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.

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Presentation transcript:

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: <100mK; Pulkovo: <1mK) 4. Nearby BGR or Cosmological?- Detection of SZ- effect (Y.Par, 1970) as the proof of Cosmological origin of CMB 5.First check of the J.Silk prediction (protogalaxies at z=1000) with strong NEGATIVE result (Y.Par, Ph.D 1969) Deep CONTACT WITH ZELDOVICH GROUP Ideology changed: from proto galaxies to protoclusters; pancekes UP-DOWN 5. Check of scalar, vector, tensor modes of CMB anisotropy (Y.Par, 1973, 1975, 1984). All results below predictions 6. Check of neutrino (Moscow University data) Cosmology 7. Check of inflation Cosmology – POSITIVE RESULT (Y.Par, A.Starobinski, A.Chepurnov) ZELDOVICH-SAKHAROV and “COSMOLOGICAL GENE” Project

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, Галатические координаты и полоса Зенитного обзора

Новый обзор 500 кв. градусов

RZF и FIRST

RZF и DSS

RZF и FRII

RZF и FIRST: Tripple Merging??

Кандидат в самый мощный объект Ранней Вселенной RG z=4.515 S 120mJy, SMBH

VLA изображение и БТА R – фильтр (Ly- alpha)

Synchrotron Galaxy noise: Models and new RATAN-600 data

Синхротрон на высоких широтах и «Two-step» реионизация

Синхротрон и поляризация Наиболее точный прогноз для ПЛАНКА

Обнаружение шума на l=200

Synchrotron Galaxy SCREEN

Обнаружение радио грануляции на 1см на Луне

МАРС-2, 1см Луна и ФАЗА (см край)

1/f шум на дм. больше белой компоненты в 10 раз.

Galaxy Synchrotron and l=200

bII Spectral Index variation

RATAN-600 and WMAP Example of possible WMAP correction and 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

МАРС-3 (32 рупора) и Поляризация Сахаровских осцилляций

Fundamental Science and Technology

CMB PROBEMS and New Type of the TELESCOPES

OLD and NEW ASTRONOMY