Discovery of a possibly old galaxy at z = 6.027, multiply imaged by the massive cluster Abell 383

Johan Richard, Jean Paul Kneib, Harald Ebeling, Daniel P Stark, Eiichi Egami, Andrew K. Fiedler

Research output: Contribution to journalArticle

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Abstract

We report the discovery of a unique z = 6.027 galaxy, multiply imaged by the cluster Abell 383 and detected in new Hubble Space Telescope ACS and WFC3 imaging, as well as in Warm Spitzer observations. This galaxy was selected as a pair of i-dropouts; its suspected high redshift was confirmed by the measurement of a strong Lyman α line in both images using Keck/DEIMOS. Combining Hubble and Spitzer photometry after correcting for contamination by line emission (estimated to be a small effect), we identify a strong Balmer break of 1.5 mag. Taking into account the magnification factor of 11.4 ± 1.9 (2.65 ± 0.17 mag) for the brightest image, the unlensed AB magnitude for the source is 27.2±0.05 in theH band, corresponding to a 0.4 L* galaxy, and 25.7 ± 0.08 at 3.6 μm. The UV slope is consistent with β ~ 2.0, and from the rest-frame UV continuum we measure a current star formation rate of 2.4 ± 1.1 M⊙ yr-1. The unlensed half-light radius is measured to be 300 pc, from which we deduce a star-forming surface density of ~10 M⊙ yr-1 kpc--2. The Lyman α emission is found to be extended over ~3 arcsec along the slit, corresponding to ~5 kpc in the source plane. This can be explained by the presence of a much larger envelope of neutral hydrogen around the star-forming region. Finally, fitting the spectral energy distribution (SED) using seven photometric data points with simple SED models, we derive the following properties: very little reddening, an inferred stellar mass of M* = 6 × 109 M⊙, and an inferred age of ~800 Myr (corresponding to a redshift of formation of ~18). The star formation rate of this object was likely much stronger in the past than at the time of observation, suggesting that we may be missing a fraction of galaxies at z ~ 6 which have already faded in rest-frame UV wavelengths.

Original languageEnglish (US)
JournalMonthly Notices of the Royal Astronomical Society: Letters
Volume414
Issue number1
DOIs
StatePublished - Jun 2011
Externally publishedYes

Fingerprint

galaxies
star formation rate
spectral energy distribution
energy
hydrogen
wavelength
dropouts
stars
magnification
stellar mass
Hubble Space Telescope
photometry
slits
contamination
envelopes
slopes
continuums
radii
rate
distribution

Keywords

  • Galaxies: high redshift
  • Gravitational lensing: strong

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Discovery of a possibly old galaxy at z = 6.027, multiply imaged by the massive cluster Abell 383. / Richard, Johan; Kneib, Jean Paul; Ebeling, Harald; Stark, Daniel P; Egami, Eiichi; Fiedler, Andrew K.

In: Monthly Notices of the Royal Astronomical Society: Letters, Vol. 414, No. 1, 06.2011.

Research output: Contribution to journalArticle

Richard, Johan ; Kneib, Jean Paul ; Ebeling, Harald ; Stark, Daniel P ; Egami, Eiichi ; Fiedler, Andrew K. / Discovery of a possibly old galaxy at z = 6.027, multiply imaged by the massive cluster Abell 383. In: Monthly Notices of the Royal Astronomical Society: Letters. 2011 ; Vol. 414, No. 1.
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abstract = "We report the discovery of a unique z = 6.027 galaxy, multiply imaged by the cluster Abell 383 and detected in new Hubble Space Telescope ACS and WFC3 imaging, as well as in Warm Spitzer observations. This galaxy was selected as a pair of i-dropouts; its suspected high redshift was confirmed by the measurement of a strong Lyman α line in both images using Keck/DEIMOS. Combining Hubble and Spitzer photometry after correcting for contamination by line emission (estimated to be a small effect), we identify a strong Balmer break of 1.5 mag. Taking into account the magnification factor of 11.4 ± 1.9 (2.65 ± 0.17 mag) for the brightest image, the unlensed AB magnitude for the source is 27.2±0.05 in theH band, corresponding to a 0.4 L* galaxy, and 25.7 ± 0.08 at 3.6 μm. The UV slope is consistent with β ~ 2.0, and from the rest-frame UV continuum we measure a current star formation rate of 2.4 ± 1.1 M⊙ yr-1. The unlensed half-light radius is measured to be 300 pc, from which we deduce a star-forming surface density of ~10 M⊙ yr-1 kpc--2. The Lyman α emission is found to be extended over ~3 arcsec along the slit, corresponding to ~5 kpc in the source plane. This can be explained by the presence of a much larger envelope of neutral hydrogen around the star-forming region. Finally, fitting the spectral energy distribution (SED) using seven photometric data points with simple SED models, we derive the following properties: very little reddening, an inferred stellar mass of M* = 6 × 109 M⊙, and an inferred age of ~800 Myr (corresponding to a redshift of formation of ~18). The star formation rate of this object was likely much stronger in the past than at the time of observation, suggesting that we may be missing a fraction of galaxies at z ~ 6 which have already faded in rest-frame UV wavelengths.",
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AB - We report the discovery of a unique z = 6.027 galaxy, multiply imaged by the cluster Abell 383 and detected in new Hubble Space Telescope ACS and WFC3 imaging, as well as in Warm Spitzer observations. This galaxy was selected as a pair of i-dropouts; its suspected high redshift was confirmed by the measurement of a strong Lyman α line in both images using Keck/DEIMOS. Combining Hubble and Spitzer photometry after correcting for contamination by line emission (estimated to be a small effect), we identify a strong Balmer break of 1.5 mag. Taking into account the magnification factor of 11.4 ± 1.9 (2.65 ± 0.17 mag) for the brightest image, the unlensed AB magnitude for the source is 27.2±0.05 in theH band, corresponding to a 0.4 L* galaxy, and 25.7 ± 0.08 at 3.6 μm. The UV slope is consistent with β ~ 2.0, and from the rest-frame UV continuum we measure a current star formation rate of 2.4 ± 1.1 M⊙ yr-1. The unlensed half-light radius is measured to be 300 pc, from which we deduce a star-forming surface density of ~10 M⊙ yr-1 kpc--2. The Lyman α emission is found to be extended over ~3 arcsec along the slit, corresponding to ~5 kpc in the source plane. This can be explained by the presence of a much larger envelope of neutral hydrogen around the star-forming region. Finally, fitting the spectral energy distribution (SED) using seven photometric data points with simple SED models, we derive the following properties: very little reddening, an inferred stellar mass of M* = 6 × 109 M⊙, and an inferred age of ~800 Myr (corresponding to a redshift of formation of ~18). The star formation rate of this object was likely much stronger in the past than at the time of observation, suggesting that we may be missing a fraction of galaxies at z ~ 6 which have already faded in rest-frame UV wavelengths.

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