As in Fig. 4 but for different angular distances between the moon and target ρ. The three observations shown are from Run B at ρ = 20 (black), 45 (dark gray), and 90° (gray). The flux values for ρ = 20° were shifted up by 2000 and for ρ = 45° by 1000 phot s−1 m−2 μm−1 arcsec−2 for clarity.
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