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Cosmic microwave background: Probing the universe from z = 6 to 1100
David N. Spergel
Astrophysical Sciences
Physics
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Keyphrases
Ground-based Observations
100%
Line-of-sight
100%
Physical Processes
100%
Wilkinson Microwave Anisotropy Probe
100%
Cosmic Microwave Background
100%
Recombination
100%
Growth of Structures
100%
Polarization Fluctuation
100%
CMB Observations
100%
Reionization
100%
Cosmic Microwave Background Polarization
100%
Physical Condition
100%
Temperature Fluctuation
100%
Cosmic Microwave Background Temperature
100%
Space Observation
100%
Physics
Cosmic Microwave Background
100%
Physics
50%
Physical Process
50%
Microwave Anisotropy Probe
50%
Line of Sight
50%
Reionization
50%