Zooplankton oxygen consumption and nutrient release in relation to species composition, animals size and enviromental conditions in the Baltic Sea during May and August

[EN] Zooplankton metabolism in terms of oxygen consumption and ñutrient reléase (ammonia, phosphate) were measiu'ed in the Baltic Sea, a températe área with high envirormiental changes both in space and in time. Plankton of the surface layer were analysed with balance measurements in 4 size classes between 50 and 1000 nm during spring in 1988, 1990 and 1991, in summer 19^8 and 1990 as well. The use of electrón transport system (ETS), and the Glutamate Dehydrogenase (GDH) activity as indicators for respiration and ammonia reléase respectively, enlarged the data density and made a three dimensional resolution available (May 1990, 1991). Data are in the range of the latitudinal dependend magnitude. They reflect slight interannual, more seasonal and regional aspects. Animáis size, temperature, food concentration, and species composition influence the specific rates

The VIMOS-VLT Deep Survey: the evolution of type-1 AGN

Quasars and AGN play an important role in many aspects of the modern cosmology. Of particular interest is the issue of the interplay between AGN activity and formation and evolution of galaxies and structures. Studies on nearby galaxies revealed that most (and possibly all) galaxy nuclei contain a super-massive black hole (SMBH) and that between a third and half of them are showing some evidence of activity (Kormendy and Richstone, 1995). The discovery of a tight relation between black holes mass and velocity dispersion of their host galaxy suggests that the evolution of the growth of SMBH and their host galaxy are linked together. In this context, studying the evolution of AGN, through the luminosity function (LF), is fundamental to constrain the theories of galaxy and SMBH formation and evolution. Recently, many theories have been developed to describe physical processes possibly responsible of a common formation scenario for galaxies and their central black hole (Volonteri et al., 2003; Springel et al., 2005a; Vittorini et al., 2005; Hopkins et al., 2006a) and an increasing number of observations in different bands are focused on collecting larger and larger quasar samples. Many issues remain however not yet fully understood. In the context of the VVDS (VIMOS-VLT Deep Survey), we collected and studied an unbiased sample of spectroscopically selected faint type-1 AGN with a unique and straightforward selection function. Indeed, the VVDS is a large, purely magnitude limited spectroscopic survey of faint objects, free of any morphological and/or color preselection. We studied the statistical properties of this sample and its evolution up to redshift z 4. Because of the contamination of the AGN light by their host galaxies at the faint magnitudes explored by our sample, we observed that a significant fraction of AGN in our sample would be missed by the UV excess and morphological criteria usually adopted for the pre-selection of optical QSO candidates. If not properly taken into account, this failure in selecting particular sub-classes of AGN could, in principle, affect some of the conclusions drawn from samples of AGN based on these selection criteria. The absence of any pre-selection in the VVDS leads us to have a very complete sample of AGN, including also objects with unusual colors and continuum shape. The VVDS AGN sample shows in fact redder colors than those expected by comparing it, for example, with the color track derived from the SDSS composite spectrum. In particular, the faintest objects have on average redder colors than the brightest ones. This can be attributed to both a large fraction of dust-reddened objects and a significant contamination from the host galaxy. We have tested these possibilities by examining the global spectral energy distribution of each object using, in addition to the U, B, V, R and I-band magnitudes, also the UV-Galex and the IR-Spitzer bands, and fitting it with a combination of AGN and galaxy emission, allowing also for the possibility of extinction of the AGN flux. We found that for 44% of our objects the contamination from the host galaxy is not negligible and this fraction decreases to 21% if we restrict the analysis to a bright subsample (M1450 <-22.15). Our estimated integral surface density at IAB < 24.0 is 500 AGN per square degree, which represents the highest surface density of a spectroscopically confirmed sample of optically selected AGN. We derived the luminosity function in B-band for 1.0 < z < 3.6 using the 1/Vmax estimator. Our data, more than one magnitude fainter than previous optical surveys, allow us to constrain the faint part of the luminosity function up to high redshift. A comparison of our data with the 2dF sample at low redshift (1 < z < 2.1) shows that the VDDS data can not be well fitted with the pure luminosity evolution (PLE) models derived by previous optically selected samples. Qualitatively, this appears to be due to the fact that our data suggest the presence of an excess of faint objects at low redshift (1.0 < z < 1.5) with respect to these models. By combining our faint VVDS sample with the large sample of bright AGN extracted from the SDSS DR3 (Richards et al., 2006b) and testing a number of different evolutionary models, we find that the model which better represents the combined luminosity functions, over a wide range of redshift and luminosity, is a luminosity dependent density evolution (LDDE) model, similar to those derived from the major Xsurveys. Such a parameterization allows the redshift of the AGN density peak to change as a function of luminosity, thus fitting the excess of faint AGN that we find at 1.0 < z < 1.5. On the basis of this model we find, for the first time from the analysis of optically selected samples, that the peak of the AGN space density shifts significantly towards lower redshift going to lower luminosity objects. The position of this peak moves from z 2.0 for MB <-26.0 to z 0.65 for -22< MB <-20. This result, already found in a number of X-ray selected samples of AGN, is consistent with a scenario of “AGN cosmic downsizing”, in which the density of more luminous AGN, possibly associated to more massive black holes, peaks earlier in the history of the Universe (i.e. at higher redshift), than that of low luminosity ones, which reaches its maximum later (i.e. at lower redshift). This behavior has since long been claimed to be present in elliptical galaxies and it is not easy to reproduce it in the hierarchical cosmogonic scenario, where more massive Dark Matter Halos (DMH) form on average later by merging of less massive halos.

