Radio emission from satellite-Jupiter interactions (especially Ganymede)

Analyzing a database of 26 years of observations of Jupiter from the Nan\c{c}ay Decameter Array, we study the occurrence of Io-independent emissions as a function of the orbital phase of the other Galilean satellites and Amalthea. We identify unambiguously the emissions induced by Ganymede and characterize their intervals of occurrence in CML and Ganymede phase and longitude. We also find hints of emissions induced by Europa and, surprisingly, by Amalthea. The signature of Callisto-induced emissions is more tenuous.Comment: 14 pages, 7 figures, in "Planetary Radio Emissions VIII", G. Fischer, G. Mann, M. Panchenko and P. Zarka eds., Austrian Acad. Sci. Press, Vienna, in press, 201

Photometry of cometary nuclei: Rotation rates, colours and a comparison with Kuiper Belt Objects

We present time-series data on Jupiter Family Comets (JFCs) 17P/Holmes, 47P/Ashbrook-Jackson and 137P/Shoemaker-Levy 2. In addition we also present results from `snap-shot' observations of comets 43P/Wolf-Harrington, 44P/Reinmuth 2, 103P/Hartley 2 and 104P/Kowal 2 taken during the same run. The comets were at heliocentric distances of between 3 and 7 AU at this time. We present measurements of size and activity levels for the snap-shot targets. The time-series data allow us to constrain rotation periods and shapes, and thus bulk densities. We also measure colour indices (V-R) and (R-I) and reliable radii for these comets. We compare all of our findings to date with similar results for other comets and Kuiper Belt Objects (KBOs). We find that the rotational properties of nuclei and KBOs are very similar, that there is evidence for a cut-off in bulk densities at ~ 0.6 g cm^{-3} in both populations, and the colours of the two populations show similar correlations. For JFCs there is no observational evidence for the optical colours being dependant on either position in the orbit or on orbital parameters.Comment: 15 pages, 19 figures, accepted for publication in MNRA

The nucleus of 103P/Hartley 2, target of the EPOXI mission

103P/Hartley 2 was selected as the target comet for the Deep Impact extended mission, EPOXI, in October 2007. There have been no direct optical observations of the nucleus of this comet, as it has always been highly active when previously observed. We aimed to recover the comet near to aphelion, to a) confirm that it had not broken up and was in the predicted position, b) to provide astrometry and brightness information for mission planning, and c) to continue the characterisation of the nucleus. We observed the comet at heliocentric distances between 5.7 and 5.5 AU, using FORS2 at the VLT, at 4 epochs between May and July 2008. We performed VRI photometry on deep stacked images to look for activity and measure the absolute magnitude and therefore estimate the size of the nucleus. We recovered the comet near the expected position, with a magnitude of m_R = 23.74 \pm 0.06 at the first epoch. The comet had no visible coma, although comparison of the profile with a stellar one showed that there was faint activity, or possibly a contribution to the flux from the dust trail from previous activity. This activity appears to fade at further epochs, implying that this is a continuation of activity past aphelion from the previous apparition rather than an early start to activity before the next perihelion. Our data imply a nucleus radius of \le 1 km for an assumed 4% albedo; we estimate a ~6% albedo. We measure a colour of (V-R) = 0. 26 \pm 0.09.Comment: 5 pages, 4 figures, accepted for publication in A&

Differences in salivary α-amylase levels among women with different taste sensitivities

