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