Star formation density and Halpha luminosity function of an emission-line-selected galaxy sample at z~ 0.24

Eduard Westra, David Jones

Research output: Contribution to journalArticleResearchpeer-review

10 Citations (Scopus)

Abstract

We use narrow-band imaging (full width at half-maximum = 70 ??) to select a sample of emission-line galaxies between 0.20 a?? z a?? 1.22 in two fields covering 0.5 deg2. We use spectroscopic follow-up to select a subsample of HI?-emitting galaxies at z a?? 0.24 and determine the HI? luminosity function and star formation density at z a?? 0.24 for both of our fields. Corrections are made for imaging and spectroscopic incompleteness, extinction and interloper contamination on the basis of the spectroscopic data. When compared to each other, we find the field samples differ by I?I? = 0.2 in faint-end slope and I?log [L* (erg s-1)] = 0.2 in luminosity.
Original languageEnglish
Pages (from-to)339 - 354
Number of pages16
JournalMonthly Notices of the Royal Astronomical Society
Volume383
Issue number1
DOIs
Publication statusPublished - 2008
Externally publishedYes

Cite this