Saliva is the main component of taste receptor cells external environment, and consequently it may have a decisive role in taste perception. Taste sensitivity varies among different individuals. Sensitivity to the compound n-6-propylthiouracil (PROP) has been considerably studied and besides the known influence of genetic background, the contribution of perireceptor environment is not completely clear yet. Salivary α-amylase (one of the main proteins of saliva) is involved in carbohydrate digestion and its enzymatic activity may change the levels of sugars present in the mouth, influencing food perception. To evaluate differences in salivary total protein content and α-amylase activity and expression among individuals with different PROP taste sensitivities. Sixty seven female women (18-30 years old) were classified in one of the three groups of taste sensitivity (non-taster, medium-taster or super-taster), according to the perceived intensity for PROP, using Labeled Magnitude Scales. Saliva was collected without stimulation. Flow rate was calculated by dividing total volume for the 5 minutes collection. Bradford method was used for total protein assessment. Dinitrosalicylic acid assay was used for measuring the starch-hydrolyzing activity of salivary α-amylase, while the expression of this enzyme was evaluated by Wester blot. 20,9% of the subjects were classified as non-taters. The three groups presented similar saliva flow rates and total protein content was not significantly different although a tendency for lower protein concentration in medium-tasters individuals was observed. Salivary α-amylase activity (U/min) was higher in supertasters (P<0,05). Salivary α-amylase activity (U/min) was higher in super-tasters (P<0,05) without any significant differences in expression. In women individual differences in saliva composition can contribute to the different taste sensitivity. One of the differences appears to be α-amylase enzymatic activity. The reason for this deserves to be elucidated, as well as the potential involvement of others salivary proteins

Ensemble Properties of Comets in the Sloan Digital Sky Survey

We present the ensemble properties of 31 comets (27 resolved and 4 unresolved) observed by the Sloan Digital Sky Survey (SDSS). This sample of comets represents about 1 comet per 10 million SDSS photometric objects. Five-band (u,g,r,i,z) photometry is used to determine the comets' colors, sizes, surface brightness profiles, and rates of dust production in terms of the Af{\rho} formalism. We find that the cumulative luminosity function for the Jupiter Family Comets in our sample is well fit by a power law of the form N(< H) \propto 10(0.49\pm0.05)H for H < 18, with evidence of a much shallower fit N(< H) \propto 10(0.19\pm0.03)H for the faint (14.5 < H < 18) comets. The resolved comets show an extremely narrow distribution of colors (0.57 \pm 0.05 in g - r for example), which are statistically indistinguishable from that of the Jupiter Trojans. Further, there is no evidence of correlation between color and physical, dynamical, or observational parameters for the observed comets.Comment: 19 pages, 8 tables, 11 figures, to appear in Icaru

Multimedia delivery in the future internet

The term “Networked Media” implies that all kinds of media including text, image, 3D graphics, audio and video are produced, distributed, shared, managed and consumed on-line through various networks, like the Internet, Fiber, WiFi, WiMAX, GPRS, 3G and so on, in a convergent manner [1]. This white paper is the contribution of the Media Delivery Platform (MDP) cluster and aims to cover the Networked challenges of the Networked Media in the transition to the Future of the Internet. Internet has evolved and changed the way we work and live. End users of the Internet have been confronted with a bewildering range of media, services and applications and of technological innovations concerning media formats, wireless networks, terminal types and capabilities. And there is little evidence that the pace of this innovation is slowing. Today, over one billion of users access the Internet on regular basis, more than 100 million users have downloaded at least one (multi)media file and over 47 millions of them do so regularly, searching in more than 160 Exabytes1 of content. In the near future these numbers are expected to exponentially rise. It is expected that the Internet content will be increased by at least a factor of 6, rising to more than 990 Exabytes before 2012, fuelled mainly by the users themselves. Moreover, it is envisaged that in a near- to mid-term future, the Internet will provide the means to share and distribute (new) multimedia content and services with superior quality and striking flexibility, in a trusted and personalized way, improving citizens’ quality of life, working conditions, edutainment and safety. In this evolving environment, new transport protocols, new multimedia encoding schemes, cross-layer inthe network adaptation, machine-to-machine communication (including RFIDs), rich 3D content as well as community networks and the use of peer-to-peer (P2P) overlays are expected to generate new models of interaction and cooperation, and be able to support enhanced perceived quality-of-experience (PQoE) and innovative applications “on the move”, like virtual collaboration environments, personalised services/ media, virtual sport groups, on-line gaming, edutainment. In this context, the interaction with content combined with interactive/multimedia search capabilities across distributed repositories, opportunistic P2P networks and the dynamic adaptation to the characteristics of diverse mobile terminals are expected to contribute towards such a vision. Based on work that has taken place in a number of EC co-funded projects, in Framework Program 6 (FP6) and Framework Program 7 (FP7), a group of experts and technology visionaries have voluntarily contributed in this white paper aiming to describe the status, the state-of-the art, the challenges and the way ahead in the area of Content Aware media delivery platforms

Influence of taste sensitivity in diet choices and obesity among children.

