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List of contributors
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- By Sefanja Achterberg, James A. Adams, Angelika Alonso, Bettina Anders, Ana Patrícia Antunes, Johannes Binder, Manuel Bolognese, Louis R. Caplan, Paolo Costa, Sofie De Blauwe, Exuperio Díez-Tejedor, Philipp Eisele, Alex Förster, Blanca Fuentes, Ruth Geraldes, Martin Griebe, Valentin Held, Gregory Helsen, Michael G. Hennerici, Eva Hornberger, Micha Kablau, L. Jaap Kappelle, Rolf Kern, Patricia Martínez-Sánchez, Tilman Menzel, Nadja Meyer, Caroline Ottomeyer, Suzanne Persoon, Alessandro Pezzini, Miriam M. Pfeiffer, Björn Reuter, Katlijn Schotsmans, Christopher Schwarzbach, Markus Stürmlinger, Kristina Szabo, Tiago Teodoro, Ralph Werner, Johannes C. Wöhrle, Marc Wolf
- Edited by Michael G. Hennerici, Ruprecht-Karls-Universität Heidelberg, Germany, Rolf Kern, Ruprecht-Karls-Universität Heidelberg, Germany, Louis R. Caplan, Kristina Szabo, Ruprecht-Karls-Universität Heidelberg, Germany
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- Book:
- More Case Studies in Stroke
- Published online:
- 05 June 2014
- Print publication:
- 15 May 2014, pp ix-xii
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The science of EChO
- Giovanna Tinetti, James Y-K. Cho, Caitlin A. Griffith, Olivier Grasset, Lee Grenfell, Tristan Guillot, Tommi T. Koskinen, Julianne I. Moses, David Pinfield, Jonathan Tennyson, Marcell Tessenyi, Robin Wordsworth, Alan Aylward, Roy van Boekel, Angioletta Coradini, Therese Encrenaz, Ignas Snellen, Maria R. Zapatero-Osorio, Jeroen Bouwman, Vincent Coudé du Foresto, Mercedes Lopez-Morales, Ingo Mueller-Wodarg, Enric Pallé, Franck Selsis, Alessandro Sozzetti, Jean-Philippe Beaulieu, Thomas Henning, Michael Meyer, Giuseppina Micela, Ignasi Ribas, Daphne Stam, Mark Swain, Oliver Krause, Marc Ollivier, Emanuele Pace, Bruce Swinyard, Peter A.R. Ade, Nick Achilleos, Alberto Adriani, Craig B. Agnor, Cristina Afonso, Carlos Allende Prieto, Gaspar Bakos, Robert J. Barber, Michael Barlow, Peter Bernath, Bruno Bézard, Pascal Bordé, Linda R. Brown, Arnaud Cassan, Céline Cavarroc, Angela Ciaravella, Charles Cockell, Athéna Coustenis, Camilla Danielski, Leen Decin, Remco De Kok, Olivier Demangeon, Pieter Deroo, Peter Doel, Pierre Drossart, Leigh N. Fletcher, Matteo Focardi, Francois Forget, Steve Fossey, Pascal Fouqué, James Frith, Marina Galand, Patrick Gaulme, Jonay I. González Hernández, Davide Grassi, Matt J. Griffin, Ulrich Grözinger, Manuel Guedel, Pactrick Guio, Olivier Hainaut, Robert Hargreaves, Peter H. Hauschildt, Kevin Heng, David Heyrovsky, Ricardo Hueso, Pat Irwin, Lisa Kaltenegger, Patrick Kervella, David Kipping, Geza Kovacs, Antonino La Barbera, Helmut Lammer, Emmanuel Lellouch, Giuseppe Leto, Mercedes Lopez Morales, Miguel A. Lopez Valverde, Manuel Lopez-Puertas, Christophe Lovi, Antonio Maggio, Jean-Pierre Maillard, Jesus Maldonado Prado, Jean-Baptiste Marquette, Francisco J. Martin-Torres, Pierre Maxted, Steve Miller, Sergio Molinari, David Montes, Amaya Moro-Martin, Olivier Mousis, Napoléon Nguyen Tuong, Richard Nelson, Glenn S. Orton, Eric Pantin, Enzo Pascale, Stefano Pezzuto, Ennio Poretti, Raman Prinja, Loredana Prisinzano, Jean-Michel Réess, Ansgar Reiners, Benjamin Samuel, Jorge Sanz Forcada, Dimitar Sasselov, Giorgio Savini, Bruno Sicardy, Alan Smith, Lars Stixrude, Giovanni Strazzulla, Gautam Vasisht, Sandrine Vinatier, Serena Viti, Ingo Waldmann, Glenn J. White, Thomas Widemann, Roger Yelle, Yuk Yung, Sergey Yurchenko
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- Journal:
- Proceedings of the International Astronomical Union / Volume 6 / Issue S276 / October 2010
- Published online by Cambridge University Press:
- 10 November 2011, pp. 359-370
- Print publication:
- October 2010
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The science of extra-solar planets is one of the most rapidly changing areas of astrophysics and since 1995 the number of planets known has increased by almost two orders of magnitude. A combination of ground-based surveys and dedicated space missions has resulted in 560-plus planets being detected, and over 1200 that await confirmation. NASA's Kepler mission has opened up the possibility of discovering Earth-like planets in the habitable zone around some of the 100,000 stars it is surveying during its 3 to 4-year lifetime. The new ESA's Gaia mission is expected to discover thousands of new planets around stars within 200 parsecs of the Sun. The key challenge now is moving on from discovery, important though that remains, to characterisation: what are these planets actually like, and why are they as they are?
