University of Geneva

About: University of Geneva is a education organization based out in Geneva, Switzerland. It is known for research contribution in the topics: Population & Planet. The organization has 26887 authors who have published 65265 publications receiving 2931373 citations. The organization is also known as: Geneva University & Universite de Geneve.

The endocytic pathway: a mosaic of domains

Abstract: Organelles in the endocytic pathway are composed of a mosaic of structural and functional regions. These regions consist, at least in part, of specialized protein-lipid domains within the plane of the membrane, or of protein complexes associated with specific membrane lipids. Whereas some of these molecular assemblies can be found in more than one compartment, a given combination seems to be unique to each compartment, indicating that membrane organization might be modular.

Enhancement of structural preservation and immunocytochemical staining in low temperature embedded pancreatic tissue.

Abstract: The recently developed low temperature embedding procedure with the resin Lowicryl K4M (Carlemalm E, Garavito M, Villiger W: Proc 7th Eur Cong Electron Microsc, 1980, p 656; Garavito M, Carlemalm E, Villiger W: Proc 7th Eur Cong Electron Microsc, 1980, p 658) was tested for its suitability for embedding of glutaraldehyde-fixed rat pancreatic tissue and for postembedding staining of thin sections with the protein A-gold (pAg) technique (Roth J, Bendayan M, Orci L: J Histochem Cytochem 26:1074, 1978) for amylase. Compared to conventional Epon embedding of glutaraldehyde fixed tissue, the low temperature embedding method with Lowicryl K4M resulted in a superior preservation of the general cellular fine structure, particularly in the Golgi apparatus. For low temperature embedded tissue, the quantitative evaluation of the immunocytochemical labeling for amylase showed a more specific staining of the rough endoplasmic reticulum, the Golgi apparatus, and the zymogen granules. This was due to a significant loweri...

Mutagenic deamination of cytosine residues in DNA.

Abstract: Spontaneous deamination converts cytosine to uracil, which is excised from DNA by the enzyme uracil-DNA glycosylase, leading to error-free repair. 5-Methylcytosine residues are deaminated to thymine, which cannot be excised and repaired by this system. As a result, 5-methylcytosine residues are hotspots for spontaneous transitions, as demonstrated in the lacI gene of Escherichia coli. We show here that in bacteria which lack uracil-DNA glycosylase (Ung-) and cannot excise uracil residues from DNA, the rate of spontaneous transition at cytosine residues is raised to the hotspot rate at 5-methylcytosine residues. These studies provide direct evidence that the deamination of cytosine is a significant source of spontaneous mutations.

Roads to turbulence in dissipative dynamical systems

Abstract: Three scenarios leading to turbulence in theory and experiment are outlined. The respective mathematical theories are explained and compared.

Gaia Data Release 1 - Astrometry: one billion positions, two million proper motions and parallaxes

Abstract: Gaia Data Release 1 (Gaia DR1) contains astrometric results for more than 1 billion stars brighter than magnitude 20.7 based on observations collected by the Gaia satellite during the first 14 months of its operational phase. We give a brief overview of the astrometric content of the data release and of the model assumptions, data processing, and validation of the results. For stars in common with the Hipparcos and Tycho-2 catalogues, complete astrometric single-star solutions are obtained by incorporating positional information from the earlier catalogues. For other stars only their positions are obtained by neglecting their proper motions and parallaxes. The results are validated by an analysis of the residuals, through special validation runs, and by comparison with external data. Results. For about two million of the brighter stars (down to magnitude ~11.5) we obtain positions, parallaxes, and proper motions to Hipparcos-type precision or better. For these stars, systematic errors depending e.g. on position and colour are at a level of 0.3 milliarcsecond (mas). For the remaining stars we obtain positions at epoch J2015.0 accurate to ~10 mas. Positions and proper motions are given in a reference frame that is aligned with the International Celestial Reference Frame (ICRF) to better than 0.1 mas at epoch J2015.0, and non-rotating with respect to ICRF to within 0.03 mas/yr. The Hipparcos reference frame is found to rotate with respect to the Gaia DR1 frame at a rate of 0.24 mas/yr. Based on less than a quarter of the nominal mission length and on very provisional and incomplete calibrations, the quality and completeness of the astrometric data in Gaia DR1 are far from what is expected for the final mission products. The results nevertheless represent a huge improvement in the available fundamental stellar data and practical definition of the optical reference frame.