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Optical-IR Spectral Energy Distributions of z>2 Lyman Break Galaxies

Marcin Sawicki·H. K. C. Yee
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Abstract

Broadband optical and IR spectral energy distributions are determined for spectroscopically confirmed z>2 Lyman break objects in the Hubble Deep Field (HDF). These photometric data are compared to spectral synthesis models which take into account the effects of metallicity and of internal reddening due to dust. It is found that, on average, Lyman break objects are shrouded in enough dust (typically E(B-V)~0.3) to suppress their UV fluxes by a factor of more than 10. The dust-corrected star formation rate in a typical HDF Lyman break object is ~60 h^-2 M_sun/yr (q_0=0.5). Furthermore, these objects are dominated by very young (<~0.2 Gyr, and a median of ~25 Myr) stellar populations, suggesting that star formation at high redshift is episodic rather than continuous. Typically, these star formation episodes produce ~10^9 h^-2 M_sun of stars, or ~1/20 of the stellar mass of a present-day L* galaxy.

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Marcin Sawicki, H. K. C. Yee. 1997-12-17. Optical-IR Spectral Energy Distributions of z>2 Lyman Break Galaxies. https://doi.org/10.1086/300291

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