The assessment of visual short-term memory in considering the underlying processes and their relation to psychometric intelligence

By means of fixed-links modeling the present study assessed processes involved in visual short-term memory functioning and investigates how these processes are related to intelligence. Using a color change detection task, short-term memory demands increased across three experimental conditions as a function of number of presented stimuli. We measured amount of information retained in visual short-term memory by hit rate as well as speed of visual short-term memory scanning by reaction time. For both measures, fixed-links modeling revealed a constant process reflecting processes irrespective of task manipulation as well as two increasing processes reflecting the increasing short-term memory demands. For visual short-term memory scanning, a negative association between intelligence and the constant process was found but no relationship between intelligence and the increasing processes. Thus, basic processing speed, rather than speed influenced by visual short-term memory demands, differentiates between high- and low-intelligent individuals. Intelligence was positively related to the experimental processes of shortterm memory retention but not to the constant process. In sum, significant associations with intelligence were only obtained when the specific processes of short-term memory were decomposed emphasizing the importance of a thorough assessment of cognitive processes when investigating their relation to intelligence.

Procoagulant reactivity to laboratory acute mental stress in Africans and Caucasians, and its relation to depressive symptoms: the SABPA study.

The risk of cardiovascular disease is dramatically increasing in Africans (black). The prothrombotic stress response contributes to atherothrombotic disease and is modulated by depressive symptoms. We examined coagulation reactivity to acute mental stress and its relation to psychological well-being in Africans relative to Caucasians (white). A total of 102 African and 165 Caucasian school teachers underwent the Stroop Color-Word Conflict test. Circulating levels of von Willebrand factor (VWF) antigen, fibrinogen, and D-dimer were measured before and after the Stroop. Cardiovascular reactivity measures were also obtained. All participants completed the Patient Health Questionnaire-9 and the General Health Questionnaire-28 for the assessment of depressive symptoms and total psychological distress, respectively. After controlling for covariates, resting levels of VWF, fibrinogen, and D-dimer were higher in Africans than in Caucasians (all p-values ≤0.006). Depressive symptoms and psychological distress were not significantly associated with resting coagulation measures. Stress reactivity in VWF (p<0.001) and fibrinogen (p=0.016), but not in D-dimer (p=0.27), were decreased in Africans relative to Caucasians with Africans showing greater reactivity of total peripheral resistance (p=0.017). Depressive symptoms, but not general psychological distress, were associated with greater VWF increase (p=0.029) and greater fibrinogen decrease (p=0.030) in Africans relative to Caucasians. In conclusion, Africans showed greater hypercoagulability at rest but diminished procoagulant reactivity to acute mental stress when compared with Caucasians. Ethnic differences in the vascular adrenergic stress response might partially explain this finding. Depressive symptoms were associated with exaggerated VWF reactivity in Africans relative to Caucasians. The clinical implications of these findings for Africans need further study.

