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Ya.B. Zeldovich and Early History of Pulkovo Radio Astronomy School. 1. Unidentified CMB signal (T.Shmaonov, 1957, Ph.D) 2. CMB or Black Body population of Radio Sources? (Y.Par, 1968) 3.CMB polarization (Penzias:
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3K: Nearby or Very distant?
First ZS (SZ) effect , 1970
RATAN-600 World biggest REFLECTOR
RATAN-600 Deep Fields
New 32- Channels Deep Zenith Survey
WMAP,
500 .
RZF FIRST
RZF DSS
RZF FRII
RZF FIRST: Tripple Merging??
RG z=4.515 S 120mJy, SMBH
VLA R (Ly- alpha)
Synchrotron Galaxy noise: Models and new RATAN-600 data
Two-step
l=200
Synchrotron Galaxy SCREEN
1
-2, 1 ( )
1/f . 10 .
Galaxy Synchrotron and l=200
bII Spectral Index variation
RATAN-600 and WMAPExample of possible WMAP correctionand Z reionization interpretation
CMB E-Polarization History
RATAN-600 and World DATA(polarization from synchrotron)
Discovery of the Sky polarization at 30GHz with up to 0.1 arcmin resolution
-3 (32 )
Fundamental Science and Technology
CMB PROBEMS and New Type of the TELESCOPES
OLD and NEW ASTRONOMY