8 resultados para Expansion du cumulus

em Archivo Digital para la Docencia y la Investigación - Repositorio Institucional de la Universidad del País Vasco


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Duración (en horas): De 11 a 20 horas. Nivel educativo: Grado

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Forma parte del dossier "Penser les banquets grec et romain, Entre représentations et pratiques". Actes de la table ronde Le banquet dans l'Antiquité 6 janvier 2007, Institut national d'histoire de l'art - Paris. Coordinado por Robin Nadeau

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Modernitatearen asmakuntza bat besterik ez da guk "lanak" bezala ezagutzen duguna. Lan hau ezagutzeko,burutzeko eta bakoitzaren bizitzaren muinean kokatzeko erabiltzen dugun modua asmatu izan zen; eta gero, industrialismoaren bidez orokortu egin zen

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En une génération, entre 1975 et 1995, le paysage du marché du travail auquel les jeunes font face a radicalement changé.

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LABURPENA: Ingelesaren sarrera goiztiarra ohikoa bihurtu da Euskal Autonomia Erkidegoko ikastetxeetan. Jendeak, oro har, bere eraginkortasuna defendatzen du, baina bere hedapen neurrigarriak kontrako jarrerak ere sustatu ditu. Zurrunbiloaren erdian dago haurra, ingurutik helarazten zaizkion mezuen bitartez hizkuntzekiko bere ikuspegia osatuz doalarik. Bere jarreretan eragiten duten aldagai anitzen artean irakasleek zeresan berezia dute. Hori dela eta, zenbait irakaslek ingelesaren sarrera goiztiarrarekiko duten ikuspuntua aztertzea du helburu ikerketak. Emaitzei erreparatuz, nola tutoreek hala ingeleseko irakasleek jarrera baikorra agertu duten arren, ingelesari eskaini beharko litzaiokeen denborak bereizketa argia azalerazi du. Halaber, irakasleen uste eta iritziak, zenbaitetan, ikasleen adinaren garrantzian oinarritutako sineskerietatik haratago doazela plazaratu da.

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We review the appropriateness of using SNIa observations to detect potential signatures of anisotropic expansion in the Universe. We focus on Union2 and SNLS3 SNIa datasets and use the hemispherical comparison method to detect possible anisotropic features. Unlike some previous works where nondiagonal elements of the covariance matrix were neglected, we use the full covariance matrix of the SNIa data, thus obtaining more realistic and not underestimated errors. As a matter of fact, the significance of previously claimed detections of a preferred direction in the Union2 dataset completely disappears once we include the effects of using the full covariance matrix. Moreover, we also find that such apreferred direction is aligned with the orthogonal direction of the SDSS observational plane and this suggests a clear indication that the SDSS subsample of the Union2 dataset introduces a significant bias, making the detected preferred direction unphysical. We thus find that current SNIa surveys are inappropriate to test anisotropic features due to their highly non-homogeneous angular distribution in the sky. In addition, after removal of the highest in homogeneous sub-samples, the number of SNIa is too low. Finally, we take advantage of the particular distribution of SNLS SNIa sub- sample in the SNLS3 data set, in which the observations were taken along four different directions. We fit each direction independently and find consistent results at the 1 sigma level. Although the likelihoods peak at relatively different values of Omega(m), the low number of data along each direction gives rise to large errors so that the likelihoods are sufficiently broad as to overlap within 1 sigma. (C) 2014 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license (http:// creativecommons. org/licenses/by/4.0/).