In the past ten years, we have learned how to obtain the first spectra of exoplanets using transit transmission and emission spectroscopy. With the high stability of Spitzer, Hubble, and large ground-based telescopes the spectra of bright close-in massive planets can be obtained and species like water vapour, methane, carbon monoxide and dioxide have been detected. With transit science came the first tangible remote sensing of these planetary bodies and so one can start to extrapolate from what has been learnt from Solar System probes to what one might plan to learn about their faraway siblings. As we learn more about the atmospheres, surfaces and near-surfaces of these remote bodies, we will begin to build up a clearer picture of their construction, history and suitability for life.
The Exoplanet Characterisation Observatory, EChO, will be the first dedicated mission to investigate the physics and chemistry of Exoplanetary Atmospheres. By characterising spectroscopically more bodies in different environments we will take detailed planetology out of the Solar System and into the Galaxy as a whole.
EChO has now been selected by the European Space Agency to be assessed as one of four M3 mission candidates.
Abondance des mouches des fruits dans les zones de production fruitières de Côte d’Ivoire : dynamique des populations de Bactrocera invadens (Diptera : Tephritidae)
- Ossey Robert N’Dépo, N’klo Hala, Kouassi Allou, Louis Roi Aboua, Kouassi Philippe Kouassi, Jean-François Vayssières, Marc De Meyer
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Introduction. L’objectif de notre étude a été de recenser les différentes espèces de Tephritidae présentes sur arbres fruitiers dans trois régions climatiques différentes de Côte d’Ivoire et d’identifier quelques plantes hôtes auxquelles elles sont associées. Matériel et méthodes. Un dispositif de pièges utilisant différentes phéromones a été mis en place dans les régions agro écologiques du sud (Azaguié, Abidjan) et du centre (Yamoussoukro) de la Côte d’Ivoire entre juin 2005 et septembre 2006. En complément, une collecte de fruits a été effectuée dans ces mêmes régions ainsi qu’au nord du pays (Korhogo). La fluctuation de la population de Bactrocera invadens a été suivie à partir de relevés hebdomadaires des pièges. Les mouches émergées des fruits collectés ont été identifiées et comptées. Résultats et discussion. Au total, 23 espèces de mouches des fruits ont été identifiées dont huit espèces particulières à Azaguié, une espèce à Abidjan et une espèce à Yamoussoukro. Les espèces B. invadens et D. mediovittatus ont été identifiées pour la première fois en Côte d’Ivoire. L’espèce B. invadens s’est révélée majoritaire sur les stations du sud et du centre de la Côte d’Ivoire. Elle est représentée à 85 % à Azaguié, à 99,90 % à Abidjan et à 95,40 % à Yamoussoukro. Le méthyl eugénol et le dorsalure ont été les plus efficaces pour capturer un grand nombre d’individus. Les genres Ceratitis et Dacus, bien que présentant une diversité spécifique, sont faiblement représentés sur les sites expérimentaux étudiés. Selon les zones agro écologiques et la période de fructification des manguiers en Côte d’Ivoire, les populations de B. invadens présentent différents pics de croissance. Conclusion. Des études complémentaires sur la biologie et le comportement de ce ravageur s’avéreront nécessaires pour l’application des méthodes de lutte optimale en vergers en Afrique de l’Ouest et, plus particulièrement, en Côte d’Ivoire.
