There appears to be continuing confusion as to whether or not counts of extragalactic radio sources are compatible with the steady state theory. Ryle and Clarke found considerable discrepancies between the observed counts and those predicted on the basis of steady state. Hoyle argues that the source counts are in agreement with the steady state theory except for a deficiency of only 5 sources per steradian at the bright end. I present here an explicit derivation of source counts expected in the steady state on the basis of identifications and redshifts of a complete sample of radio galaxies and quasi-stellar sources
In this paper we show normalized differential source counts $n(S)$ at 408 MHz and 1.4 GHz of radio ...
A simple numerical procedure for analysing the counts of extra-galactic radio sources is described. ...
We present spectra for a sample of radio sources from the FIRST survey, and use them to define the f...
There appears to be continuing confusion as to whether or not counts of extragalactic radio sources ...
The problem of the number count of radio sources as a function of the incident flux is shown to depe...
The numerical consequences of the theory developed in two previous papers are examined in more detai...
The existence of large condensations introduces a descrete element into the steady state theory. Thi...
The data on angular sizes and redshifts of ultracompact radio sources used by Jackson & Dodgson ...
The most powerful radio sources in the local Universe are found in giant elliptical galaxies. Lookin...
We use the most up-to-date cosmological evolution models of dusty star-forming galaxies an...
The radio sky covers a large range of sources, from small single galaxies to large clusters of galax...
I define 3 samples of extragalactic radio sources of type FRII, containing 26 objects in total. The...
A sample of 20 powerful extended radio galaxies with redshifts between zero and 2 were used to deter...
The large number of differences between high- and low-redshift radio galaxies have almost all been d...
International audienceWe use the most up-to-date cosmological evolution models of dusty star-forming...
In this paper we show normalized differential source counts $n(S)$ at 408 MHz and 1.4 GHz of radio ...
A simple numerical procedure for analysing the counts of extra-galactic radio sources is described. ...
We present spectra for a sample of radio sources from the FIRST survey, and use them to define the f...
There appears to be continuing confusion as to whether or not counts of extragalactic radio sources ...
The problem of the number count of radio sources as a function of the incident flux is shown to depe...
The numerical consequences of the theory developed in two previous papers are examined in more detai...
The existence of large condensations introduces a descrete element into the steady state theory. Thi...
The data on angular sizes and redshifts of ultracompact radio sources used by Jackson & Dodgson ...
The most powerful radio sources in the local Universe are found in giant elliptical galaxies. Lookin...
We use the most up-to-date cosmological evolution models of dusty star-forming galaxies an...
The radio sky covers a large range of sources, from small single galaxies to large clusters of galax...
I define 3 samples of extragalactic radio sources of type FRII, containing 26 objects in total. The...
A sample of 20 powerful extended radio galaxies with redshifts between zero and 2 were used to deter...
The large number of differences between high- and low-redshift radio galaxies have almost all been d...
International audienceWe use the most up-to-date cosmological evolution models of dusty star-forming...
In this paper we show normalized differential source counts $n(S)$ at 408 MHz and 1.4 GHz of radio ...
A simple numerical procedure for analysing the counts of extra-galactic radio sources is described. ...
We present spectra for a sample of radio sources from the FIRST survey, and use them to define the f...