Terracota, Arquitectura y Barcelona: siglos XIX y XX

Creemos que la terracota, en cuanto que materia, posee sufi cientes cualidades, por sí mismay por su vinculación con la arquitectura en la que se ubica, que la hacen merecedora de unestudio profundo y de un acercamiento respetuoso. Un producto cerámico que aporta comopropiedad fundamental su carácter escultórico. Valores que pretendemos sean totalmente explícitos, con la condición que sean fácilmente reconocibles. Un material que defi ne un momento de la historia y de la historia de la arquitectura de Barcelona, incompleta sin el estudio sistemático que presentamos.

Terracota, Arquitectura y Barcelona: siglos XIX y XX

Creemos que la terracota, en cuanto que materia, posee sufi cientes cualidades, por sí mismay por su vinculación con la arquitectura en la que se ubica, que la hacen merecedora de unestudio profundo y de un acercamiento respetuoso. Un producto cerámico que aporta comopropiedad fundamental su carácter escultórico. Valores que pretendemos sean totalmente explícitos, con la condición que sean fácilmente reconocibles. Un material que defi ne un momento de la historia y de la historia de la arquitectura de Barcelona, incompleta sin el estudio sistemático que presentamos.

La crítica antieclesiástica en La Lozana Andaluza.

Se analiza cómo Alberti aprovecha la crítica velada de Francisco Delicado, autor de 'La Lozana Andaluza' para hacer referencia a hechos recientes de la historia de España y hacer más obvia la crítica anticlerical.

GALAXIES BEHIND THE GALACTIC PLANE: FIRST RESULTS AND PERSPECTIVES FROM THE VVV SURVEY

VISTA Variables in the Via Lactea (VVV) is an ESO variability survey that is performing observations in near-infrared bands (ZY JHK(s)) toward the Galactic bulge and part of the disk with the completeness limits at least 3 mag deeper than Two Micron All Sky Survey. In the present work, we searched in the VVV survey data for background galaxies near the Galactic plane using ZY JHK(s) photometry that covers 1.636 deg(2). We identified 204 new galaxy candidates by analyzing colors, sizes, and visual inspection of multi-band (ZY JHK(s)) images. The galaxy candidate colors were also compared with the predicted ones by star count models considering a more realistic extinction model at the same completeness limits observed by VVV. A comparison of the galaxy candidates with the expected one by Millennium simulations is also presented. Our results increase the number density of known galaxies behind the Milky Way by more than one order of magnitude. A catalog with galaxy properties including ellipticity, Petrosian radii, and ZY JHK(s) magnitudes is provided, as well as comparisons of the results with other surveys of galaxies toward the Galactic plane.

Lobelia fulgens Queen Victoria eine dankbare Fenster- und Gartenblume

Von A. Sliwa

Calmness of the Feasible Set Mapping for Linear Inequality Systems

In this paper we deal with parameterized linear inequality systems in the n-dimensional Euclidean space, whose coefficients depend continuosly on an index ranging in a compact Hausdorff space. The paper is developed in two different parametric settings: the one of only right-hand-side perturbations of the linear system, and that in which both sides of the system can be perturbed. Appealing to the backgrounds on the calmness property, and exploiting the specifics of the current linear structure, we derive different characterizations of the calmness of the feasible set mapping, and provide an operative expresion for the calmness modulus when confined to finite systems. In the paper, the role played by the Abadie constraint qualification in relation to calmness is clarified, and illustrated by different examples. We point out that this approach has the virtue of tackling the calmness property exclusively in terms of the system’s data.