Introduction: The prevalence of childhood overweight and obesity in Portugal is about 35% (Rito et al., 2012). Lifestyle and dietary habits are important risk factors for weight gain. Food choice and acceptance greatly relies on food perception. The evaluation of taste sensitivity in children and its relation to dietary choices and Body Mass Index (BMI) will be important in a context of obesity prevention. Nonetheless, methodologies for accessing taste sensitivity in children needs to be optimized and adjusted and in Portugal there is not an established protocol. Objectives: To test and optimize a protocol for sweet and bitter taste sensitivity, in Portuguese children, adapted from a protocol already used in German children (Knof et al., 2011). Methods: 20 children, 12 boys and 8 girls, with ages between 8 and 10 years old, were presented with 5 concentrations of sweet (3 – 16 g/L sucrose) and 5 concentrations of bitter taste solutions (0,05 – 0,25 g/L caffeine) and asked for selected the ones perceived as different from water. Results: Test conditions, both the type of presentation and time of tests, resulted for children with the ages tested. For sweet taste, the number and range of concentrations from test solutions appeared to be adequate in the age group between 8 and 10 years. For bitter taste in 80% of children the answers were not consensual with the range of concentrations. Conclusions: The results from the present work suggest that the concentrations used for access bitter taste sensitivity in children from other countries are not sensed by Portuguese children, showing the importance of adjusting adequate concentrations according to sociocultural habits. This may be possible being due to the complex pathway for bitter taste transduction

Avaliação das alterações na sensibilidade para os gostos doce e amargo em ratos sujeitos a uma dieta hiperlipídica

A obesidade é actualmente considerada uma epidemia estando associada a uma predisposição genética do indivíduo e a um consumo energético desadequado O consumo de alimentos ricos em gordura é um dos factores que contribui para o ganho de peso e obesidade. O gosto é um factor determinante na escolha de alimentos e variações individuais na sensibilidade gustativa podem condicionar os hábitos alimentares. O presente trabalho teve como objectivo avaliar potenciais alterações na sensibilidade para os gostos doce e amargo resultantes de um ganho de peso induzido pelo consumo prolongado de uma dieta rica em gordura. Um grupo de ratos Wistar fêmeas mantido numa dieta standard (N=5) e um grupo de animais da mesma estirpe (N=5) com ganho de peso induzido pelo consumo de uma dieta rica em gordura (14% gordura total), durante 12 semanas, foram submetidos a testes de microestrutura de ingestão de líquidos. Os ensaios consistiram na testagem de duas soluções de diferentes concentrações de sacarose (0,3 e 0,1M), para o gosto doce, e duas soluções de diferentes concentrações de quinino (0,1 e 1 mM), para o gosto amargo. Antes de cada ensaio os animais foram submetidos a um jejum hídrico de 16 horas, sendo posteriormente colocados em gaiolas individuais equipadas com um sensor ligado a um computador. Foram feitos os registos das lambidelas, com uma sensibilidade de 20 mili-segundos. Os níveis plasmáticos de insulina e leptina foram avaliados por ELISA. Não se observaram diferenças significativas nos níveis destas hormonas entre os dois grupos testados, apesar dos pesos significativamente mais elevados dos animais sujeitos a dieta rica em gordura. Foram observados aumentos no tamanho dos intervalos de ingestão (nº de lambidelas/cluster), para a solução doce mais concentrada, nos animais tratados com dieta rica em gordura. Essas diferenças apenas se observaram no primeiro minuto de ensaio, sugerindo que as diferenças se devem a alterações de sensibilidade gustativa e não a factores pós-ingestivos. Estes resultados sugerem que indivíduos com aumentos de peso induzidos pelo consumo prolongado de níveis elevados de gordura poderão ter alterações na percepção do gosto doce