The 5 GHz strong source surveys. IV - Survey of the area between declination 35 and 70 degrees and summary of source counts, spectra and optical identifications

I. I. K. Pauliny‐Toth, A. Witzel, H. Kuehr, E. B. Fomalont, M. M. Davis, K. I. Kellermann

The Astronomical Journal · 1978 · 78 citations · 0 references

Concepts

Abstract

A new zone (54) has been surveyed at 5 GHz and is essentially complete above 0.5 Jy. A total of 269 sources above this flux density were found in an area of 1.71 sr between declinations of 35 and 70 . Accurate flux densities at 2.7, 5.0, and 10.7 GHz are given, together with source coordinates accurate to between 1 and 5 arcsec, and proposed optical identifications. Sources below the completeness limit are also listed, giving a catalog of 484 sources. The results of the S4 survey are combined with those of the previous 5 GHz surveys, with a 5 GHz strong source sample derived from the Parkes 2.7 GHz surveys, and with samples taken from deeper surveys made at 5 GHz to discuss the source counts, the source spectra and their relation to the optical identifications. The 5 GHz source counts differ from those derived at lower frequencies in that there is less evidence for either a steepening of the counts at high flux densities or for their convergence at very low flux densities. The counts indicate a possible anisotropy related to the superga1actic system.