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The ACS Fornax Cluster Survey V Measurement and Recalibration of Surface Brightness Fluctuations and a Precise Value of the Fornax Virgo Relative Distance

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Figure 2. Mean SBF z 850 magnitude vs. (g 475 −z 850 ) color for the 43 ACSFCS galaxies
Figure 3 displays the (g 475 −z 850 ) histogram for the total sample of 128 galaxies in Fornax and Virgo (omitting the more distant W  galaxies) with SBF measurements from the present work and from ACSVCS-XIII, respectively
Figure 4. Reduced χ 2 as a function of the relative Fornax–Virgo dis- dis-tance modulus Δ(m−M) FV for a second-order polynomial fit to the  com-bined z 850 −(g 475 −z 850 ) relation for 118 Fornax and Virgo galaxies with (g 475 −z 850 ) > 1.02 (gray cir
Table 2 (Continued) Galaxy (g −z) m z (m −M) d B T Name (1) (2) (3) (4) (5) (6) (7) VCC1664 1.421 ± 0.014 29.188 ± 0.021 31.013 ± 0.071 15.9 ± 0.5 12.0 NGC4564 VCC1692 1.421 ± 0.014 29.343 ± 0.020 31.168 ± 0.071 17.1 ± 0.6 11.8 NGC4570 VCC1695 1.055 ± 0.01
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