Efecto del tiempo de maceración sobre el color, la composición tánica y la astringencia de vinos Cabernet Sauvignon y Malbec

El objetivo del trabajo fue estudiar el efecto del tiempo de maceración sobre la composición tánica, el color y la astringencia de vinos Cabernet Sauvignon y Malbec, provenientes de la Zona Alta del Río Mendoza y saber qué tiempo de maceración permite una mayor expresión del color y del cuerpo del vino. A partir de dos vinificaciones industriales, se realizaron muestreos para determinar las curvas de extracción de los componentes fenólicos y del color. Además, se llevaron a cabo dos experimentos probando un tiempo de maceración corto, de 5 días, uno “clásico" en la región, de 10 días, y uno largo, de 20 días. En los vinos resultantes se determinó el perfil fenólico, discriminando los componentes tánicos y del color, durante el primer año de conservación en vasijas de vidrio. Se utilizaron técnicas de espectrometría VIS y UV y los vinos fueron evaluados por un panel de expertos degustadores. La variedad Cabernet S. siguió un patrón de extracción de antocianos y taninos durante la maceración acorde con lo que indica la bibliografía. La magnitud del color rojo alcanzó un máximo cerca del 10º día y luego sufrió una caída que, en la maceración de 20 días, significó una pérdida de alrededor de un 10%. Los taninos aumentaron rápidamente hasta el 10º día y luego continuaron creciendo muy lentamente. Los vinos Cabernet S. obtenidos con maceración de 10 días y de 20 días resultaron muy superiores en cuanto a los contenidos de antocianos, color polimérico y taninos. También provocaron sensaciones de concentración y untuosidad mayores. Además resultaron más ásperos, astringentes y secantes que los de 5 días, pero estas sensaciones fueron moderadas. Los vinos de 20 días fueron similares a los de 10 días salvo en que alcanzaron un contenido mayor de polifenoles totales y de taninos no astringentes. La variedad Malbec siguió un patrón de extracción de antocianos y taninos similar al Cabernet S. hasta el 10º día, pero luego ambos mostraron una caída pronunciada, como consecuencia de un deterioro oxidativo. La maceración de 10 días resultó óptima y los vinos se destacaron por su mayor contenido en polifenoles totales, antocianos, color polimérico y taninos. Estos atributos provocaron sensaciones de concentración y untuosidad destacadas y similares a las de los Cabernet S. de 10 y 20 días. Las sensaciones de secante, áspero y astringente fueron menores que en los Cabernet. Los Malbec de 5 días resultaron muy pobres en atributos y los de 20 días con característics intermedias entre los de 5 y los de 10 días. En ambas variedades la pérdida en los contenidos de antocianos copigmentados se acompañó de un aumento proporcional en los contenidos de antocianos polimerizados. Durante el estacionamiento todos los vinos Cabernet S. y Malbec sufrieron una degradación de polifenoles totales, antocianos y taninos. El ritmo de degradación de cada compuesto fue similar para los distintos vinos, sin importar las concentraciones iniciales del compuesto. En ambas variedades los polifenoles totales y los taninos se correlacionaron positivamente con la aspereza, la astringencia, lo secante, la untuosidad y la concentración. Lo secante se asoció negativamente con la proporción de taninos no precipitables con gelatina. La espectrometría VIS y UV, como método instrumental de análisis, resultó suficientemente potente como para permitir una la apreciación del perfil fenólico y diferenciar los vinos Cabernet S. de los Malbec, independientemente del tiempo de maceración con que fueron elaborados.

Caracterización por contenido de β-carotenos de ocho cultivares de zanahoria (Daucus carota L.) y su relación con el color

El objetivo fue determinar, durante dos años, el contenido de β-caroteno y su relación con el Índice de Color (IC), de ocho cultivares comerciales del tipo 'Flakkee' cultivadas en el INTA La Consulta. El diseño experimental a campo utilizado fue en bloques al azar con 3 repeticiones. Se evaluó β-caroteno (espectrofotometría a 450 nm) y se calculó el IC, mediante captación de imagen digital con PC y escáner, midiendo L, a y b del Sistema CIELAB. Los datos fueron analizados por ACP (análisis de componentes principales), la visualización de la variabilidad, por cartografiado de datos, análisis de varianza, pruebas de diferencia de medias y correlaciones. Los contenidos de β-carotenos y el IC de los cultivares se mantuvieron constantes durante los dos años estudiados, resultando las cultivares Natasha, Flakesse y Colmar las de mayor valor nutricional en cuanto a aporte de β-carotenos. En el rango de valores menores de 18 mg%g de β-carotenos, se observó una correlación positiva significativa en las cultivares Supreme, Spring y Laval. No se encontró una correlación alta lineal entre el IC y el contenido de β-carotenos. El uso del IC resulta adecuado para predecir, en un intervalo de valores, el contenido de β-carotenos en cultivares de zanahoria.

