Semi-Empirical Cepheid Period-Luminosity Relations in Sloan Magnitudes

Details Semi-Empirical Cepheid Period-Luminosity Relations in Sloan Magnitudes Semi-Empirical Cepheid Period-Luminosity Relations in Sloan Magnitudes

2007-06-11

arxiv.org/abs/0706.1537v1

Astrophys.J.667:35-37,2007

Astronomy and Astrophysics

Astrophysics

4 pages, 2 tables and 2 figures, ApJ accepted

Scientific paper

10.1086/520802

In this paper we derive semi-empirical Cepheid period-luminosity (P-L) relations in the Sloan ugriz magnitudes by combining the observed BVI mean magnitudes from the Large Magellanic Cloud Cepheids (LMC) and theoretical bolometric corrections. We also constructed empirical gr band P-L relations, using the publicly available Johnson-Sloan photometric transformations, to be compared with our semi-empirical P-L relations. These two sets of P-L relations are consistent with each other.

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