Aspects of Speaking-Face Data Corpus Design Methodology

This paper develops a methodology for the design of audiovideo data corpora of the speaking face. Existing corpora are surveyed and the principles of data specification, data description and statistical representation are analysed both from an application-driven and from a scientifically motivated perspective. Furthermore, the possibility of "opportunistic" design of speaking-face data corpora is considered

Feeding Programs for Newly Arrived or Recently Weaned Calves

Fall is a stressful time for calves. They are generally weaned at this time. Following weaning, they are often transported or moved to a sale barn or unfamiliar facility. Upon arrival, they may be mixed with other cattle, subjected to processing and forced to eat unfamiliar feeds. In addition, all of these stresses may be compounded by foul weather. To combat the negative impacts of stress cattlemen should strive to get new calves on feed as rapidly as possible. Proper nutrition and a consistent health program are essential when starting calves on feed. Proper nutrition is important from two standpoints. First, the success of any health program is highly dependant on the nutritionals status of the calf. In order for the immune system of the calf to form antibodies in response to vaccination programs, sufficient protein, energy vitamins and minerals must be available. The second reason is more obvious. The calf simply needs to consume feed in order to grow and thrive. Ownership and facility costs are generally high. Feeder cattle need to gain weight in order to make money for cattlemen. Newly arrived or recently weaned calves do not readily eat upon arrival in a feedlot. Texas data (Hutcheson, 1980) suggests that a surprisingly high percentage of cattle do not eat during the first few days in the feedlot. Table 1 shows that on day one in the feedlot, only 21.7% of the cattle eat. On day three, over 40% of the cattle will not eat. On seven, 30% of the cattle will not eat. And on day 10, an average of 15% of the cattle will not eat. These data suggest that getting cattle started on feed is a major problem. Three problems need to be addressed in order to get cattle started on feed. First, recently weaned or newly arrived cattle will generally not recognize the feed bunk and may not recognize water troughs. Second, new cattle may not recognize the feed that the producer wishes to feed him. Finally, feed intake by new cattle will likely be low due to stress. The remaining section of this paper focus on managing around these problems. Additional sections include discussions of feed additives, commercial receiving, or weaning rations and health programs

Thinking outside the box: effects of modes larger than the survey on matter power spectrum covariance

Accurate power spectrum (or correlation function) covariance matrices are a crucial requirement for cosmological parameter estimation from large scale structure surveys. In order to minimize reliance on computationally expensive mock catalogs, it is important to have a solid analytic understanding of the different components that make up a covariance matrix. Considering the matter power spectrum covariance matrix, it has recently been found that there is a potentially dominant effect on mildly non-linear scales due to power in modes of size equal to and larger than the survey volume. This beat coupling effect has been derived analytically in perturbation theory and while it has been tested with simulations, some questions remain unanswered. Moreover, there is an additional effect of these large modes, which has so far not been included in analytic studies, namely the effect on the estimated average density which enters the power spectrum estimate. In this article, we work out analytic, perturbation theory based expressions including both the beat coupling and this local average effect and we show that while, when isolated, beat coupling indeed causes large excess covariance in agreement with the literature, in a realistic scenario this is compensated almost entirely by the local average effect, leaving only ~ 10% of the excess. We test our analytic expressions by comparison to a suite of large N-body simulations, using both full simulation boxes and subboxes thereof to study cases without beat coupling, with beat coupling and with both beat coupling and the local average effect. For the variances, we find excellent agreement with the analytic expressions for k < 0.2 hMpc−1 at z = 0.5, while the correlation coefficients agree to beyond k = 0.4 hMpc−1. As expected, the range of agreement increases towards higher redshift and decreases slightly towards z = 0. We finish by including the large-mode effects in a full covariance matrix description for arbitrary survey geometry and confirming its validity using simulations. This may be useful as a stepping stone towards building an actual galaxy (or other tracer's) power spectrum covariance matrix

