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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 6.

Galaxy number counts in the UVOT u filter (red triangles). U number counts from Capak et al. (2004; green diamonds), Eliche-Moral et al. (2006; blue X's), and Metcalfe et al. (2001; black circles), as well as SDSS u number counts from Yasuda et al. (2001; cyan plus signs) are also plotted with a conversion to the UVOT u filter as described in the text. Yasuda et al. (2001) and Metcalfe et al. (2001) do not tabulate their errors. Model number counts are also plotted for a starburst template galaxy and Calzetti et al. (1994) dust model with A V = 1, and galaxy luminosity function parameters from Ilbert et al. (2005) are shown in black for non-evolving (solid line) and an evolving (dashed line) galaxy luminosity functions. 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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