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Timing analysis of SGR 1627-41. Liang, Jau-Shian Dep. of Physics, NTHU 2004/3/11. Outline. Introduction (1).SGR 1627-41 (2).epoch folding,H-test Data Reduction and Analysis Future work. introduction. 1. The first SGR was observed on March 5, 1979.

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Timing analysis of sgr 1627 41

Timing analysis of SGR 1627-41

Liang, Jau-Shian

Dep. of Physics, NTHU

2004/3/11


Outline
Outline

  • Introduction

    (1).SGR 1627-41

    (2).epoch folding,H-test

  • Data Reduction and Analysis

  • Future work


Introduction
introduction

  • 1. The first SGR was observed on March 5, 1979.

  • 2. It was discovered some bursts repeated at the same position in 1986.

  • 3. Properties of SGRs

    (1)they repeat

    (2)soft spectra

    (3)short duration


Sgr 1627 41
SGR 1627-41

  • First observation:

    Ulysses (1998–07-17)

  • RA, DEC SINBAD 16h35m52.00s,-47o35’14.0”J2000

    BappoSAX 16h35m49.8s,-47o35’44”J2000

    ASCA 16h35m46.41s,-47o35’13.1”J2000

  • associate with nearby SNR : SNR G337.0-0.1


phases

Phases:

The probability density of phases:


Epoch folding

If Nj is large, S is approximately distributed as xn-12 for a flat probability density.


Rayleigh test

If the phase probability density is flat, the displacements are a two-dimensional random walk.


The means of c and s depend on the Fourier transform sine and cosine amplitudes of f(q).

The Rayleigh power is P=R2/N

==>

The random variabl 2P is therefore approximately distributed as x22.

==>


Z and cosine amplitudes of f(m2 -test and H-test

A generalization of the Rayleigh test:

Include the effect of a zealous obser in the caculation of significance:


Compare fft with epoch folding
Compare FFT with Epoch Folding and cosine amplitudes of f(

  • Epoch folding is more sensitive to the nonsinusoidal pulse shapes characteristics of X-ray pulsars.

  • Epoch folding provides a straightforward approach to handling gaps which routinely appear in data.

  • Epoch folding is extremely time-consuming on the computer.


Compare h test with epoch folding
Compare H-test with Epoch Folding and cosine amplitudes of f(

  • Epoch folding is more sensitive to the nonsinusoidal pulse shapes characteristics of X-ray pulsars.

  • The H-test is free of the binning uncertainties associated with epoch folding.


Data reduction and analysis
Data Reduction and Analysis and cosine amplitudes of f(

ASCA

1. 57041000 HURLEY 1999-02-06

duration:187.6ks gis:78.4ks sis:72.7ks

BoppoSAX

1. 70821005 Jan van Paradijs 1999-08-08

lecs:34.8ks mecs:80.4ks

2. 70566001 Jan van Paradijs 1998-08-06

lecs:21.3ks mecs:44.9ks

3. 70566002 Jan van Paradijs 1998-09-16

lecs:12ks mecs:30ks


Data reduction
Data reduction and cosine amplitudes of f(

  • Use standard screened event file

  • Filtering

    Filter region

    Filter energy: 1-10kev (21-213)

  • Barycentric correction


  • Elevation Angle (ELV) and cosine amplitudes of f(>5

  • Stable Pointing Directions (ACS, ANG_DIST): ACS==0 && ANG_DIST 0 && ANG_DIST <0.01

  • South Atlantic Anomaly (SAA) ==0

  • Cut-off Rigidity (COR)>4 (GeV/c)

  • (G2_H0+G2_H2+G3_H0+G3_H2)<45 && (G2_H0+G2_H2+G3_H0+G3_H2)<0.45*COR**2-13*COR+125 && RBM_CONT <100



gis2 the GIS is 6 arcmin (24 pixels).

ra=16h35m46.41s

dec=-47o35’13”.1

Radius=4’

Ntotal=48.8k

Nreg=2355


gis3 the GIS is 6 arcmin (24 pixels).

ra=16h35m46.41s

dec=-47o35’13”.1

Radius=4’

Ntotal=51.4k

Nreg=3017


Data reduction bapposax
Data reduction(BappoSAX) the GIS is 6 arcmin (24 pixels).

  • Merging of MECS units:MECS2, MECS3 > MECS23

  • Filtering

    Filter time : GTI_XY.fits

    Filter region

    Filter energy: 2-10kev (43-215)

  • Barycentric correction


70566001 the GIS is 6 arcmin (24 pixels).

Ra=16h35m49.8s

dec=-47o35’44”

Radius=4’

Ntotal=49.9k

Nreg=2359


70566002 the GIS is 6 arcmin (24 pixels).

Ra=16h35m49.8s

dec=-47o35’44”

Radius=4’

Ntotal=27.3k

Nreg=1340


70566005 the GIS is 6 arcmin (24 pixels).

Ra=16h35m49.8s

dec=-47o35’44”

Radius=4’

Ntotal=65.3k

Nreg=2409


Use efsearch to detect signal in a large range of period
Use efsearch to detect signal in a large range of period the GIS is 6 arcmin (24 pixels).

  • Data: ASCA gis2 & gis3

  • Range of period: 1-1000 s

  • Resolution: p*p/T/10, T=138600 s

  • Total tries: 1323k tries


  • Data:SAX 70566001, 70566002, 70821005 the GIS is 6 arcmin (24 pixels).

  • Range of period: 1-1000 s

  • Resolution: p*p/T/10

  • Total tries:

    70566001 887k tries T=85634

    70566002 651k tries T=62376

    70821005 1662k tries T=163642


Use h test to detect signal in a large range of period
Use H-test to detect signal in a large range of period the GIS is 6 arcmin (24 pixels).

  • Data:SAX 70566001, 70566002, 70821005 Range of period: 1-1000 s

  • Resolution: p*p/T/10,


Future work
Future work the GIS is 6 arcmin (24 pixels).

  • Combine more data: XTE data

  • Search other range of period: 0.01-1 s

  • Estimate upper limit


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