The determination of the spatial distribution parameters of extragalactic radio sources observed in the decameter range - P(D)-analysis at a frequency of 25 MHz

Mathematics – Logic

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Decametric Waves, Extragalactic Radio Sources, Radiant Flux Density, Radiation Distribution, Radio Telescopes, Spatial Distribution

Scientific paper

An observational procedure is developed for determining experimentally the confusion fluctuations distribution of the UTR-2 radio telescope in the decametric wavelength range. The estimates of the "source number - flux density" differential relation parameters at the frequency 25 MHz for weak, unresolved by the telescope, radio sources have been obtained with the aid of the P(D)-analysis of the confusion distribution. An upturn section in the n25(S)/nE(S) - relation graph in the flux density range 0.75 - 10 Jy has been discovered. The cosmological effect of decrease of space density of the most distant extragalactic radio sources observed in the decametric range has been established.

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