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FMOS near-IR spectroscopy of herschel-selected galaxies: Star formation rates, metallicity and dust attenuation at z ~ 1

Roseboom, IG; Bunker, A; Sumiyoshi, M; Wang, L; Dalton, G; Akiyama, M; Bock, J; ... Zemcov, M; + view all (2012) FMOS near-IR spectroscopy of herschel-selected galaxies: Star formation rates, metallicity and dust attenuation at z ~ 1. Monthly Notices of the Royal Astronomical Society , 426 (3) 1782 - 1792. 10.1111/j.1365-2966.2012.21777.x. Green open access

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Abstract

We investigate the properties (e.g. star formation rate, dust attenuation, stellar mass and metallicity) of a sample of infrared (IR) luminous galaxies at z ∼ 1 via near-IR spectroscopy with Subaru-FMOS. Our sample consists of Herschel SPIRE and Spitzer MIPS selected sources in the COSMOS field with photometric redshifts in the range of 0.7 < zphot < 1.8, which have been targeted in two pointings (0.5 deg2) with FMOS. We find a modest success rate for emission-line detections, with candidate Hα emission lines detected for 57 of 168 SPIRE sources (34 per cent). By stacking the near-IR spectra we directly measure the mean Balmer decrement for the Hα and Hβ lines, finding a value of 〈E(B − V)〉 = 0.51 ± 0.27 for 〈LIR〉 = 1012 L⊙ sources at 〈z〉 = 1.36. By comparing star formation rates estimated from the IR and from the dust-uncorrected Hα line we find a strong relationship between dust attenuation and star formation rate. This relation is broadly consistent with that previously seen in star-forming galaxies at z ∼ 0.1. Finally, we investigate the metallicity via the N2 ratio, finding that z ∼ 1 IR-selected sources are indistinguishable from the local mass–metallicity relation. We also find a strong correlation between dust attenuation and metallicity, with the most metal-rich IR sources experiencing the largest levels of dust attenuation.

Type: Article
Title: FMOS near-IR spectroscopy of herschel-selected galaxies: Star formation rates, metallicity and dust attenuation at z ~ 1
Open access status: An open access version is available from UCL Discovery
DOI: 10.1111/j.1365-2966.2012.21777.x
Publisher version: http://dx.doi.org/10.1111/j.1365-2966.2012.21777.x
Language: English
Additional information: © 2012 RAS Definitive versions of articles pre-2013 are available at http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1365-2966, now published by http://mnras.oxfordjournals.org
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/1372820
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