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Ya.B. Zeldovich and Early History of Pulkovo Radio Astronomy School

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)

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Ya.B. Zeldovich and Early History of Pulkovo Radio Astronomy School

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  1. Ya.B. Zeldovich and Early Historyof 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

  2. 3K: Nearby or Very distant?

  3. First ZS (SZ) effect , 1970

  4. RATAN-600 World biggest REFLECTOR

  5. RATAN-600 Deep Fields

  6. New 32- Channels Deep Zenith Survey

  7. Кандидат в самый мощный объект Ранней ВселеннойRG z=4.515 S 120mJy, SMBH

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

  9. Synchrotron Galaxy noise: Models and new RATAN-600 data

  10. Синхротрон на высоких широтахи «Two-step»реионизация

  11. Синхротрон и поляризацияНаиболее точный прогноз для ПЛАНКА

  12. Обнаружение шума на l=200

  13. Synchrotron Galaxy SCREEN

  14. 1/f шум на дм. больше белой компоненты в 10 раз.

  15. Galaxy Synchrotron andl=200

  16. bII Spectral Index variation

  17. RATAN-600 and WMAPExample of possible WMAP correctionand Z reionization interpretation

  18. CMB E-Polarization History

  19. RATAN-600 and World DATA(polarization from synchrotron)

  20. Discovery of the Sky polarization at 30GHz with up to 0.1 arcmin resolution

  21. МАРС-3 (32 рупора) и Поляризация Сахаровских осцилляций

  22. Fundamental Science and Technology

  23. CMB PROBEMS and New Typeof theTELESCOPES

  24. OLD and NEW ASTRONOMY

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