990 resultados para Gregorio X, Papa-


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EvalCOMIX es un servicio Web de autoría y despliegue de instrumentos que una vez integrado con Moodle permite el uso de dichos instrumentos para la evaluación de distintas actividades realizadas por los alumnos. La evaluación podrá ser realizada tanto por parte del docente como por parte de los propios alumnos a sí mismos o al resto de compañeros. La primera integración de esta herramienta fue realizada para la versión 1.9 de Moodle. Para la integración de la versión 2.X de Moodle se ha decidido realizar mejoras en distintos aspectos. Uno de ellos es la portabilidad de la integración, la cual depende intrínsecamente de su procedimiento de instalación.

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Contiene: Vol. 1: Tomus primus, pars prima (1843. XX, 457 p.) -- Vol. 2: Tomus primus, pars altera (1844. X, 491 p.) -- Vol. 3: Tomus secundus, pars prima (1844. VII, 525 p.) -- Vol. 4: Tomus secundus, pars altera (1844. VIII, 587 p.) -- Vol. 5: Tomus tertius, pars prima (1844. VII, 536 p.) -- Vol. 6: Tomus tertius, pars secunda (1844. IX, 734 p.) -- Vol. 7: Tomus tertius, pars tertia (1844. IX, 864 p.) -- Vol. 8: Tomus quartus, pars prima (1844. VII, 570 p.) -- Vol. 9: Tomus quartus, pars secunda (1845. VIII, 541 p.) -- Vol. 10: Tomus quintus, pars prima (1845. IX, 871 p.) -- Vol. 11: Tomus quintus, pars secunda (1845. VIII, 572 p.) -- Vol. 12: Ad jus ecclesiasticum universum indices universi primus titulorum alter rerum secundum ordinem decretalium postremus verborum (1845. 958 p.)

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Novaes completed the work through the life of Pius VI; it was continued by Vita del sommo pontifice Pio VII / E. Pistolesi.

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We present new radial velocity measurements of eight stars that were secured with the spectrograph SOPHIE at the 193 cm telescope of the Haute-Provence Observatory. The measurements allow detecting and characterizing new giant extrasolar planets. The host stars are dwarfs of spectral types between F5 and K0 and magnitudes of between 6.7 and 9.6; the planets have minimum masses Mp sin i of between 0.4 to 3.8 MJup and orbitalperiods of several days to several months. The data allow only single planets to be discovered around the first six stars (HD 143105, HIP 109600, HD 35759, HIP 109384, HD 220842, and HD 12484), but one of them shows the signature of an additional substellar companion in the system. The seventh star, HIP 65407, allows the discovery of two giant planets that orbit just outside the 12:5 resonance in weak mutual interaction. The last star, HD 141399, was already known to host a four-planet system; our additional data and analyses allow new constraints to be set on it. We present Keplerian orbits of all systems, together with dynamical analyses of the two multi-planet systems. HD 143105 is one of the brightest stars known to host a hot Jupiter, which could allow numerous follow-up studies to be conducted even though this is not a transiting system. The giant planets HIP 109600b, HIP 109384b, and HD 141399c are located in the habitable zone of their host star.

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The Body Mass Index (BMI) has been used worldwide as an indicator of fatness. However, the universal cut-off points by the World Health Organisation (WHO) classification may not be appropriate for every ethnic group when consider the relationship with their actual total body fatness(%BF). The application of population-specific classifications to assess BMI may be more relevant to public health. Ethnic differences in the BMI%BF relationship between 45 Japanese and 42 Australian-Caucasian males were assessed using whole body dual-energy X-ray absorptiometry (DXA) scan and anthropometry using a standard protocol. Japanese males had significantly (p<0.05) greater %BF at given BMI values than Australian males. When this is taken into account the newly proposed Asia-Pacific BMI classification of BMI 23 as overweight and 25 as obese may better assess the level of obesity that is associated increased health risks for this population. To clarify the current findings, further studies that compare the relationships across other Japanese populations are recommended.

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By using the Rasch model, much detailed diagnostic information is available to developers of survey and assessment instruments and to the researchers who use them. We outline an approach to the analysis of data obtained from the administration of survey instruments that can enable researchers to recognise and diagnose difficulties with those instruments and then to suggest remedial actions that can improve the measurement properties of the scales included in questionnaires. We illustrate the approach using examples drawn from recent research and demonstrate how the approach can be used to generate figures that make the results of Rasch analyses accessible to non-specialists.

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It is often postulated that an increased hip to shoulder differential angle (`X-Factor') during the early downswing better utilises the stretch-shorten cycle and improves golf performance. The current study aims to examine the potential relationship between the X-Factor and performance during the tee-shot. Seven golfers with handicaps between 0 and 10 strokes comprised the low-handicap group, whilst the high-handicap group consisted of eight golfers with handicaps between 11 and 20 strokes. The golfers performed 20 drives and three-dimensional kinematic data were used to quantify hip and shoulder rotation and the subsequent X-Factor. Compared with the low-handicap group, the high-handicap golfers tended to demonstrate greater hip rotation at the top of the backswing and recorded reduced maximum X-Factor values. The inconsistencies evident in the literature may suggest that a universal method of measuring rotational angles during the golf swing would be beneficial for future studies, particularly when considering potential injury.