Figure 5 from Ultraviolet Number Counts of Galaxies from Swift Ultraviolet/Optical Telescope Deep Imaging of the Chandra Deep Field South

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

Authors: E. A. Hoversten, C. Gronwall, D. E. Vanden Berk, T. S. Koch, A. A. Breeveld, P. A. Curran, D. A. Hinshaw, F. E. Marshall, P. W. A. Roming, M. H. Siegel, and M. Still

HOVERSTEN et al. 2009 The Astrophysical Journal 705 1462.

Provider: AAS Journals

Caption: Figure 5.

UV number counts in the uvw1 filter (red triangles). In addition to the description from Figure 3, model number counts assuming the cosmic spectrum of Baldry et al. (2002) as a template are shown in red for both non-evolving (solid line) and evolving (dashed line) luminosity functions.

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