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Brightness-weighted differential source counts $S^2 n(S)$ spanning the eight decades of flux density between $0.25,mumathrm{Jy}$ and 25 Jy at 1.4 GHz were measured from (1) the confusion brightness distribution in the MeerKAT DEEP2 image below $10,mumathrm{Jy}$, (2) counts of DEEP2 sources between $10,mumathrm{Jy}$ and $2.5,mathrm{mJy}$, and (3) counts of NVSS sources stronger than $2.5,mathrm{mJy}$. We present our DEEP2 catalog of $1.7 times 10^4$ discrete sources complete above $S = 10,mumathrm{Jy}$ over $Omega = 1.04,mathrm{deg}^2$. The brightness-weighted counts converge as $S^2 n(S) propto S^{1/2}$ below $S = 10,mumathrm{Jy}$, so $>99%$ of the $Delta T_mathrm{b} sim 0.06,mathrm{K}$ sky brightness produced by active galactic nuclei and $approx96%$ of the $Delta T_mathrm{b} sim 0.04,mathrm{K}$ added by star-forming galaxies has been resolved into sources with $S geq 0.25,mumathrm{Jy}$. The $Delta T_mathrm{b} approx 0.4,mathrm{K}$ excess brightness measured by ARCADE 2 cannot be produced by faint sources smaller than $approx 50,mathrm{kpc}$ if they cluster like galaxies.
We present very long baseline interferometry (VLBI) observations of 179 radio sources in the COSMOS field with extremely high sensitivity using the Green Bank Telescope (GBT) together with the Very Long Baseline Array (VLBA) (VLBA+GBT) at 1.4 GHz, to
We present a study of the 1173 sources brighter than $S_{1.4,rm GHz}= 120,mu$Jy detected over an area of $simeq 1.4,hbox{deg}^{2}$ in the Lockman Hole field. Exploiting the multi-band information available in this field for $sim$79% of the sample, so
We matched the 1.4 GHz local luminosity functions of star-forming galaxies (SFGs) and active galactic nuclei to the 1.4 GHz differential source counts from $0.25 mumathrm{Jy}$ to 25 Jy using combinations of luminosity and density evolution. We prese
We present results from simulations of the extragalactic polarized sky at 1.4 GHz. As the basis for our polarization models, we use a semi-empirical simulation of the extragalactic total intensity (Stokes I) continuum sky developed at the University
Aims. To investigate the flux density modulation from pulsars and the existence of specific behaviour of modulation index versus frequency. Methods. Several pulsars have been observed with the Effelsberg radio telescope at 8.35 GHz. Their flux densit