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On the fluctuations of the surface brightness of galaxies [PDF]

Astrophysics and Space Science, 1988
We consider the problem of correlation between the surface brightnesses of two nearby points for an external galaxy under certain simplifying assumptions. A probability density function for these intensities are derived, as are its moments and correlation coefficient.
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An Update on the Hubble Constant from Surface Brightness Fluctuations

The surface brightness fluctuation (SBF) method is a powerful way to measure distances to evolved galaxies without recent star formation. We have published a value of the Hubble constant using WFC3/IR to measure distances out to 100 Mpc, tied indirectly to a Cepheid calibration.
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Investigating Resolved Stellar Populations with Surface Brightness Fluctuations.

2006
Raimondo, G., Brocato, E., Cantiello, M., CAPACCIOLI, MASSIMO   +3 more
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Surface Brightness Fluctuations as a Probe of Stellar Populations

1994
Richter, G. M., Böhm, P., CAPACCIOLI, MASSIMO, LONGO, GIUSEPPE, Lorentz, H.   +4 more
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