107 resultados para Riz


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Monogr??fico con el t??tulo: "Formaci??n del profesorado en el Espacio Europeo de Educaci??n Superior"

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La finalidad de estas propuesta curriculares es facilitar que las escuelas encuentren elementos para sustentar un trabajo m??s organizado y eficaz para la ense??anza de la Lengua de Signos Espa??ola (LSE) y que se compartan experiencias entre los profesionales as?? como contribuir a poner en pr??ctica m??todos de ense??anza y aprendizaje mejores. Estas propuestas curriculares cobran especial relevancia en los centros biling??es que as?? lo recogen en sus proyectos educativos y ling????sticos, que observan principios b??sicos como el mismo estatus para las dos lenguas, y profesionales sordos y oyentes como referentes ling????sticos y culturales de cada una de las lenguas. En estos centros el fin educativo que se pretende es que el alumnado sordo adquiera buenas competencias en las dos lenguas para asegurar el aprendizaje de todo tipo de contenidos curriculares. Cuando se considera la LSE como un ??rea curricular se garantiza un compromiso real respecto a la asignaci??n de tiempos espacios y recursos personales y materiales en los centros en los que se imparte.

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Linguistic palaeontology permits the identification of two language families whose linguistic ancestors pose the likeliest candidates for the original domesticators of rice, viz. Hmong-Mien and Austroasiatic. In the 2009 model, the ancient Hmong-Mien was identified as the primary domesticators of Asian rice, and the ancient Austroasiatics as the secondary domesticators. Recent rice genetic research leads to the modification of this model for rice domestication, but falls short of identifying the original locus of rice domestication. At the same time, the precise whereabouts of the Austroasiatic homeland remains disputed. Linguistic evidence unrelated to rice agriculture has been adduced to support a southern homeland for Austroasiatic somewhere within the Bay of Bengal littoral. The implications of new rice genetic research are discussed, the linguistic palaeontological evidence is reassessed, and an enduring problem with the archaeology of rice agriculture is highlighted.

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The EVI1 gene, located at chromosome band 3q26, is overexpressed in some myeloid leukemia patients with breakpoints either 5' of the gene in the t(3;3)(q21;q26) or 3' of the gene in the inv(3)(q21q26). EVI1 is also expressed as part of a fusion transcript with the transcription factor AML1 in the t(3;21)(q26;q22), associated with myeloid leukemia. In cells with t(3;21), additional fusion transcripts are AML1-MDS1 and AML1-MDS1-EVI1. MDS1 is located at 3q26 170-400 kb upstream (telomeric) of EVI1 in the chromosomal region in which some of the breakpoints 5' of EVI1 have been mapped. MDS1 has been identified as a single gene as well as a previously unreported exon(s) of EVI1 We have analyzed the relationship between MDS1 and EVI1 to determine whether they are two separate genes. In this report, we present evidence indicating that MDS1 exists in normal tissues both as a unique transcript and as a normal fusion transcript with EVI1, with an additional 188 codons at the 5' end of the previously reported EVI1 open reading frame. This additional region has about 40% homology at the amino acid level with the PR domain of the retinoblastoma-interacting zinc-finger protein RIZ. These results are important in view of the fact that EVI1 and MDS1 are involved in leukemia associated with chromosomal translocation breakpoints in the region between these genes.

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Includes bibliographical references.

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Mode of access: Internet.

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Mode of access: Internet.

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Microfilm.

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We present optical, near-IR, and radio follow-up of 16 Swift bursts, including our discovery of nine afterglows and a redshift determination for three. These observations, supplemented by data from the literature, provide an afterglow recovery rate of 52% in the optical/near-IR, much higher than in previous missions (BeppoSAX, HETE-2, INTEGRAL, and IPN). The optical/near-IR afterglows of Swift events are on average 1.8 mag fainter at t = 12 hr than those of previous missions. The X-ray afterglows are similarly fainter than those of pre-Swift bursts. In the radio the limiting factor is the VLA threshold, and the detection rate for Swift bursts is similar to that for past missions. The redshift distribution of pre-Swift bursts peaked at z similar to 1, whereas the six Swift bursts with measured redshifts are distributed evenly between 0.7 and 3.2. From these results we conclude that ( 1) the pre-Swift distributions were biased in favor of bright events and low-redshift events, ( 2) the higher sensitivity and accurate positions of Swift result in a better representation of the true burst redshift and brightness distributions ( which are higher and dimmer, respectively), and (3) similar to 10% of the bursts are optically dark, as a result of a high redshift and/or dust extinction. We remark that the apparent lack of low-redshift, low-luminosity Swift bursts and the lower event rate than prelaunch estimates ( 90 vs. 150 per year) are the result of a threshold that is similar to that of BATSE. In view of these inferences, afterglow observers may find it advisable to make significant changes in follow-up strategies of Swift events. The faintness of the afterglows means that large telescopes should be employed as soon as the burst is localized. Sensitive observations in RIz and near-IR bands will be needed to discriminate between a typical z similar to 2 burst with modest extinction and a high-redshift event. Radio observations will be profitable for a small fraction (similar to 10%) of events. Finally, we suggest that a search for bright host galaxies in untriggered BAT localizations may increase the chance of finding nearby low-luminosity GRBs.