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A population of faint low surface brightness galaxies in the Perseus cluster core

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Figure

Figure 1. Deep view of the Perseus cluster core. Left: V -band mosaic. The image dimensions are 0.58◦(=ˆ 0.71 Mpc at 72.3 Mpc) ineast-west and north-south direction
Figure 2. Detection rates of visually identified model galaxies astion rates are based on 30-40 models of one type, with the samehalf-light radius and magnitude, but varying ellipticity and thussurface brightness, that were inserted into one copy of the mo-
Table 1. Coordinates and structure parameters of faint LSB galaxy candidates in the Perseus cluster core.for Galactic foreground extinction
Table 1 – continued
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