Presentation is loading. Please wait.

Presentation is loading. Please wait.

Image Deconvolution of XMM-Newton Data

Similar presentations


Presentation on theme: "Image Deconvolution of XMM-Newton Data"— Presentation transcript:

1 Image Deconvolution of XMM-Newton Data
Tao Song, Steve Sembay Dept. Physics & Astronomy University of Leicester

2 Overview Introduction Richardson-Lucy Algorithm IDL program Examples
Future works

3 Vela PWNe Chandra EPIC-MOS Deconvolved

4 Introduction Observed images are usually degraded, i.e. the shape of a target will be distorted by the PSF. Image deconvolution is to recover the original scene from the observed degraded data. Two types of algorithms: empirical (e.g. CLEAN) and theoretical (e.g. Richardson-Lucy) IDL software was developed to do image deconvolution on XMM-Newton data Modified Richardson-Lucy algorithms and blind deconvolution algorithm were tested

5 Richardson-Lucy Deconvolution
where where n is the number of pixels in a image.

6 IDL program – main panel

7 IDL program – detail panel

8 Examples – P0401240501M1S001MIEVLI0000.FIT
1.1’’ per pixel FLAG == 0 CCDNR == 1 PATTERN == 0 50 Iterations 2 = 1.80 PSF Data: PSF_M1_0a_VelaPSR_110208_i3_s1.fits

9 Examples – P0401240501M1S001MIEVLI0000.FIT
Peak: (Y=244) FWHM: 3.14 (242.37~245.51) Peak: (X=268) FWHM: 3.29 (266.70~269.99) Peak: (Y=244) FWHM: 7.45 (240.28~247.73) Peak: (X=269) FWHM: 8.32 (264.58~272.91)

10 Examples – P011108001M1S001MIEVLI000.FIT
1.1’’ per pixel FLAG == 0 CCDNR == 1 PATTERN == 0 50 Iterations 2 = 1.33 PSF Data: PSF_M1_0a_VelaPSR_110208_i3_s1.fits

11 Examples – P011108001M1S001MIEVLI000.FIT
Peak: (Y=235) FWHM: 4.19 (232.96~237.15) Peak: (X=257) FWHM: 4.39 (254.35~258.74) Peak: (Y=235) FWHM: (227.38~241.56) Peak: (X=257) FWHM: (249.44~263.23)

12 Examples – blind deconvolution
2 = 1.24 vs. 2 = 1.80 2 = 1.20 vs. 2 = 1.33

13 Examples – blind deconvolution
Output strongly depends on the initial inputs, i.e. observed image and PSF

14 Examples – blind deconvolution
A hint ? (which one is more proper ?)

15 Examples – blind deconvolution
2 = vs 2 = 1.80 Peak: (Y=244) FWHM: 3.07 (242.38~245.45) Peak: (X=268) FWHM: 3.19 (266.71~269.90) Peak: (Y=244) FWHM: 3.14 (242.37~245.51) Peak: (X=268) FWHM: 3.29 (266.70~269.99)

16 Examples – blind deconvolution
2 = vs 2 = 1.33 Peak: (Y=235) FWHM: 4.17 (232.94~237.10) Peak: (X=257) FWHM: 4.38 (254.32~258.70) Peak: (Y=235) FWHM: 4.19 (232.96~237.15) Peak: (X=257) FWHM: 4.39 (254.35~258.74)

17 Future works Apply image deconvolution on more XMM-Newton Data
More tests on different PSFs (based on the outputs of blind deconvolution) Modifications on original Richardson-Lucy algorithm More functions in the IDL program


Download ppt "Image Deconvolution of XMM-Newton Data"

Similar presentations


Ads by Google