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        A submillimetre galaxy at z=4.76 in the LABOCA survey of the Extended Chandra Deep Field South

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        0902.4464v1 (PDF, 518Kb)
        Author
        Coppin, Kristen
        Smail, Ian
        M. Alexander, David
        Weiss, Axel
        Walter, Fabian
        Swinbank, Mark
        Greve, Thomas
        Kovacs, Attila
        De Breuck, Carlos
        Dickinson, Mark
        Ibar, Edo
        Ivison, Rob
        Reddy, Naveen
        Spinrad, Hyron
        Stern, Daniel
        Brandt, Niel
        Chapman, Scott
        Dannerbauer, Helmut
        van Dokkum, Pieter
        Dunlop, James
        Frayer, David
        Gawiser, Eric
        Geach, James
        Huynh, Minh
        Knudsen, Kirsten
        Koekemoer, Anton
        Lehmer, Bret
        Menten, Karl
        Papovich, Casey
        Rix, Hans-Walter
        Schinnerer, Eva
        Wardlow, Julie
        van der Werf, Paul
        Attention
        2299/11301
        Abstract
        We report on the identification of the highest redshift submm-selected source currently known: LESSJ033229.4-275619. This source was detected in the Large Apex BOlometer CAmera (LABOCA) Extended Chandra Deep Field South (ECDFS) Submillimetre Survey (LESS), a sensitive 870-um survey (~1.2-mJy rms) of the full 30'x30' ECDFS with the LABOCA camera on the Atacama Pathfinder EXperiment (APEX) telescope. The submm emission is identified with a radio counterpart for which optical spectroscopy provides a redshift of z=4.76. We show that the bolometric emission is dominated by a starburst with a star formation rate of ~1000 Msun/yr, although we also identify a moderate luminosity Active Galactic Nucleus (AGN) in this galaxy. Thus it has characteristics similar to those of z~2 submm galaxies (SMGs), with a mix of starburst and obscured AGN signatures. This demonstrates that ultraluminous starburst activity is not just restricted to the hosts of the most luminous (and hence rare) QSOs at z~5, but was also occurring in less extreme galaxies at a time when the Universe was less than 10% of its current age. Assuming that we are seeing the major phase of star formation in this galaxy, then we demonstrate that it would be identified as a luminous distant red galaxy at z~3 and that the current estimate of the space density of z>4 SMGs is only sufficient to produce ~10% of the luminous red galaxy population at these early times. However, this leaves open the possibility that some of these galaxies formed through less intense, but more extended star formation events. If the progenitors of all of the luminous red galaxies at z~3 go through an ultraluminous starburst at z>4 then the required volume density of z>4 SMGs will exceed that predicted by current galaxy formation models by more than an order of magnitude.
        Publication date
        2009
        Published in
        Monthly Notices of the Royal Astronomical Society
        Published version
        https://doi.org/10.1111/j.1365-2966.2009.14700.x
        Other links
        http://hdl.handle.net/2299/11301
        Relations
        School of Physics, Astronomy and Mathematics
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