An I-band calibration of the SBF method at blue colours
12S.Mieskeetal.:SBFcalibrationatbluecolours
asingleonewithsomeuniformscatter.We ndevidencethatthefaintergalaxiesinoursamplesexhibityoungerinte-gratedagesandhighermetallicitiesthanthebrightergalax-ies.
–FromapurelyempiricalSBFcalibration(relation
5)wede-ducea0.34±0.14magcosmicscatterof
MItobemoresensitivetodi erentage/metallicity
combinationsinbluecoloursthanatredcolours.
–ApplyingtheempiricalcalibrationtotheSBFmeasure-mentsofHydraandCentaurusclusterdEsfromMieske&Hilker(2003b)andMieskeetal.(2005)hasnoe ectontherelativeSBFdistanceofbothgalaxyclusters.Alsotheabsolutedistancesdonotrequirecorrection.
Acknowledgements.Wethanktheanonymousrefereeforhiscom-mentsandsuggestionswhichhelpedtoimprovethepaper.Weowethankstothesta atLasCampanasObservatoryfortheirassistanceincarryingouttheobservations.SMacknowledgessupportbyDFGprojectHI855/1andDAADPh.D.grantKennzi erD/01/35298.LIwassupportedbyFONDAP“CenterforAstrophysics”.
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