Los imaginarios sociales sobre el infierno en la pintura de Hernando de la Cruz, 1629

En 1629, Hernando de la Cruz, guía espiritual de Mariana de Jesús, pintó para la iglesia jesuítica de Quito un cuadro de gran formato sobre el Infierno. El lienzo se colocó a la entrada del templo, frente a la Gloria de los predestinados, pintada en un formato similar, por el mismo autor. Estos fueron los lienzos más grandes del edificio y se ubicaron a la entrada del mismo. Esta tesis intentará responder porqué de entre todos los temas religiosos, los jesuitas quiteños escogieron representar al infierno como la vista principal de entrada a su iglesia. Para ello, explora el contexto de producción y circulación de la imagen infernal, indaga en las prácticas de la sociedad quiteña que pudieron influir en la decisión jesuítica. Luego, se aborda el imaginario jesuítico sobre la noción de condena eterna en su época; así como el papel de la Compañía de Jesús como productora de esta representación y de una forma particular de mirar e interpretar esta pintura, acompañándola de usos religiosos como la confesión o la penitencia. Finalmente, se analizará la pintura en relación tanto con las prácticas sociales quiteñas, como con los imaginarios jesuíticos del fuego eterno. En esta tesis utiliza como fuentes a historias ejemplares, sermones, pinturas y textos catequéticos producidos entre 1600 y 1697. Para abordarlas utiliza la metodología de la historia contextual del arte y de la nueva historia cultural. De esta manera ensaya una interpretación del universo de significación de la pintura de Hernando de la Cruz.

Acarología forense [Forensic acarology]

Mites are a highly diversified group of chelicerates (arthropods) adapted to a broad spectrum of habitats and diets, presenting extreme specificity to habitats. They are considered to be important indicators of environmental conditions including those modified by human beings. Therefore, they can inform about the environment where a corpse has been exposed to, about the route of specific merchandises, as well as about other applied aspects of forensic entomology. It is not rare the presence of species adapted to cadaveric environments. Jean Pierre Mégnin, forensic veterinarian considered pioneer in the development of forensic entomology, conscious about the importance of mites as forensic indicators, was the first including mites in the decomposition process. For Mégnin, wave six was formed by mites only. Due to the increasing interest of forensic experts in including these organisms in their analysis of trace evidence, as mites are one of the most ubiquitous organisms, we have developed standards for the sampling, conservation and custody of mite evidence of forensic interest.

Upper limit on the cosmic-ray photon flux above 10(19) eV using the surface detector of the Pierre Auger Observatory

A method is developed to search for air showers initiated by photons using data recorded by the surface detector of the Auger Observatory. The approach is based on observables sensitive to the longitudinal shower development, the signal risetime and the curvature of the shower front. Applying this method to the data, tipper limits on the flux of photons of 3.8 x 10(-3), 2.5 x 10(-3), and 2.2 x 10(-3) km(-2) sr(-1) yr(-1) above 10(19) eV, 2 x 10(19) eV, and 4 x 10(19) eV are derived, with corresponding limits on the fraction of photons being 2.0%, 5.1%, and 31% (all limits at 95% c.l.). These photon limits disfavor certain exotic models of sources of cosmic rays. The results also show that the approach adopted by the Auger Observatory to calibrate the shower energy is not strongly biased by a contamination from photons. (C) 2008 Elsevier B.V. All rights reserved.

Advanced functionality for radio analysis in the Offline software framework of the Pierre Auger Observatory

The advent of the Auger Engineering Radio Array (AERA) necessitates the development of a powerful framework for the analysis of radio measurements of cosmic ray air showers. As AERA performs ""radio-hybrid"" measurements of air shower radio emission in coincidence with the surface particle detectors and fluorescence telescopes of the Pierre Auger Observatory, the radio analysis functionality had to be incorporated in the existing hybrid analysis solutions for fluorescence and surface detector data. This goal has been achieved in a natural way by extending the existing Auger Offline software framework with radio functionality. In this article, we lay out the design, highlights and features of the radio extension implemented in the Auger Offline framework. Its functionality has achieved a high degree of sophistication and offers advanced features such as vectorial reconstruction of the electric field, advanced signal processing algorithms, a transparent and efficient handling of FFTs, a very detailed simulation of detector effects, and the read-in of multiple data formats including data from various radio simulation codes. The source code of this radio functionality can be made available to interested parties on request. (C) 2011 Elsevier B.V. All rights reserved.

Trigger and aperture of the surface detector array of the Pierre Auger Observatory

The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detectors, for the study of extensive air showers (EAS) generated by ultra-high-energy cosmic rays. We describe the trigger hierarchy, from the identification of candidate showers at the level of a single detector, amongst a large background (mainly random single cosmic ray muons), up to the selection of real events and the rejection of random coincidences. Such trigger makes the surface detector array fully efficient for the detection of EAS with energy above 3 x 10(18) eV, for all zenith angles between 0 degrees and 60 degrees, independently of the position of the impact point and of the mass of the primary particle. In these range of energies and angles, the exposure of the surface array can be determined purely on the basis of the geometrical acceptance. (C) 2009 Elsevier B.V. All rights reserved.

Atmospheric effects on extensive air showers observed with the surface detector of the Pierre Auger observatory

Atmospheric parameters, Such as pressure (P), temperature (T) and density (rho proportional to P/T), affect the development of extensive air showers initiated by energetic cosmic rays. We have Studied the impact of atmospheric variations on extensive air showers by means of the surface detector of the Pierre Auger Observatory. The rate of events shows a similar to 10% seasonal modulation and similar to 2% diurnal one. We find that the observed behaviour is explained by a model including the effects associated with the variations of P and rho. The former affects the longitudinal development of air showers while the latter influences the Moliere radius and hence the lateral distribution of the shower particles. The model is validated with full simulations of extensive air showers using atmospheric profiles measured at the site of the Pierre Auger Observatory. (C) 2009 Elsevier B.V. All rights reserved.

Upper limit on the cosmic-ray photon fraction at EeV energies from the Pierre Auger Observatory

From direct observations of the longitudinal development of ultra-high energy air showers performed with the Pierre Auger Observatory, upper limits of 3.8%, 2.4%, 3.5% and 11.7% (at 95% c.l.) are obtained on the fraction of cosmic-ray photons above 2, 3, 5 and 10 EeV (1 EeV equivalent to 10(18) eV), respectively. These are the first experimental limits on ultra-high energy photons at energies below 10 EeV. The results complement previous constraints on top-down models from array data and they reduce systematic uncertainties in the interpretation of shower data in terms of primary flux, nuclear composition and proton-air cross-section. (C) 2009 Elsevier B.V. All rights reserved.

Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory

The Pierre Auger Collaboration has reported. evidence for anisotropy in the distribution of arrival directions of the cosmic rays with energies E > E(th) = 5.5 x 10(19) eV. These show a correlation with the distribution of nearby extragalactic objects, including an apparent excess around the direction of Centaurus A. If the particles responsible for these excesses at E > E(th) are heavy nuclei with charge Z, the proton component of the sources should lead to excesses in the same regions at energies E/Z. We here report the lack of anisotropies in these directions at energies above E(th)/Z (for illustrative values of Z = 6, 13, 26). If the anisotropies above E(th) are due to nuclei with charge Z, and under reasonable assumptions about the acceleration process, these observations imply stringent constraints on the allowed proton fraction at the lower energies.