(fh

)T(fS

)(fh 22

2 |~

|21

|~

|1

d),|(),|(,d),0|()|(0

0

0

00 nnnn ShpSheSpS

(f)h(f)n(f)x~~~

Page 8: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Hough statistics

• After performing the HT using N SFTs, the probability that the pixel {,,f0,fi} has a number count n is given by a binomial distribution:

• The Hough false alarm and false dismissal probabilities for a threshold n0

Candidates selection

)1(,

)1(),|(

2 pNpNpn

ppn

NNpnP

n

nNn

presentsignal

absentsignal

p

1

00

0

0

0

)1(),,(

)1(),,(

n

n

nNnH

N

nn

nNnH

n

NNn

n

NNn

Page 9: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Frequentist Analysis

• Perform the Hough transform for a set of points in parameter space ={,,f0,fi} S , given the data:

HT: S N n(

• Determine the maximum number count n*n* = max (n( S

• Determine the probability distribution p(n|h0) for a range of h0

30% 90%

Page 10: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Frequentist Analysis

• Perform the Hough transform for a set of points in parameter space ={,,f0,fi} S , given the data:

HT: S N n(

• Determine the maximum number count n*n* = max (n( S

• Determine the probability distribution p(n|h0) for a range of h0

• The 95% frequentist upper limit h095% is the value such that for repeated trials with a signal

h0 h095%, we would obtain n n* more than 95% of the time

N

nn

%

n|hp*

95

00.95

•Compute p(n|h0) via Monte Carlo signal injection, using S , and 0

[0,2], [-/4,/4], cos [-1,1].

Page 11: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Code Status

Stand-alone search code in final phase Test and validation codes (under CVS at AEI) Hough routines are part of the LAL library:

Page 12: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Code Status II

Auxiliary functions C-LAL compliant (under CVS at AEI to be incorporated into LAL or LALApps):– Read SFT data– Peak Selection (in white & color noise)– Statistical analysis of the Hough maps– Compute <v(t)>

Under development:– Implementation of an automatic handling of noise features.

Robust PSD estimator. – Monte Carlo signal injection analysis code.– Condor submission job.– Input search parameter files

Page 13: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Validation code-Signal only case- (f0=500 Hz)

• bla

Page 14: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Validation code-Signal only case- (f0=500 Hz)

Page 15: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Signal only case II

Page 16: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Signal only case II

Page 17: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Results on simulated data

Statistics of the Hough maps

f0~300Hz

tobs=60days

N=1440 SFTs

tSFT=1800s =0.2231

<n> = N=321.3074

n=(N(1-))=15.7992

Page 18: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Noise only case

Page 19: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Number count probability distribution

1440 SFTs

1991 maps

58x58 pixels

Page 20: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Comparison with a binomial distribution

Page 21: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

Set of upper limit. Frequentist approach.

95 %

N

nn

%

n|hp*

95

00.95

n*=395 =0.295

h095%

Page 22: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

1887 Calibrated SFT’s H1

TSFT = 1800s, Band : 263-268 Hz

H1 Analysis – the SFTs

26 SFT, 0.95 or 1.05

Page 23: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

H1 Results 264-265 Hz

Input: 1861 SFT

0.5x0.5 srad

Output: 19811 maps

(51x51 sky locations)

N=1861 SFTs =0.2019

Mean number count=373.8130

<n> = N=375.7294

n=(N(1-))=17.3168

Page 24: Status of the Hough CW search code - Plans for S2 -

LSC Meeting, August‘03, A.M. Sintes

H1 Results 264-265 Hz“upper limit estimate”

Loudest event n*=473

95%

n*

95 % upper limit

n*=473 =0.2715

220

2

22

50

3|

~|4

/105.5

SFTi

Hzin

Th)(fh

)(fS

22

)46.0(|

~|

SFTin

i

)T(fS

)(fh

h095% ~ 5x10-23 ?

Very preliminary