Thinking outside the box: effects of modes larger than the survey on matter power spectrum covariance

Accurate power spectrum (or correlation function) covariance matrices are a crucial requirement for cosmological parameter estimation from large scale structure surveys. In order to minimize reliance on computationally expensive mock catalogs, it is important to have a solid analytic understanding of the different components that make up a covariance matrix. Considering the matter power spectrum covariance matrix, it has recently been found that there is a potentially dominant effect on mildly non-linear scales due to power in modes of size equal to and larger than the survey volume. This beat coupling effect has been derived analytically in perturbation theory and while it has been tested with simulations, some questions remain unanswered. Moreover, there is an additional effect of these large modes, which has so far not been included in analytic studies, namely the effect on the estimated average density which enters the power spectrum estimate. In this article, we work out analytic, perturbation theory based expressions including both the beat coupling and this local average effect and we show that while, when isolated, beat coupling indeed causes large excess covariance in agreement with the literature, in a realistic scenario this is compensated almost entirely by the local average effect, leaving only similar to 10% of the excess. We test our analytic expressions by comparison to a suite of large N-body simulations, using both full simulation boxes and subboxes thereof to study cases without beat coupling, with beat coupling and with both beat coupling and the local average effect. For the variances, we find excellent agreement with the analytic expressions for k < 0.2 hMpc(-1) at z = 0.5, while the correlation coefficients agree to beyond k = 0.4 hMpc(-1). As expected, the range of agreement increases towards higher redshift and decreases slightly towards z = 0. We finish by including the large-mode effects in a full covariance matrix description for arbitrary survey geometry and confirming its validity using simulations. This may be useful as a stepping stone towards building an actual galaxy (or other tracer's) power spectrum covariance matrix

Earth-like Habitats in Planetary Systems

Understanding the concept of habitability is related to an evolutionary knowledge of the particular planet-in-question. Additional indications so-called "systemic aspects" of the planetary system as a whole governs a particular planet's claim on habitability. Here we focus on such systemic aspects and discuss their relevance to the formation of an 'Earth-like' habitable planet. We summarize our results obtained by lunar sample work and numerical models within the framework of the Research Alliance "Planetary Evolution and Life". We consider various scenarios which simulate the dynamical evolution of the Solar System and discuss the likelihood of forming an Earth-like world orbiting another star. Our model approach is constrained by observations of the modern Solar System and the knowledge of its history. Results suggest that the long-term presence of terrestrial planets is jeopardized due to gravitational interactions if giant planets are present. But habitability of inner rocky planets may be supported in those planetary systems hosting giant planets. Gravitational interactions within a complex multiple-body structure including giant planets may supply terrestrial planets with materials which formed in the colder region of the proto-planetary disk. During these processes, water, the prime requisite for habitability, is delivered to the inner system. This may occur either during the main accretion phase of terrestrial planets or via impacts during a post-accretion bombardment. Results for both processes are summarized and discussed with reference to the lunar crater record. Starting from a scenario involving migration of the giant planets this contribution discusses the delivery of water to Earth, the modification of atmospheres by impacts in a planetary system context and the likelihood of the existence of extrasolar Earth-like habitable worlds.Comment: 36 Pages, 6 figures, 2014, Special Issue in Planetary and Space Science on the Helmholtz Research Alliance on Planetary Evolution and Lif

The cratering record of Ganymede and the origin of potential impactors: open issues

The origin of impactors on the Galilean satellites of Jupiter is an open question. In this study we present results from a mapping campaign based on reprocessed Voyager and Galileo SSI images in order to derive a thourough data base of Ganymede's crater distributions

Therapie der blanden Struma: Erfahrungen mit einer Kombination von 100 µg L-Thyroxin und 10 µg L-Trijodthyronin

