Luminosity functions using new radio surveys

Luminosity functions using new radio surveys

<p>Galaxy evolution at radio wavelengths is often measured using luminosity functions which are commonly based on the luminosity (L) and redshift (z) of individual sources as well as the overall distribution for a sample. However, an important factor when K-correcting radio sources to their r...

Disgrifiad llawn

Manylion Llyfryddiaeth
Prif Awdur:	Peters, J
Awduron Eraill:	Jarvis, M
Fformat:	Traethawd Ymchwil
Iaith:	English
Cyhoeddwyd:	2019
Pynciau:	Galaxy evolution Astronomy Galaxies Astrophysics Active galaxies Interferometry Radio astronomy Radio telescopes

Eitemau Tebyg

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Remnant Radio Galaxy Candidates of Small Angular Sizes
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