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( J. C. Kim ),( Patricia Seitz ),( Li-shiue Gau ),( Kyoung Tae Kim ),( Eunkyun Park ) 한국체육학회 2020 International journal of human movement science Vol.14 No.2
This qualitative study is to explore the meaning of having a female coach for a male team. Along with various secondary data, first-hand experiences of hiring managers who have previously hired female coaches for male teams were used. Four male athletic directors from high schools located in the U.S. Northeast region were interviewed, and a cross-case analysis method was adopted for tagging data and determining themes. Four primary themes emerged: 1) Prior experiences with a female coach when being an athlete or a coach influence the perceived meaning of seeing a female coach for a male team; 2) It was emphasized to hire the most qualified candidate for the job, with gender not being a crucial criteria in the hiring process; 3) Organizational work environment existed hidden obstacles that a female coach for a male team would face; and 4) Nevertheless, females were encouraged to apply for coaching positions on male teams if they met the qualifications. Regardless of gender, the most desirable candidates possessing professional qualifications and knowledge should be hired. This study concluded that the trend for a low percentage of female applicants for male teams needs to be improved and thus to enhance gender diversity.
Shin, I.-G.,Udalski, A.,Han, C.,Gould, A.,Dominik, M.,Fouqué,, P.,Kubiak, M.,Szymań,ski, M. K.,Pietrzyń,ki, G.,Soszyń,ski, I.,Ulaczyk, K.,Wyrzykowski, Ł.,DePoy, D. L.,Dong, S.,Gau IOP Publishing 2011 The Astrophysical journal Vol.735 No.2
<P>We present the result of the analysis of the gravitational binary-lensing event OGLE-2005-BLG-018. The light curve of the event is characterized by two adjacent strong features and a single weak feature separated from the strong features. The light curve exhibits noticeable deviations from the best-fit model based on standard binary parameters. To explain the deviation, we test models including various higher-order effects of the motions of the observer, source, and lens. From this, we find that it is necessary to account for the orbital motion of the lens in describing the light curve. From modeling the light curve considering the parallax effect and Keplerian orbital motion, we are able to not only measure the physical parameters but also to find a complete orbital solution of the lens system. It is found that the event was produced by a binary lens located in the Galactic bulge with a distance of 6.7 +/- 0.3 kpc from the Earth. The individual lens components with masses 0.9 +/- 0.3 M-circle dot and 0.5 +/- 0.1 M-circle dot are separated with a semi-major axis of a = 2.5 +/- 1.0 AU and orbiting each other with a period P = 3.1 +/- 1.3 yr. This event demonstrates that it is possible to extract detailed information about binary lens systems from well-resolved lensing light curves.</P>