Perspectives of Space Submillimeter Astronomy
St. Petersburg, Russia, 30 September - 2 October, 2002

Viewgaphs of the presentation

	A.T. Bajkova The Methods of the CMB power angular spectrum reconstruction
	Slide02 Statistical description of the CMB anisotropies and mapping of small-angle sky patches
	Slide03 A model of the microwave sky
	Slide04 The data analysis pipeline
	Slide05 Spectral dependence of the Galactic components
	Slide06 Contribution of the various components as a function of angular scale. Contour levels of the different components in the angular scale-frequency plane
	Slide07 Physical model of the detected signal
	Slide08 Component separation methods
	Slide09 Testing of the Generalized Maximum Entropy Method (GMEM) for the CMB and point sources (PS) separation task
	Slide10 Examples of different UV-coverages in two-dimensional Fourier space used for GMEM reconstruction of PS distribution
	Slide11 Example N1 of separation of the CMB and PS components using the GMEM
	Slide12 Power angular spectra of components shown in Fig. P3
	Slide13 Example N2 of separation of the CMB and PS for large number of weak point sources
	Slide14 Example N3 of separation of the CMB and PS for larger number (than in Example N2) of weak point sources
	Slide15 Example N4 of reconstruction of the CMB in place of strong nonGaussianity (Galactic plane) using Fienup-like iteration algorithm
	Slide16 Formula for generation of the CMB and PS maps for simulation tasks
	Slide17 Simulation of high-precision removal of PS from CMB detected maps using interpolation algorithm in places of non-Gaussian contaminations: (a)the CMB given map (b)given PS distribution (c)CMB+PS detected map (d)UV-coverage in Fourier space used for recover of PS (e)the reconstructed PS map (f)the CMB reconstructed map obtained after subtraction of the PS reconstructed map (g)places of PS contaminations (h)(i)improved CMB maps reconstructed using two different interpolation algorithms
	Slide18 Angular power spectra of maps shown in Fig.P9
	Slide19 Angular power spectra of components in case of taking into account the instrumental pixel noise contribution

1. Bajkova A.T. et al. Maximum entropy method for reconstruction of the CMB images. - Gravitation & Cosmology, Supplement I (2002), pp. 77-82, astro-ph/0205112.

2. Bajkova A.T. A method of separation of the point sources foreground from the CMB maps. - Radiophysics & Quantum Electronics (in press).