@article {370,
	title = {The Radio Structure of a Sample of 101 Quasars from the Parkes {\textpm}4{\textordmasculine} Survey},
	journal = {Monthly Notices of the Royal Astronomical Society},
	volume = {176},
	year = {1976},
	month = {08/1976},
	pages = {275-306},
	chapter = {275},
	keywords = {Angular Distribution, Astronomical Catalogs, Quasars, Radio Emission, Radio Sources (Astronomy), Radio Spectra, Spectrum Analysis, Ultrahigh Frequencies},
	author = {Michael Bentley and Philip Haves and Ralph E. Spencer and David Stannard}
}
@article {372,
	title = {High Resolution Observations of Extended Radio Sources at 1666 MHz},
	journal = {Monthly Notices of the Royal Astronomical Society},
	volume = {173},
	year = {1975},
	author = {Michael Bentley and Philip Haves and Ralph E. Spencer and David Stannard}
}
@article {375,
	title = {The Polarization of Radio Sources at 31 CM},
	journal = {Monthly Notices of the Royal Astronomical Society},
	volume = {169},
	year = {1974},
	month = {10/1974},
	pages = {117-131},
	chapter = {117},
	abstract = {<p>Measurements of the linear polarization of extragalactic radio sources have been made over a range of wavelengths in order to study both the properties of the sources themselves and the Faraday rotation along the line of sight to the observer. As part of a continuing program of such measurements the flux densities and integrated polarizations of 226 sources (including 134 quasars) were observed at 966 MHz (lambda 31 cm), to complement previous measurements at lambda 49 and lambda 74 cm (Conway et al. 1972). These results have been combined with others at shorter wavelengths in a discussion of the polarization properties of quasars (Conway et al. 1974). All the sources have angular sizes of 1 arcmin or less</p>},
	keywords = {Astronomical Catalogs, extragalactic radio sources, faraday effect, interferometry, microwave emission, polarized electromagnetic radiation, Quasars, radiant flux density, radio astronomy, statistical analysis, tables (data), very high frequencies},
	author = {Philip Haves and Robin G. Conway and David Stannard}
}
@article {374,
	title = {QSOs of High Redshift?},
	journal = {Nature},
	volume = {252},
	year = {1974},
	month = {11/1974},
	pages = {209-210},
	chapter = {209},
	author = {Ian W.A. Browne and Michael Bentley and Philip Haves and Neil J. McEwan and Ralph E. Spencer and David Stannard}
}
@article {376,
	title = {The Radio Polarization of Quasars},
	journal = {Monthly Notices of the Royal Astronomical Society},
	volume = {168},
	year = {1974},
	month = {07/1974},
	pages = {137-162},
	chapter = {137},
	abstract = {<p>Observations over a wide range of wavelengths, 2.2 <= λ <= 73 cm, have been combined to define the wavelength variation of the degree of linear polarization m(λ) for 120 quasars with known redshift. For the majority, m(λ) decreases monotonically with increasing wavelength but for 35 sources the polarization curve is inverted at short wavelengths. A classification is given, based on both the polarization curve and the radio spectrum, and the results are interpreted in terms of the presence or absence of opaque components in the source. The depolarization which occurs at long wavelengths is accounted for by a combination of spectral effects and Faraday depolarization. For 46 steep-spectrum sources the depolarization curve appears to be dominated by the Faraday effect, and has been used to deduce the electron density within the radiating components. In this group of sources the correlation between depolarization and redshift noted by Kronberg et al. is confirmed and strengthened. A discussion is given of some theoretical models of radio sources in the light of the depolarization data.</p>},
	author = {Robin G. Conway and Philip Haves and Philipp P. Kronberg and David Stannard and Jacques P. Vall{\'e}e and John F. C. Wardle}
}
