Near-Infrared Observations of a Redshift 5.34 Galaxy: Further Evidence for Dust Absorption in the Early Universe

October 1998 • 1998ApJ...506L..89A

Authors • Armus, L. • Matthews, K. • Neugebauer, G. • Soifer, B. T.

Abstract • Imaging at 1.25 and 2.20 μm has been obtained of the field containing the galaxy (RD1) found at redshift z=5.34 by Dey et al. This galaxy has been detected at 1.25 μm, while the lower redshift (z=4.02) galaxy also found in the same field by Dey et al. was detected at both 1.25 and 2.20 μm. Comparison to stellar population synthesis models indicates that if RD1 is a young (t<10⁸ yr) galaxy, significant reddening (A_V>0.5 mag) is indicated. Combined with observations of other high-redshift systems, these data show that dust is likely to be an important component of young galaxies even at redshifts of z>5. The extinction-corrected monochromatic luminosity of RD1 at 1500 Å is then a factor of about 3 larger than L^*₁₅₀₀ as determined by Dickinson for z~3 starburst galaxies. The implied star formation rate in RD1, corrected for extinction, is ~50-100 h^-2₅₀ M_solar yr^-1.

Based on observations obtained at the W. M. Keck Observatory, which is operated jointly by the California Institute of Technology and the University of California.

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Lee Armus

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