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    Ultraviolet Number Counts of Galaxies from Swift Ultraviolet/Optical Telescope Deep Imaging of the Chandra Deep Field South

    Access Status
    Fulltext not available
    Authors
    Hoversten, E.
    Gronwall, C.
    Vanden Berk, D.
    Koch, T.
    Breeveld, A.
    Curran, Peter
    Hinshaw, D.
    Marshall, F.
    Roming, P.
    Siegel, M.
    Still, M.
    Date
    2009
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Hoversten, E. and Gronwall, C. and Vanden Berk, D. and Koch, T. and Breeveld, A. and Curran, P. and Hinshaw, D. et al. 2009. Ultraviolet Number Counts of Galaxies from Swift Ultraviolet/Optical Telescope Deep Imaging of the Chandra Deep Field South. The Astrophysical Journal. 705: pp. 1462-1468.
    Source Title
    The Astrophysical Journal
    Additional URLs
    http://iopscience.iop.org/0004-637X/705/2/1462/pdf/apj_705_2_1462.pdf
    ISSN
    0004-637X
    URI
    http://hdl.handle.net/20.500.11937/41331
    Collection
    • Curtin Research Publications
    Abstract

    Deep Swift UV/Optical Telescope (UVOT) imaging of the Chandra Deep Field South is used to measure galaxynumber counts in three near-ultraviolet (NUV) filters (uvw2: 1928 Å, uvm2: 2246 Å, and uvw1: 2600 Å) and the uband (3645 Å). UVOT observations cover the break in the slope of the NUV number counts with greater precisionthan the number counts by the Hubble Space Telescope Space Telescope Imaging Spectrograph and the GalaxyEvolution Explorer, spanning a range 21 mAB 25. Model number counts confirm earlier investigations infavoring models with an evolving galaxy luminosity function.

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