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Detectability of High-Redshift Elliptical Galaxies in the Hubble Deep Field

Published 1997 November 4 © 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Dan Maoz 1997 ApJ 490 L135 DOI 10.1086/311027

1538-4357/490/2/L135

Abstract

Relatively few intensively star-forming galaxies at redshifts of z>2.5 have been found in the Hubble Deep Field (HDF). This has been interpreted to imply a low space density of elliptical galaxies at high z, possibly due to a late (z<2.5) epoch of formation or to dust obscuration of the ellipticals that are forming at z~3. I use Hubble Space Telescope UV (~2300 Å) images of 25 local early-type galaxies to investigate a third option, that ellipticals formed at z>4.5 and were fading passively by 2<z<4.5. Present-day early-type galaxies are faint and centrally concentrated in the UV. If elliptical galaxies formed their stars in a short burst at z>4.5 and have faded passively to their present brightnesses at UV wavelengths, they would generally be below the HDF detection limits in any of its bands at z>2.5. Quiescent z~3 ellipticals, if they exist, should turn up in sufficiently deep IR images.

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10.1086/311027