= On the Use of Trigonometric Parallaxes for the Calibration of Luminosity Systems: Theory by T. E. Lutz and D. H. Kelker
{c}
{tag=Work by T. E. Lutz}
{tag=Work by D. H. Kelker}
{title2=1973}
https://doi.org/10.1086/129506
PASP 85, 573–578. Primary classical treatment of parallax-based <luminosity> <calibration> under a spatial-population model. Its assumptions do not justify a universal correction to every modern individual-star distance inference. Bibliographic details are also verified in the references of <An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent by G. Pietrzyński and others>.
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