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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 1.

Field of view for UVOT CDF-S observations. Contours indicate the area covered with at least 98% of the maximum exposure time as described in the text and tabulated in Table 1. The contours are uvw2 (thin solid line), uvm2 (dotted line), uvw1 (dashed line), and u (dot-dashed line). For reference, the extent of the CDF-S (Giacconi et al. 2002), Hubble Ultra Deep Field (Beckwith et al. 2006), and Great Observatories Origins Deep Survey (Giavalisco et al. 2004) are denoted by thick contours which are labeled.

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