39,484 research outputs found
Web-based Gene Pathogenicity Analysis (WGPA): a web platform to interpret gene pathogenicity from personal genome data
UNLABELLED: As the volume of patient-specific genome sequences increases the focus of biomedical research is switching from the detection of disease-mutations to their interpretation. To this end a number of techniques have been developed that use mutation data collected within a population to predict whether individual genes are likely to be disease-causing or not. As both sequence data and associated analysis tools proliferate, it becomes increasingly difficult for the community to make sense of these data and their implications. Moreover, no single analysis tool is likely to capture all relevant genomic features that contribute to the gene's pathogenicity. Here, we introduce Web-based Gene Pathogenicity Analysis (WGPA), a web-based tool to analyze genes impacted by mutations and rank them through the integration of existing prioritization tools, which assess different aspects of gene pathogenicity using population-level sequence data. Additionally, to explore the polygenic contribution of mutations to disease, WGPA implements gene set enrichment analysis to prioritize disease-causing genes and gene interaction networks, therefore providing a comprehensive annotation of personal genomes data in disease. AVAILABILITY AND IMPLEMENTATION: wgpa.systems-genetics.net
On the harmonicity of normal almost contact metric structures
We consider normal almost contact structures on a Riemannian manifold and,
through their associated sections of an ad-hoc twistor bundle, study their
harmonicity, as sections or as maps. We rewrite these harmonicity equations in
terms of the Riemann curvature tensor and find conditions relating the
harmonicity of the almost contact and almost complex structures of the total
and base spaces of the Morimoto fibration.Comment: 14 page
Informal Referrals, Employment and Wages: Seeking Causal Directions
Employers and job seekers rely extensively on job informational networks to fill vacancies or to find a job. The widespread use of job contacts to find work has been largely associated with labor outcomes, such as finding a job or even affecting wages. Some scholars have claimed that informal referrals play a determinant role in reducing informational mismatches between potential employers and job seekers. Although several studies have shown that the use of friends and relatives is correlated with labor outcomes, little is known about the causal effect. In this article, I aim to identify whether there is a causal effect of using informal referrals on two main outcomes: the probability of being employed and hourly wages. I use a large data set from Colombia, the Living Standard Survey 2003, to contrast the results from three main methodologies: standard OLS estimation, propensity-score matching, and instrumental variables. Results suggest that much of the positive effect of using informal referrals on employment reflects the prevalence of informal-sector jobs to be filled through this method rather than a causal effect. On the contrary, the results for hourly wages suggest a negative causal effect of using job informational networks, which is explained by the low-quality/poor matches theory. Yet, this is only true in formal-sector firms.informal referrals, job search methods, employment rates, hourly wages, selec- tion bias, OLS, Propensity-Score Matching, Instrumental Variables, Roy Model
A search for brown-dwarf like secondaries in cataclysmic variables
We present VTL/ISAAC infrared spectroscopy of a sample of short orbital
period cataclysmic variables which are candidates for harboring substellar
companions. We have detected the KI and NaI absorption lines of the companion
star in VY Aqr. The overall spectral distribution in this system is best fit
with a M9.5 type dwarf spectra, implying a distance of pc. VY Aqr
seems to fall far from the theoretical distribution of secondary star
temperatures around the orbital period minimum. Fitting of the IR spectral
energy distribution (SED) was performed by comparing the observed spectrum with
late-type templates. The application of such a spectral fitting procedure
suggests that the continuum shape in the 1.1-2.5 m spectral region in
short orbital period cataclysmic variables may be an useful indicator of the
companion spectral type. The SED fitting for RZ Leo and CU Vel suggests M5 type
dwarf companions, and distances of 340 110 and 150 50 pc,
respectively. These systems may be placed in the upper evolution branch for
short period cataclysmic variables.Comment: accepted for publication in MNRAS, 6 pages, 7 figure
An empirical calibration of nebular abundances based on the sulphur emission lines
We present an empirical calibration of nebular abundances based on the strong
emission lines of [SII] and [SIII] in the red part of the spectrum through the
definition of a sulphur abundance parameter S23. This calibration presents two
important advantages against the commonly used one based on the optical oxygen
lines: it remains single-valued up to abundances close to solar and is rather
independent of the degree of ionization of the nebula.Comment: 10 pages, 8 figures. Accepted for publication in MNRA
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