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arXiv · astro-ph/9310029

Optimal Galaxy Distance Estimators

Martin A. Hendry·John F. L. Simmons
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Abstract

The statistical properties of galaxy distance estimators are studied and a rigorous framework is developed for identifying and removing the effects of Malmquist bias due to obsevational selection. The prescription of Schechter (1980) for defining unbiased distance estimators is extended to more general -- and more realistic -- cases. The derivation of `optimal' unbiased distance estimators of minimum dispersion, by utilising information from additional -- suitably correlated -- observables, is discussed and the results applied to a calibrating sample from the Fornax cluster, as used in the Mathewson spiral galaxy redshift survey. The optimal distance estimator derived from I-band magnitude, diameter and 21cm line width has an intrinsic scatter which is 25 \% smaller than that of the Tully-Fisher relation quoted for this calibrating sample. (Figures are available on request).

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Martin A. Hendry, John F. L. Simmons. 1993-10-14. Optimal Galaxy Distance Estimators. https://doi.org/10.1086/174832

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