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• W2102440976 abstract "Context.The surface brightness fluctuation (SBF) method is a powerful tool for deriving distances to galaxies for which single stars cannot be resolved. Up to now, the method has been calibrated mainly at red colours due to the intrinsic faintness of blue early-type galaxies." @default.
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• W2102440976 date "2006-09-12" @default.
• W2102440976 modified "2023-09-27" @default.
• W2102440976 title "An <i><b>I</b></i>-band calibration of surface brightness fluctuation measurements at blue colours" @default.
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• W2102440976 doi "https://doi.org/10.1051/0004-6361:20054685" @default.
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