LBDS 53W091: An old, red galaxy at z = 1.552

Hyron Spinrad, Arjun Dey, Daniel Stern, James Dunlop, John Peacock, Raul Jimenez, Rogier Windhorst

Research output: Contribution to journalArticle

262 Scopus citations

Abstract

The weak radio source LBDS 53W091 is associated with a very faint (R ≈ 24.5) red (R-K ≈ 5.8) galaxy. Long spectroscopic integrations with the W. M. Keck telescope have provided an absorption-line redshift, z = 1.552 ± 0.002. The galaxy has a rest frame ultraviolet spectrum very similar to that of an F6 V star, and a single-burst old stellar population that matches the IR colors, the optical energy distribution and the spectral discontinuities has a minimum age of 3.5 Gyr. We present detailed population synthesis analyses of the observed spectrum in order to estimate the time since the last major epoch of star formation. We discuss the discrepancies in these estimates resulting from using different models, subjecting the UV spectrum of M32 to the same tests as a measure of robustness of these techniques. The models most consistent with the data tend to yield ages at z = 1.55 of ≳ 3.5 Gyr, similar to that inferred for the intermediate-age population in M32. Depending upon the assumed Hubble constant and the value of Ω0, only certain cosmological expansion times are consistent with the age of LBDS 53W091; in particular, for Ω0 = 1, only models with H0 ≲ 45 km s-1 Mpc-1 are permitted. For H0 = 50 km s-1 Mpc-1 and Ω0 = 0.2, we derive a formation redshift, z,z≥ 5.

Original languageEnglish (US)
Pages (from-to)581-601
Number of pages21
JournalAstrophysical Journal
Volume484
Issue number2
DOIs
StatePublished - 1997

Keywords

  • Distance scale
  • Galaxies: distances and redshifts
  • Galaxies: evolution
  • Galaxies: photometry
  • Galaxies: stellar content

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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    Spinrad, H., Dey, A., Stern, D., Dunlop, J., Peacock, J., Jimenez, R., & Windhorst, R. (1997). LBDS 53W091: An old, red galaxy at z = 1.552. Astrophysical Journal, 484(2), 581-601. https://doi.org/10.1086/304381