The ultraviolet luminosity function of star-forming galaxies between redshifts of 0.6 and 1.2

We use ultraviolet imaging taken with the XMM-Newton Optical Monitor telescope (XMM-OM), covering 280 square arcminutes in the UVW1 band (effective wavelength 2910 Angstroms) to measure rest-frame ultraviolet (1500 Angstrom) luminosity functions of galaxies with redshifts z between 0.6 and 1.2. The...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	arXiv.org 2021-06
Hauptverfasser:	Page, M J, Dwelly, T, McHardy, I, Seymour, N, Mason, K O, Sharma, M, Kennea, J A, Sasseen, T P, Rawlings, J I, Breeveld, A A, Ferreras, I, Loaring, N S, Walton, D J, Symeonidis, M
Format:	Artikel
Sprache:	eng
Schlagworte:	Active galactic nuclei Galaxies Infrared imaging Infrared photometry Luminosity Physics - Astrophysics of Galaxies Red shift Star formation Ultraviolet astronomy Ultraviolet imagery XMM (spacecraft)
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!