School counselor role in student success workshop

Includes bibliographical references (leaves 38-39)A workshop for principals, school administrators, and teachers has been created in an effort to assist with the clarification of the various roles of professional school counselors. The purpose of this graduate project is to develop a workshop that may be utilized by professional school counselors to describe counselor responsibilities to their school's faculty and staff. (See more in text.

Trans-splicing of the mod(mdg4) Complex Locus Is Conserved Between the Distantly Related Species Drosophila melanogaster and D. virilis

The modifier of mdg4, mod(mdg4), locus in Drosophila melanogaster represents a new type of complex gene in which functional diversity is resolved by mRNA trans-splicing. A protein family of >30 transcriptional regulators, which are supposed to be involved in higher-order chromatin structure, is encoded by both DNA strands of this locus. Mutations in mod(mdg4) have been identified independently in a number of genetic screens involving position-effect variegation, modulation of chromatin insulators, apoptosis, pathfinding of nerve cells, and chromosome pairing, indicating pleiotropic effects. The unusual gene structure and mRNA trans-splicing are evolutionary conserved in the distantly related species Drosophila virilis. Chimeric mod(mdg4) transcripts encoded from nonhomologous chromosomes containing the splice donor from D. virilis and the acceptor from D. melanogaster are produced in transgenic flies. We demonstrate that a significant amount of protein can be produced from these chimeric mRNAs. The evolutionary and functional conservation of mod(mdg4) and mRNA trans-splicing in both Drosophila species is furthermore demonstrated by the ability of D. virilis mod(mdg4) transgenes to rescue recessive lethality of mod(mdg4) mutant alleles in D. melanogaster

Performance of Seven Commercial Phytases in an in Vitro Simulation of Poultry Digestive Tract

The aim of,this study was to compare the biochemical, properties of seven commercially, available phytase products as well as their catalytic performance in an in vitro simulation of the digestive tract of poultry. Their enzymatic properties relevant with respect to phytate dephosphorylation in the digestive tract of birds were determined under identical assay conditions. All phytase-products included in the study showed an acid pH optimum of activity and were capable of releasing the organically bound phosphate from phytate during the in vitro simulation. However, their overall biochemical properties and relative catalytic performances were remarkably different The in vitro degradation system was considered as a simple and useful tool to evaluate the suitability of a phytase to be used as a feed supplement. Although relevant factors such as dietary P levels, intestinal phytase, and P absorption ate not implemented in the system, this approach might help to reduce the number of feeding trials necessary in the, search for a better Suited phytase for animal feeding application

Integrative genome analyses identify key somatic driver mutations of small-cell lung cancer

Small-cell lung cancer (SCLC) is an aggressive lung tumor subtype with poor prognosis. We sequenced 29 SCLC exomes, 2 genomes and 15 transcriptomes and found an extremely high mutation rate of 7.4 ± 1 protein-changing mutations per million base pairs. Therefore, we conducted integrated analyses of the various data sets to identify pathogenetically relevant mutated genes. In all cases, we found evidence for inactivation of TP53 and RB1 and identified recurrent mutations in the CREBBP, EP300 and MLL genes that encode histone modifiers. Furthermore, we observed mutations in PTEN, SLIT2 and EPHA7, as well as focal amplifications of the FGFR1 tyrosine kinase gene. Finally, we detected many of the alterations found in humans in SCLC tumors from Tp53 and Rb1 double knockout mice. Our study implicates histone modification as a major feature of SCLC, reveals potentially therapeutically tractable genomic alterations and provides a generalizable framework for the identification of biologically relevant genes in the context of high mutational background

The PLATO Mission

International audiencePLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large number of stars. PLATO will detect small planets (down to <2 R_(Earth)) around bright stars (<11 mag), including terrestrial planets in the habitable zone of solar-like stars. With the complement of radial velocity observations from the ground, planets will be characterised for their radius, mass, and age with high accuracy (5 %, 10 %, 10 % for an Earth-Sun combination respectively). PLATO will provide us with a large-scale catalogue of well-characterised small planets up to intermediate orbital periods, relevant for a meaningful comparison to planet formation theories and to better understand planet evolution. It will make possible comparative exoplanetology to place our Solar System planets in a broader context. In parallel, PLATO will study (host) stars using asteroseismology, allowing us to determine the stellar properties with high accuracy, substantially enhancing our knowledge of stellar structure and evolution. The payload instrument consists of 26 cameras with 12cm aperture each. For at least four years, the mission will perform high-precision photometric measurements. Here we review the science objectives, present PLATO's target samples and fields, provide an overview of expected core science performance as well as a description of the instrument and the mission profile at the beginning of the serial production of the flight cameras. PLATO is scheduled for a launch date end 2026. This overview therefore provides a summary of the mission to the community in preparation of the upcoming operational phases

The PLATO Mission

International audiencePLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large number of stars. PLATO will detect small planets (down to <2 R_(Earth)) around bright stars (<11 mag), including terrestrial planets in the habitable zone of solar-like stars. With the complement of radial velocity observations from the ground, planets will be characterised for their radius, mass, and age with high accuracy (5 %, 10 %, 10 % for an Earth-Sun combination respectively). PLATO will provide us with a large-scale catalogue of well-characterised small planets up to intermediate orbital periods, relevant for a meaningful comparison to planet formation theories and to better understand planet evolution. It will make possible comparative exoplanetology to place our Solar System planets in a broader context. In parallel, PLATO will study (host) stars using asteroseismology, allowing us to determine the stellar properties with high accuracy, substantially enhancing our knowledge of stellar structure and evolution. The payload instrument consists of 26 cameras with 12cm aperture each. For at least four years, the mission will perform high-precision photometric measurements. Here we review the science objectives, present PLATO's target samples and fields, provide an overview of expected core science performance as well as a description of the instrument and the mission profile at the beginning of the serial production of the flight cameras. PLATO is scheduled for a launch date end 2026. This overview therefore provides a summary of the mission to the community in preparation of the upcoming operational phases