The occulting galaxy pair UGC 3995 - Dust properties from HST and CALIFA data

B. W. Holwerda; W. C. Keel

doi:10.1051/0004-6361/201321455

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Volume 556 (August 2013)

A&A, 556 (2013) A42

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Fig. 4

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Distribution of A_V values in the green aperture in Figs. 1 or 2. The dashed line is an exponential drop fit to the values beyond A_V = 0.5. Above this value, the distribution of pixels with is well described by N = N₀ × e^{(− A_V/0.5)} with N₀ = 6799 pixels.

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