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Galaxy and mass assembly: Evolution of the Hα luminosity function and star formation rate density up to z < 0.35

Gunawardhana, M; Hopkins, Andrew M.; Bland-Hawthorn, Joss; Brough, Sarah; Sharp, Robert; Loveday, Jon; Taylor, E N; Jones, D Heath; Lara-Lopez, M A; Bauer, Amanda E; Colless, Matthew; Owers, M S; Baldry, Ivan; Lopez-Sanchez, A R; Foster, C; Bamford, Steven P.; Brown, M J I; Driver, Simon P; Drinkwater, Michael John; Liske, Jochen; Meyer, M; Norberg, P; Robotham, A. S. G.; Ching, J. H. Y.; Cluver, M E; Croom, S; Kelvin, Lee; Prescott, M.; Steele, O; Thomas, Daniel; Wang, L.

Description

Measurements of the low -z Hα luminosity function, φ, have a large dispersion in the local number density of sources (~0.5-1 Mpc-3 dex-1), and correspondingly in the star formation rate density (SFRD). The possible causes for these discrepancies include

CollectionsANU Research Publications
Date published: 2013
Type: Journal article
URI: http://hdl.handle.net/1885/73662
Source: Monthly Notices of the Royal Astronomical Society
DOI: 10.1093/mnras/stt890

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