Age-depth relation and red colour reflectance of ODP Leg 177 sites

The Antarctic Polar Front is an important biogeochemical divider in the Southern Ocean. Laminated diatom mat deposits record episodes of massive flux of the diatom Thalassiothrix antarctica beneath the Antarctic Polar Front and provide a marker for tracking the migration of the Front through time. Ocean Drilling Program Sites 1091, 1093 and 1094 are the only deep piston cored record hitherto sampled from the sediments of the circumpolar biogenic opal belt. Mapping of diatom mat deposits between these sites indicates a glacial-interglacial front migration of up to 6 degrees of latitude in the early/mid Pleistocene. The mid-Pleistocene transition marks a stepwise minimum 7° northward migration of the locus of the Polar Front sustained for about 450 kyr until an abrupt southward return to a locus similar to its modern position and further south than any mid-Pleistocene locus. This interval from a "900 ka event" that saw major cooling of the oceans and a d13C minimum through to the 424 ka Mid-Brunhes Event at Termination V is also seemingly characterised by 1) sustained decreased carbonate in the sub-tropical south Atlantic, 2) reduced strength of Antarctic deep meridional circulation, 3) lower interglacial temperatures and lower interglacial atmospheric CO2 levels (by some 30 per mil) than those of the last 400 kyr, evidencing less complete deglaciation. This evidence is consistent with a prolonged period lasting 450 kyr of only partial ventilation of the deep ocean during interglacials and suggests that the mechanisms highlighted by recent hypotheses linking mid-latitude atmospheric conditions to the extent of deep ocean ventilation and carbon sequestration over glacial-interglacial cycles are likely in operation during the longer time scale characteristic of the mid-Pleistocene transition. The cooling that initiated the "900 ka event" may have been driven by minima in insolation amplitude related to eccentricity modulation of precession that also affected low latitude climates as marked by threshold changes in the African monsoon system. The major thresholds in earth system behaviour through the mid-Pleistocene transition were likely governed by an interplay of the 100 kyr and 400 kyr eccentricity modulation of precession.

Physical parameters in relation to physiological changes of avocado during ripening (20ºc) and cold storage (6ºc) in different conditions.

The application of the response of fruits to low energy for mechanical impacts is described, for evaluation of post-harvest ripening of avocadoes of the variety "Hass". An impactor of 50g of weight, provided with an accelerometer, and free-falling from a height of 4 cm, is used; it is interfaced to a computer and uses a special software for retrieving and analyzing the deceleration data. Impact response parameters of individual fruits were compared to firmness of the pulp, measured by the most used method of double-plate puncture, as well as to other physical and physiological parameters: color, skin puncture ethylene production rate and others. Two groups of fruits were carefully selected, stored at 6º C (60 days) and ripened at 20ºC (11 days), and tested during the storage period. It is shown that, as in other types of fruits, impact response can be a good predictor of firmness in avocadoes, obtaining the same accuracy as with destructive firmness measurements. Mathematical and multiple regression models are calculated and compared to measured data, with which a prediction of storage period can be made for these fruits.

Optimization of optical systems for LED spot lights concerning the color uniformity

Spotlighting is one illumination field where the application of light emitting diodes (LED) creates many advantages. Commonly, the system for spot lights consists of a LED light engine and collimating secondary optics. Through angular or spatial separated emitted light from the source and imaging optical elements, a non uniform far field appears with colored rings, dots or patterns. Many feasible combinations result in very different spatial color distributions. Several combinations of three multi-chip light sources and secondary optical elements like reflectors and TIR lenses with additional facets or scattering elements were analyzed mainly regarding the color uniformity. They are assessed by the merit function Usl which was derived from human factor experiments and describes the color uniformity based on the visual perception of humans. Furthermore, the optical systems are compared concerning efficiency, peak candela and aspect ratio. Both types of optics differ in the relation between the color uniformity level and other properties. A plain reflector with a slightly color mixing light source performs adequate. The results for the TIR lenses indicate that they need additional elements for good color mixing or blended light source. The most convenient system depends on the requirements of the application.

