The continuum emission from 1 to 2 GHz of The HI/OH/Recombination line survey of the inner Milky Way (THOR) at 0.5) of the FIRST survey indicates that these sources might be high z extragalactic compact objects. The similar pattern of one-point and two-point statistics of unclassified and compact sources with extragalactic surveys and simulations confirms the extragalactic origin of these sources
We present radio observations at 1.5 GHz of 32 local objects selected to reproduce the physical prop...
We use redshift determinations and spectral analysis of galaxies in the 2dF Galaxy Redshift Survey t...
This document is the Accepted Manuscript of the following article: J.R. Callingham, et al, 'Extragal...
Context: Radio continuum surveys of the Galactic plane can find and characterize H II regions, super...
We carried out a large program with the Karl G. Jansky Very Large Array (VLA): THOR: The H1, OH, Re...
We carried out a large program with the Karl G. Jansky Very Large Array (VLA): “THOR: The H i, OH, R...
We carried out a large program with the Karl G. Jansky Very Large Array (VLA): “THOR: The H?I, OH, R...
We have entered a new era of radio astronomy where the low radio frequency sky is accessible to astr...
In this paper we show normalized differential source counts at 408 MHz and 1.4 GHz of radio sources ...
This paper summarizes extensive observational studies of the closest ultraluminous radio galaxy Cygn...
The radio sky covers a large range of sources, from small single galaxies to large clusters of galax...
Context. Radio continuum surveys of the Galactic plane are an excellent way to identify different so...
A simple numerical procedure for analysing the counts of extra-galactic radio sources is described. ...
Analyses of the distribution of absolute brightness temperature over the radio sky have recently led...
Ultra-deep radio surveys are an invaluable probe of dust-obscured star formation, but require a clea...
We present radio observations at 1.5 GHz of 32 local objects selected to reproduce the physical prop...
We use redshift determinations and spectral analysis of galaxies in the 2dF Galaxy Redshift Survey t...
This document is the Accepted Manuscript of the following article: J.R. Callingham, et al, 'Extragal...
Context: Radio continuum surveys of the Galactic plane can find and characterize H II regions, super...
We carried out a large program with the Karl G. Jansky Very Large Array (VLA): THOR: The H1, OH, Re...
We carried out a large program with the Karl G. Jansky Very Large Array (VLA): “THOR: The H i, OH, R...
We carried out a large program with the Karl G. Jansky Very Large Array (VLA): “THOR: The H?I, OH, R...
We have entered a new era of radio astronomy where the low radio frequency sky is accessible to astr...
In this paper we show normalized differential source counts at 408 MHz and 1.4 GHz of radio sources ...
This paper summarizes extensive observational studies of the closest ultraluminous radio galaxy Cygn...
The radio sky covers a large range of sources, from small single galaxies to large clusters of galax...
Context. Radio continuum surveys of the Galactic plane are an excellent way to identify different so...
A simple numerical procedure for analysing the counts of extra-galactic radio sources is described. ...
Analyses of the distribution of absolute brightness temperature over the radio sky have recently led...
Ultra-deep radio surveys are an invaluable probe of dust-obscured star formation, but require a clea...
We present radio observations at 1.5 GHz of 32 local objects selected to reproduce the physical prop...
We use redshift determinations and spectral analysis of galaxies in the 2dF Galaxy Redshift Survey t...
This document is the Accepted Manuscript of the following article: J.R. Callingham, et al, 'Extragal...