01622nas a2200301   4500008004100000245004700041210004300088260001200131300001200143490000800155520072700163653002600890653003200916653001900948653001900967653002300986653004001009653001201049653002501061653002001086653002501106653001801131653002601149100001801175700002201193700002001215856008501235       1974                        eng d00aThe Polarization of Radio Sources at 31 CM0 aPolarization of Radio Sources at 31 CM  c10/1974  a117-1310 v1693 a<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>10aAstronomical Catalogs10aextragalactic radio sources10afaraday effect10ainterferometry10amicrowave emission10apolarized electromagnetic radiation10aQuasars10aradiant flux density10aradio astronomy10astatistical analysis10atables (data)10avery high frequencies1 aHaves, Philip1 aConway, Robin, G.1 aStannard, David  uhttps://simulationresearch.lbl.gov/publications/polarization-radio-sources-31-cm