El color en la transfiguración del espacio: un estudio empírico de los dispositivos de transformación y configuración

La presente investigación analiza la capacidad del color de cualificar los espacios y propone una clasificación que ordene los diferentes dispositivos que actúan en este proceso. El objetivo de esta tesis es describir estos dispositivos estableciéndolos como parte inequívoca de cualquier proceso desencadenado por la presencia del binomio luz y color. El color ha sido objeto de estudio y experimentación a lo largo de la historia, en todas las artes y las distintas disciplinas relacionadas con la física, la percepción y la interacción. De este modo se realiza una aproximación teórica e histórica al color desde puntos de vista interdisciplinares, para llegar a comprender el modo en el que el color se acaba separando de la forma para pasar a formar parte de la configuración del espacio. Con el propósito de alcanzar este objetivo, se ha realizado un recorrido a través de diferentes teorías y manifestaciones artísticas realizadas en torno al color a lo largo de la Historia, para encontrar las claves de la relación del color con el espacio. Tomando de base este primer acercamiento al tema, se realiza un estudio empírico exhaustivo con modelos físicos con el fin de aislar los dispositivos que intervienen el este proceso en el que el color se pone en relación con el espacio; se analiza su variación a medida que fluctúan las características de los elementos que desencadenan los dispositivos. El objetivo es descubrir un orden, una taxonomía, que permita interpretar cualquier transformación producida por el color en el espacio. Posteriormente, se verifica la validez de esta clasificación estudiando siete espacios modelo en los que el color transfigura el espacio mediante la activación conjunta de varios de los dispositivos analizados. Se ha elegido este grupo de siete espacios debido a que, al tomarlos como suma, sus interiores engloban todos los fenómenos encontrados en el análisis previo. El conjunto de los dispositivos que actúan en cada espacio forma un sistema único e irrepetible que tiene que ver con su transfiguración espacial mediante la luz y el color. Estos sistemas constituyen parte de la génesis propia de cada espacio a través de una secuencia de dispositivos de transformación y configuración espacial que lo hace singular. Los dispositivos clasificados en esta investigación se encuentran en cualquier espacio en el que intervengan la luz y el color, agrupándose secuencialmente en sistemas determinados que cualifican el espacio arquitectónico. ABSTRACT This research analyzes the ability of the colour to qualify the spaces and proposes a classification to arrange the different devices that act in this process. The aim of this thesis is to describe these devices, unequivocally established as part of any process triggered by the presence of light and color pairing. Colour has been the subject of study and experimentation throughout history, in all the arts and disciplines related to physics, perception and interaction. Thus a theoretical and historical approach to the colour is developed from interdisciplinary points of view, in order to understand the way that colour separates from the form and is part of the space configuration. With the purpose of reaching this target, there has been a journey through the artistic movements and theories on colour throughout history, seeking for the key points of its relation with the space. Based on these first intuitions as a starting point, an exhaustive empirical study is made with physical models with the purpose of isolating the devices that participate in this process where colour is related with the space as well as analyzing their variation to the extent that the characteristics of the elements which cause them fluctuate. The objective is to discover an order, a taxonomy that allows to performing any transformation produced by the colour in the space. Afterwards, the validity of this classification is verified by studying seven model spaces in which the colour transfigures the space by the combined activation of several analyzed devices. These seven spaces were chosen due to all the phenomenon set in the previous analysis are included in their interior space. The group of devices that act on each space creates an unrepeatable and unique system that has to do with its spatial transfiguration by means of light and colour. These systems form part of the origin itself of each space through a sequence of devices of spatial transformation and configuration that make this space unique. The devices sorted in this research transform and configure any space in which light and colour participate, sequentially grouping together in determined systems that qualify the architectonic space.

Ultrasensitive detection of pathological prion protein aggregates by dual-color scanning for intensely fluorescent targets

A definite diagnosis of prion diseases such as Creutzfeldt–Jakob disease (CJD) relies on the detection of pathological prion protein (PrPSc). However, no test for PrPSc in cerebrospinal fluid (CSF) has been available thus far. Based on a setup for confocal dual-color fluorescence correlation spectroscopy, a technique suitable for single molecule detection, we developed a highly sensitive detection method for PrPSc. Pathological prion protein aggregates were labeled by specific antibody probes tagged with fluorescent dyes, resulting in intensely fluorescent targets, which were measured by dual-color fluorescence intensity distribution analysis in a confocal scanning setup. In a diagnostic model system, PrPSc aggregates were detected down to a concentration of 2 pM PrPSc, corresponding to an aggregate concentration of approximately 2 fM, which was more than one order of magnitude more sensitive than Western blot analysis. A PrPSc-specific signal could also be detected in a number of CSF samples from patients with CJD but not in control samples, providing the basis for a rapid and specific test for CJD and other prion diseases. Furthermore, this method could be adapted to the sensitive detection of other disease-associated amyloid aggregates such as in Alzheimer's disease.