Dtsch med Wochenschr 1981; 106: 579-583 DOI: 10.1055/s-2008-1070359 © Georg Thieme Verlag KG Stuttgart · New York Therapie der blanden Struma: Erfahrungen mit einer Kombination von 100 µg L-Thyroxin und 10 µg L-Trijodthyronin Treatment of non-toxic goitre: results of combined treatment with 100 µg L-thyroxine and 10 µg L-triiodothyronine C. R. Pickardt, R. Gärtner, J. Habermann, K. Horn, P. C. Scriba, F. A. Horster, H. Wagner, K. Hengst Medizinische Klinik Innenstadt der Universität München, Klinik für Innere Medizin, Medizinische Hochschule Lübeck, Medizinische Klinik C und Poliklinik der Universität Düsseldorf sowie Medizinische Klinik und Poliklinik der Universität Münster Zusammenfassung Bei 96 Patienten mit blander Struma wurde eine offene Prüfung mit einem neuen Schilddrüsenhormonpräparat durchgeführt, das 100 µg L-Thyroxin (T4) und 10 µg L-Trijodthyronin (T3) pro Tablette enthält. Als Parameter für die therapeutisch wirksame Tagesdosis wurde die Suppression des TRH-stimulierten Thyreotropinspiegels im Serum gewählt. Hierbei war eine Tagesdosis von 50 µg T4 und 5 µg T3 bei 16 Patienten unwirksam; 75 µg T4 und 7,5 µg T3waren bei nur 4 von 12 Patienten suppressiv wirksam, während 100 µg T4 und 10 µg T3 bei allen Düsseldorfer und Münsteraner Patienten, aber nur bei 17 von 31 Patienten in München den TRH-stimulierten TSH-Anstieg supprimierte. Während der gesamten Therapiedauer blieben Thyroxin- und Trijodthyroninspiegel im Serum im Normbereich; bei einigen Patienten erhöhte sich der Quotient aus Thyroxin und thyroxinbindendem Globulin über die Norm. Zeichen einer Überdosierung oder Unverträglichkeit wurden nicht beobachtet. In pharmakokinetischen Untersuchungen an acht freiwilligen schilddrüsengesunden Probanden erreichte der mittlere Thyroxin- und Trijodthyroninspiegel etwa 2 Stunden nach Applikation sein Maximum und näherte sich nach sechs Stunden wieder der Norm. Es zeigten sich deutliche individuelle Schwankungen in den ersten Stunden nach Applikation. Wir empfehlen deshalb, Schilddrüsenhormonspiegel erst 12 oder 24 Stunden nach Applikation eines Schilddrüsenhormonpräparates zu bestimmen; zu dieser Zeit sollte auch der TRH-Test durchgeführt werden. Die Untersuchungen bestätigen die Notwendigkeit, bei der Strumatherapie mit einem Schilddrüsenhormonpräparat die suppressiv wirksame Dosis individuell zu ermitteln; diese Dosis beträgt vorzugsweise 100 µg Thyroxin und 10 µg Trijodthyronin oder 150 µg Thyroxin oder 100 µg Thyroxin und 20 µg Trijodthyronin pro Tag.A new thyroid hormone preparation (100 µg L-thyroxine [T4] and 10 µg L-triiodothyronine [T3] per tablet) was given to 96 patients with non-toxic goitre. Suppression of the TRH-stimulated thyrotropin level in serum was chosen as a measure of therapeutic effectiveness. Daily dose of 50 µg T4 and 5 µg T3 was ineffective in 16 patients; 75 µg T4 and 7.5 µg T3 was effective in only four of twelve patients, while 100 µg T4and 10 µg T3 was effective in all patients from clinics in Düsseldorf and Münster, but in only 17 of 31 patients from Munich, in suppressing the TRH-stimulated TSH rise. During the entire period of treatment serum thyroxine and triiodothyronine levels remained normal. In some patients the ratio of thyroxine to thyroxine-binding globulin was above normal. Signs of overdosage or intolerance were not observed. Pharmacokinetic studies on eight volunteers with normal thyroid function demonstrated that the mean thyroxine and triiodothyronine levels reached maximum about two hours after administration, returning towards normal after six hours. There were marked individual variations in the first hours after administration. It is therefore recommended that the thyroid hormone level be determined no earlier than 12 or 24 hours after the thyroid hormone preparation has been administered; TRH test should also be performed at this time. These results indicate the need for determining individually the effective suppressive dose of a thyroid hormone preparation in the treatment of goitre. Preferably the dose should be 100 µg thyroxine and 10 µg triiodothyronine, or 150 µg thyroxine or 100 µg thyroxine and 20 µg triiodothyronine per day

