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...
Главный автор: | Peters, J |
---|---|
Другие авторы: | Jarvis, M |
Формат: | Диссертация |
Язык: | English |
Опубликовано: |
2019
|
Предметы: |
Схожие документы
-
On the Encounter between the GASP Galaxy JO36 and the Radio Plume of GIN 049
по: Alessandro Ignesti, и др.
Опубликовано: (2023-01-01) -
An integral-field spectroscopic study of low-powered radio galaxies
по: Warren, J
Опубликовано: (2018) -
Extragalactic radio sources/
по: Heeschen, David S., и др.
Опубликовано: (1982) -
Multifrequency Radio Observations of the Dissociative Cluster Merger CIZA J0107.7+5408
по: Emma Schwartzman, и др.
Опубликовано: (2025-01-01) -
Radio galaxies : radiation transfer, dynamics, stability and evolution of a synchrotron plasmon/cA G Pacholczyk
по: 224999 Pacholczyk, A. G.
Опубликовано: (1977)