The ACS Fornax Cluster Survey. V. Measurement and Recalibration of Surface Brightness Fluctuations and a Precise Value of the Fornax--Virgo Relative Distance
John P. Blakeslee, Andres Jordan, Simona Mei, Patrick Cote, Laura, Ferrarese, Leopoldo Infante, Eric W. Peng, John L. Tonry, Michael J. West

TL;DR
This paper refines the surface brightness fluctuation calibration using HST data for early-type galaxies in Fornax and Virgo, providing precise distance measurements and constraints on cosmic scatter.
Contribution
It presents a new nonlinear calibration of z-band SBF absolute magnitude and offers the first tight constraint on the cosmic variance in SBF measurements.
Findings
Fornax distance modulus is 31.51 mag, or 20.0 Mpc.
Relative distance between Fornax and Virgo is 1.214.
Cosmic scatter in SBF is constrained to 0.06 mag.
Abstract
We present g-z color and z-band surface brightness fluctuations (SBF) measurements for 43 early-type galaxies in the Fornax cluster imaged with HST/ACS. These are combined with measurements for Virgo cluster galaxies to derive a revised, nonlinear calibration of the z-band SBF absolute magnitude as a function of g-z. In all, we tabulate recalibrated SBF distances for 134 galaxies in Virgo, Fornax, the Virgo W' group, and NGC4697 in the Virgo Southern Extension. The calibration procedure yields a precise relative distance modulus for Fornax with respect to Virgo of 0.42+/-0.03 mag, or a distance ratio 1.214 +/- 0.017. The resulting Fornax distance modulus is 31.51 +/-0.03 +/-0.15 mag, 20.0 +/-0.3 +/-1.4 Mpc, where the second set of error bars reflects systematic uncertainty from our assumed Virgo distance of 16.5 Mpc. The rms distance scatter for the early-type Fornax galaxies is…
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