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...
Main Author: | Peters, J |
---|---|
Other Authors: | Jarvis, M |
Format: | Thesis |
Language: | English |
Published: |
2019
|
Subjects: |
Similar Items
-
On the Encounter between the GASP Galaxy JO36 and the Radio Plume of GIN 049
by: Alessandro Ignesti, et al.
Published: (2023-01-01) -
An integral-field spectroscopic study of low-powered radio galaxies
by: Warren, J
Published: (2018) -
Extragalactic radio sources/
by: Heeschen, David S., et al.
Published: (1982) -
Multifrequency Radio Observations of the Dissociative Cluster Merger CIZA J0107.7+5408
by: Emma Schwartzman, et al.
Published: (2025-01-01) -
Radio galaxies : radiation transfer, dynamics, stability and evolution of a synchrotron plasmon/cA G Pacholczyk
by: 224999 Pacholczyk, A. G.
Published: (1977)