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    Chapter

    Observational Limits on Neutral Hydrogen in Primordial Protoclusters

    After recombination in the early Universe, gas will pass through a neutral phase on its way to condensation into galaxies and stars. Radio emission in the reshifted 21 cm line of neutral hydrogen can be used t...

    R. D. Davies, J. Jaaniste, E. Saar in The Large Scale Structure of the Universe (1978)

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    Chapter

    The Motion of the Local Group of Galaxies with Respect to the Background of Galaxies

    A measurement of the motion of the Local Group of galaxies through the Universe provides an indication of their peculiar motion relative to the Hubble flow consequent upon the gravitational influence of the lo...

    R. D. Davies in Early Evolution of the Universe and its Present Structure (1983)

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    Chapter

    10 to 60 Arcmin Fluctuations in the Cosmic Microwave Background

    Considerable astronomical interest attaches to sensitive measurements of temperature fluctuations of the microwave background on scales of a few arcmins to a few degrees. We describe here the first in a series...

    A. N. Lasenby, R. D. Davies in Early Evolution of the Universe and its Present Structure (1983)

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    Chapter and Conference Paper

    High Sensitivity Observations of the Microwave Background Radiation

    Angular fluctuations in the cosmic microwave background radiation are indicators of the seed structure at recombination (z ≃ 1000) which subsequently evolves into the present-day Universe (z = 0). Such measure...

    R. D. Davies, A. N. Lasenby in Observational Cosmology (1987)

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    Chapter

    Peculiar Velocities of Nearby Spiral Galaxies

    We report measurements of peculiar velocities from a sample of over 300 intermediate-type spiral galaxies. The galaxies have been observed at λ21cm at Jodrell Bank and Parkes (Staveley-Smith & Davies 1987,1988...

    L. Staveley-Smith, R. D. Davies in Large Scale Structure and Motions in the Universe (1989)

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    Chapter

    Large Scale Structure: Its possible imprint on the CMB?

    We present the new results of the Jodrell-IAC Cosmic Microwave Background (CMB) anisotropy experiment for declination +40°. A similar level of sensitivity has been achieved with respect to the reported previou...

    R. A. Watson, R. Rebolo, J. E. Beckman in Large Scale Structure and Motions in the U… (1989)

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    Chapter

    Observations of Microwave Background Anisotropy at Tenerife and Cambridge

    A brief summary of the status of microwave background anisotropy observations at Tenerife and Cambridge is given. New 15 GHz Tenerife results give a preliminary limit of ΔT/T 2.5 x 10-5 on an angu...

    A. N. Lasenby, R. D. Davies, R. A. Watson in Observational Tests of Cosmological Inflat… (1991)

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    Chapter

    New Results on CMB Structure From the Tenerife Experiments

    Temperature fluctuations in the CMB (Cosmic Microwave Background) are a key prediction of cosmological models of structure formation in the early Universe. Observations at the Teide Observatory, Tenerife using...

    R. D. Davies, C. M. Gutéerrez, R. A. Watson in Examining the Big Bang and Diffuse Backgro… (1996)