Ya.B. Zeldovich and Early Historyof Pulkovo Radio Astronomy School1. Unidentified CMB signal (T.Shmaonov, 1957, Ph.D)2. CMB or Black Body population of Radio Sources? (Y.Par, 1968)3.CMB polarization (Penzias:

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