Mercury's geochronology revised by applying Model Production Functions to Mariner 10 data: geological implications

Model Production Function chronology uses dynamic models of the Main Belt Asteroids (MBAs) and Near Earth Objects (NEOs) to derive the impactor flux to a target body. This is converted into the crater size-frequency-distribution for a specific planetary surface, and calibrated using the radiometric ages of different regions of the Moon's surface. This new approach has been applied to the crater counts on Mariner 10 images of the highlands and of several large impact basins on Mercury. MPF estimates for the plains show younger ages than those of previous chronologies. Assuming a variable uppermost layering of the Hermean crust, the age of the Caloris interior plains may be as young as 3.59 Ga, in agreement with MESSENGER results that imply that long-term volcanism overcame contractional tectonics. The MPF chronology also suggests a variable projectile flux through time, coherent with the MBAs for ancient periods and then gradually comparable also to the NEOs.Comment: Accepted by Journal Geophysical Research Letter

Modeling nuclei of radio galaxies from VLBI radio observations. Application to the BL Lac Object S5 1803+784

We present a new method to fit the variations of both coordinates of a VLBI component as a function of time, assuming that the nucleus of the radio source contains a binary black hole system (BBH system). The presence of a BBH system produces 2 perturbations of the trajectory of the ejected VLBI components. By using only the VLBI coordinates, the problem we have to solve reduces to an astrometric problem. Knowledge of the variations of the VLBI coordinates as a function of time contains the kinematical information, thus we are able to deduce the inclination angle of the source and the bulk Lorentz factor of the ejected component. Generally, there is a family of the BBH system producing the same fit to our data. To illustrate this method, we apply it to the source 1807+784. We find that the inclination of the source is i = 5.8+-1.8 degrees and the VLBI component is ejected with a bulk Lorentz factor of 3.7+-0.3. We determine the family of the BBH system which provides the best fit, assuming at first that the masses of the 2 black holes are equal and then that the masses are different. Each family of BBH systems is characterized by Tp/Tb~1.967, where Tp and Tb are the precession period of the accretion disk of the black hole ejecting the VLBI component and the orbiting period of the BBH system.Comment: 15 pages, 12 figure

Expression of Integrin αvβ3 in Gliomas Correlates with Tumor Grade and Is not Restricted to Tumor Vasculature

In malignant gliomas, the integrin adhesion receptors seem to play a key role for invasive growth and angiogenesis. However, there is still a controversy about the expression and the distribution of αvβ3 integrin caused by malignancy. The aim of our study was to assess the extent and pattern of αvβ3 integrin expression within primary glioblastomas (GBMs) compared with low-grade gliomas (LGGs). Tumor samples were immunostained for the detection of αvβ3 integrin and quantified by an imaging software. The expression of αvβ3 was found to be significantly higher in GBMs than in LGGs, whereby focal strong reactivity was restricted to GBMs only. Subsequent analysis revealed that not only endothelial cells but also, to a large extent, glial tumor cells contribute to the overall amount of αvβ3 integrin in the tumors. To further analyze the integrin subunits, Western blots from histologic sections were performed, which demonstrated a significant difference in the expression of the β3 integrin subunit between GBMs and LGGs. The presented data lead to new insights in the pattern of αvβ3 integrin in gliomas and are of relevance for the inhibition of αvβ3 integrin with specific RGD peptides and interfering drugs to reduce angiogenesis and tumor growth