Skip navigation
Skip navigation

Infrared-faint radio sources are at high redshifts: Spectroscopic redshift determination of infrared-faint radio sources using the Very Large Telescope

Herzog, A.; Middelberg, E; Norris, R P; Sharp, Robert; Spitler, Lee R.; Parker, Quentin A

Description

Context. Infrared-faint radio sources (IFRS) are characterised by relatively high radio flux densities and associated faint or even absent infrared and optical counterparts. The resulting extremely high radio-to-infrared flux density ratios up to several

CollectionsANU Research Publications
Date published: 2014
Type: Journal article
URI: http://hdl.handle.net/1885/74190
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361/201323160

Download

File Description SizeFormat Image
01_Herzog_Infrared-faint_radio_sources_2014.pdf730.43 kBAdobe PDF    Request a copy


Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  20 July 2017/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator