1967
DOI: 10.1007/bf01040968
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Precision absolute measurements of the radiation flux from the discrete sources Taurus-A and Cassiopeia-A and of the atmospheric absorption of radio waves at ?=5.28 cm

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1971
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“…Golnev et al (1965) 4.69 650 Kellermann et al (1969) 5.00 680 5 Dmitrenko and Strezhneva (1967) 5.68 646 5 Medd and Ramana (1965a) 6.66 565 5 Allen andBarrett (1966, 1967) 8.25 567 4.8 Lazarewski et al (1963) 9.36 560 5.4 Allen and Barrett (1966) 15.5 461 5.9 Williams et al (1965) 19.6 588 9 Staelin et al (1964) 25. atmosphere. A more likely explanation, as noted by Hobbs et al (1969), lies in the corrections to the observed flux densities due to the finite angular size of the Crab Nebula when narrow beamwidths are used.…”
Section: The Radio Spectrum 10mentioning
confidence: 99%
“…Golnev et al (1965) 4.69 650 Kellermann et al (1969) 5.00 680 5 Dmitrenko and Strezhneva (1967) 5.68 646 5 Medd and Ramana (1965a) 6.66 565 5 Allen andBarrett (1966, 1967) 8.25 567 4.8 Lazarewski et al (1963) 9.36 560 5.4 Allen and Barrett (1966) 15.5 461 5.9 Williams et al (1965) 19.6 588 9 Staelin et al (1964) 25. atmosphere. A more likely explanation, as noted by Hobbs et al (1969), lies in the corrections to the observed flux densities due to the finite angular size of the Crab Nebula when narrow beamwidths are used.…”
Section: The Radio Spectrum 10mentioning
confidence: 99%