A statistical study of the spectral index distribution of radiosources selected at 408 MHz.

Details A statistical study of the spectral index distribution of radiosources selected at 408 MHz. A statistical study of the spectral index distribution of radiosources selected at 408 MHz.

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...304..357g&link_type=abstract

Astronomy and Astrophysics, v.304, p.357

Astronomy and Astrophysics

Astrophysics

1

Cosmology: Observation, Radio Continuum: Galaxies

Scientific paper

We used two large, statistically complete Catalogs of radio sources, the B3 (408MHz) and the 87GB (4850MHz), to study spectral index distribution versus flux density. We derived the relation spectral index-flux density in the range 30-4000mJy (408MHz) and we introduced a new definition of average spectral index of a radiosource population. We found that there is no evidence of any change in the average spectral index within the above-mentioned flux range, and that the sky distribution of spectral index is isotropic.

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