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Fitting Cosmological Models to the Radio Source Counts

A Corrigendum to this article was published on 30 December 1967

Abstract

Inspection of a properly formulated distribution for radio sources of local luminosity shows that the distribution is not as wide as has been thought. The distribution fits a Gaussian curve, with a standard deviation of one, to a good approximation.

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References

  1. Scott, P. F., and Ryle, M., Mon. Not. Roy. Astro. Soc., 122, 389 (1961).

    Article  ADS  Google Scholar 

  2. Hughes, R. G., and Longair, M. S., Mon. Not. Roy. Astro. Soc., 135, 131 (1967).

    Article  ADS  Google Scholar 

  3. Davidson, W., Mon. Not. Roy. Astro. Soc., 123, 425 (1962).

    Article  ADS  Google Scholar 

  4. Davidson, W., and Davies, M., Mon. Not. Roy. Astro. Soc., 127, 241 (1964).

    Article  ADS  Google Scholar 

  5. Davidson, W., and Davies, M., Mon. Not. Roy. Astro. Soc., 128, 363 (1964).

    Article  ADS  Google Scholar 

  6. Longair, M. S., Mon. Not. Roy. Astro. Soc., 133, 421 (1966).

    Article  ADS  Google Scholar 

  7. Davidson, W., and Davies, M., Mon. Not. Roy. Astro. Soc., 134, 405 (1966).

    Article  ADS  Google Scholar 

  8. Longair, M. S., and Scott, P. F., Mon. Not. Roy. Astro. Soc., 130, 379 (1965).

    Article  ADS  Google Scholar 

  9. Ryle, M., and Longair, M. S., Mon. Not. Roy. Astro. Soc., 136, 123 (1967).

    Article  ADS  Google Scholar 

  10. Horton, P. W., and Daintree, E. J., Nature, 215, 917 (1967).

    Article  ADS  Google Scholar 

  11. Longair, M. S., and Scheuer, P. A. G., Nature, 215, 919 (1967).

    Article  ADS  Google Scholar 

  12. Caswell, J. L., and Wills, D., Mon. Not. Roy. Astro. Soc., 135, 231 (1967).

    Article  ADS  Google Scholar 

  13. Heeschen, D. S., and Wade, C. M., Astro. J., 69, 277 (1964).

    Article  ADS  Google Scholar 

  14. Gower, J. F. R., Mon. Not. Roy. Astro. Soc., 133, 151 (1966).

    Article  ADS  Google Scholar 

Download references

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An erratum to this article is available at https://doi.org/10.1038/2161358f0

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DAVIDSON, W. Fitting Cosmological Models to the Radio Source Counts. Nature 216, 1076–1079 (1967). https://doi.org/10.1038/2161076a0

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