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Biased Data Selection in Mars Effect Research

Suitbert Ertel, Institut für Psychologie, Gosslerstr. 14, 37073 Göttingen, Germany

Kenneth Irving, 596 Villa Ave., Staten Island, NY 10302, U.S.A.

An earlier study (Ertel, 1988) showed that original evidence for Gauquelin's Mars effect with eminent athletes (Gauquelin and Gauqelin 1970) was based on an incomplete data sample. When athletes initially discarded by Gauquelin were included the Mars effe ct declined. The present study bears on a more subtle effect of the same bias. Gauquelin's original definition of planetary effects was based on birth frequences obtained in a "narrow" zone of the planet's daily circle (G-sector zone). After accumulating results over decades of research, he found that the area just preceding his narrow zone indicated initial planetary effects; he therefore proposed to include initial sectors in an "extended" G-sector zone definition. Assuming that these initial G-sectors had been ignored prior to 1984, the authors suspected that an unbiased proportion of births for these sectors in Gauquelin's exempted data should contrast with the biased proportion known to exist in the "narrow-zone" sectors. This idea gave rise to a new bias detector (IMQ, initial vs. main sector quotient), whose validity was confirmed with the biased Gauquelin data. Selection bias for Gauquelin turned up in his athletes study only; the IMQ did not indicate like anomalies for six other professional inve stigations conducted by Gauquelin. The IMQ was also applied to three athlete samples collected by skeptic organizations. Among them, the CSICOP data for U.S. athletes revealed an anomalous IMQ similar to Gauquelin's unpublished athletes. The results therefore suggest that a certain proport ion of U.S. athletes with unwelcome positions might have been exempted from analysis (p = 0.01). Support for this suspicion is provided by complementary evidence indicating biased admissions of less eminent athletes to the U.S. sample while the preference for most eminent athletes was required. Thus an avoidance of G-sector cases, consistent with this bent, cannot be disavowed. Nevertheless the authors refrain from firm conclusions as this case is circumstantial. It is suggested to merely disregard the CSICOP's negative result of their study in future discussions of the Mars effect as long as appropriate steps to convincingly resolve remaining ambiguities have not been not made.

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