First spectroscopic measurements of [O III] emission from Lyα selected field galaxies at z ∼ 3.1

Emily M. McLinden, Steven L. Finkelstein, James E. Rhoads, Sangeeta Malhotra, Pascale Hibon, Mark L A Richardson, Giovanni Cresci, Andreas Quirrenbach, Anna Pasquali, Fuyan Bian, Xiaohui Fan, Charles E. Woodward

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Abstract

We present the first spectroscopic measurements of the [O III] 5007 line in two z3.1 Lyα emitting galaxies (LAEs) using the new near-infrared instrument LUCIFER1 on the 8.4 m Large Binocular Telescope. We also describe the optical imaging and spectroscopic observations used to identify these LAEs. Using the [O III] line we have measured accurate systemic redshifts for these two galaxies, and discovered a velocity offset between the [O III] and Lyα lines in both, with the Lyα line peaking 342 and 125 km s-1 redward of the systemic velocity. These velocity offsets imply that there are powerful outflows in high-redshift LAEs. They also ease the transmission of Lyα photons through the interstellar medium and intergalactic medium around the galaxies. By measuring these offsets directly, we can refine both Lyα-based tests for reionization, and Lyα luminosity function measurements where the Lyα forest affects the blue wing of the line. Our work also provides the first direct constraints on the strength of the [O III] line in high-redshift LAEs. We find [O III] fluxes of 7 and 36 ×10 -17 erg s-1 cm-2 in two z3.1 LAEs. These lines are strong enough to dominate broadband flux measurements that include the line (in this case, Ks -band photometry). Spectral energy distribution fits that do not account for the lines would therefore overestimate the 4000 (and/or Balmer) break strength in such galaxies, and hence also the ages and stellar masses of such high-z galaxies.

Original languageEnglish (US)
Article number136
JournalAstrophysical Journal
Volume730
Issue number2
DOIs
StatePublished - Apr 1 2011

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galaxies
flux measurement
erg
near infrared
infrared instruments
outflow
intergalactic media
spectral energy distribution
stellar mass
wings
photometry
luminosity
energy
telescopes
broadband
photons
distribution
test
measuring

Keywords

  • galaxies: high-redshift
  • intergalactic medium

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

McLinden, E. M., Finkelstein, S. L., Rhoads, J. E., Malhotra, S., Hibon, P., Richardson, M. L. A., ... Woodward, C. E. (2011). First spectroscopic measurements of [O III] emission from Lyα selected field galaxies at z ∼ 3.1. Astrophysical Journal, 730(2), [136]. https://doi.org/10.1088/0004-637X/730/2/136

First spectroscopic measurements of [O III] emission from Lyα selected field galaxies at z ∼ 3.1. / McLinden, Emily M.; Finkelstein, Steven L.; Rhoads, James E.; Malhotra, Sangeeta; Hibon, Pascale; Richardson, Mark L A; Cresci, Giovanni; Quirrenbach, Andreas; Pasquali, Anna; Bian, Fuyan; Fan, Xiaohui; Woodward, Charles E.

In: Astrophysical Journal, Vol. 730, No. 2, 136, 01.04.2011.

Research output: Contribution to journalArticle

McLinden, EM, Finkelstein, SL, Rhoads, JE, Malhotra, S, Hibon, P, Richardson, MLA, Cresci, G, Quirrenbach, A, Pasquali, A, Bian, F, Fan, X & Woodward, CE 2011, 'First spectroscopic measurements of [O III] emission from Lyα selected field galaxies at z ∼ 3.1', Astrophysical Journal, vol. 730, no. 2, 136. https://doi.org/10.1088/0004-637X/730/2/136
McLinden EM, Finkelstein SL, Rhoads JE, Malhotra S, Hibon P, Richardson MLA et al. First spectroscopic measurements of [O III] emission from Lyα selected field galaxies at z ∼ 3.1. Astrophysical Journal. 2011 Apr 1;730(2). 136. https://doi.org/10.1088/0004-637X/730/2/136
McLinden, Emily M. ; Finkelstein, Steven L. ; Rhoads, James E. ; Malhotra, Sangeeta ; Hibon, Pascale ; Richardson, Mark L A ; Cresci, Giovanni ; Quirrenbach, Andreas ; Pasquali, Anna ; Bian, Fuyan ; Fan, Xiaohui ; Woodward, Charles E. / First spectroscopic measurements of [O III] emission from Lyα selected field galaxies at z ∼ 3.1. In: Astrophysical Journal. 2011 ; Vol. 730, No. 2.
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abstract = "We present the first spectroscopic measurements of the [O III] 5007 line in two z3.1 Lyα emitting galaxies (LAEs) using the new near-infrared instrument LUCIFER1 on the 8.4 m Large Binocular Telescope. We also describe the optical imaging and spectroscopic observations used to identify these LAEs. Using the [O III] line we have measured accurate systemic redshifts for these two galaxies, and discovered a velocity offset between the [O III] and Lyα lines in both, with the Lyα line peaking 342 and 125 km s-1 redward of the systemic velocity. These velocity offsets imply that there are powerful outflows in high-redshift LAEs. They also ease the transmission of Lyα photons through the interstellar medium and intergalactic medium around the galaxies. By measuring these offsets directly, we can refine both Lyα-based tests for reionization, and Lyα luminosity function measurements where the Lyα forest affects the blue wing of the line. Our work also provides the first direct constraints on the strength of the [O III] line in high-redshift LAEs. We find [O III] fluxes of 7 and 36 ×10 -17 erg s-1 cm-2 in two z3.1 LAEs. These lines are strong enough to dominate broadband flux measurements that include the line (in this case, Ks -band photometry). Spectral energy distribution fits that do not account for the lines would therefore overestimate the 4000 (and/or Balmer) break strength in such galaxies, and hence also the ages and stellar masses of such high-z galaxies.",
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