Design of an ecologically-based IPM program for fruit flies (Diptera: Tephritidae) in Tanzania
- Maulid W. Mwatawala, Marc De Meyer, Rhodes H. Makundi, Amon P. Maerere
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Introduction. Studies to determine the pre-requisites for formulating an IPM program for fruit flies (Diptera: Tephritidae) were conducted in the Morogoro region, Central Tanzania, from 2004 to 2006. Specifically, studies aimed at determining the biodiversity of fruit flies, and their incidence and abundance in the surveyed region. Materials and methods. Adult flies were collected using McPhail traps baited with parapheromones (methyl eugenol, trimedlure and cue lure) and synthetic food baits (hydrolyzed yeast and three-component lure). Flies were also collected from infested fruits after incubation in the laboratory. A total of four sites and neighboring areas representing the three agro-ecological zones of Morogoro region were used. Results. Two key fruit fly pests were determined based on incidence in major fruits and their seasonal abundance. The invasive fruit fly, Bactrocera invadens Drew, Tsuruta and White, is the key pest in the low and medium altitude areas. On the other hand, the Natal fruit fly, Ceratitis rosa Karsch, is the key frugivorous pest in the high altitude areas. Discussion. Management programs of fruit flies need to focus on key pests, taking into consideration their breeding in the non-agricultural habitats. Components of such a program should include the Male Annihilation Technique (MAT), legislation, use of parapheromones and baits, farm hygiene and sanitation, quarantine, surveillance and postharvest treatment.
Biodiversity of fruit flies (Diptera, Tephritidae) in orchards in different agro-ecological zones of the Morogoro region, Tanzania
- Maulid W. Mwatawala, Marc De Meyer, Rhodes H. Makundi, Amon P. Maerere
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Introduction. Fruit flies (Diptera, Tephritidae) are among the major constraints in commercial horticulture in many African developing countries. Knowledge of the tephritid spectrum in any given area is a prerequisite for the development of an IPM program to alleviate the pest problem. We studied the fruit fly diversity in four main agro-ecological zones which are significant fruit-producing areas in the Morogoro Region, Tanzania. Materials and methods. Fruit fly diversity was investigated for one year (October 2004 – October 2005). Parapheromones, synthetic food attractant and protein-bait traps were used to trap the flies at the different locations in Morogoro region, Tanzania. One mixed orchard was selected at each of four locations representing the different agro-ecological zones of the region. Results. The recently introduced alien species, Bactrocera invadens, and three indigenous pest species, Ceratitis rosa, Dacus bivittatus and D. punctatifrons, were found at all the four sites, while Bactrocera cucurbitae, Ceratitis cosyra, Dacus chiwira and D. humeralis were found in three out of the four sites. The Sokoine University of Agriculture (SUA) Horticulture Unit and Mikese sites had the highest species diversity while the Mkindo and Nyandira sites had the lowest diversity. The between-habitats diversity (Beta diversity) was similar among the SUA, Mkindo and Mikese sites. Only the Nyandira site had a higher dissimilarity in comparison with the other three sites. Discussion. The most abundant species at low- and mid-elevation sites was Bactrocera invadens while, at high elevation, Ceratitis rosa was the dominant species. Protein-baited traps attracted the highest diversity of fruit flies in comparison with the more specific parapheromones. The synthetic food attractant (three-component lure) was less efficient compared with the protein bait. The large dissimilarity at the Nyandira site is probably due to the different types of host fruits found and grown in high altitude areas (mainly temperate fruits). Fruit fly species associated with these types of fruits, e.g., Ceratitis rubivora and Trirhithrum coffeae, were found only at this site.
Sequential Bone Response to Immediately Loaded Mini-Implants, in vivo Study
- Glaucio Serra Guimarães, Liliane Siqueira de Morais, Carlos Nelson Elias, Marc Andre Meyers
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- Journal:
- MRS Online Proceedings Library Archive / Volume 925 / 2006
- Published online by Cambridge University Press:
- 01 February 2011, 0925-BB03-07
- Print publication:
- 2006
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The use of osseointegrated titanium implants has been related like an excellent alternative to traditional orthodontic anchorage methodologies, and they are a necessity when dental elements lack quantity or quality, when extraoral devices are impractical, or when noncompliance during treatment is likely. In orthodontics, the implants can be use to anchor different movements. However, conventional dental implants can only be placed in limited areas such as the retromolar or the edentulous areas. Another limitation has been the direction of the force application and conventional dental implants are troublesome for patients because of the severity of the surgery, the discomfort of the initial healing, and the difficulty of oral hygiene. Due to these factors, mini-implants became widely used. They have little limitations related to the local of implantation, the surgical procedure of insertion is relatively simple and the control of direction and quantify of the force is simple to be done. These improvements were obtained due to decrease of the size, but these changes could result on significant changes to the bone-implant interface. Since, the orthodontic treatment has to be done as fast as possible. The purpose of this work is to analyze the bone healing reactions to immediately loaded mini-implant of titanium alloy grade 4 by histological, fluorescent and SEM observation, by histomorphometric analysis and by removal torque test. Material and method: Seventy two mini-implants were inserted in eighteen New Zealand rabbits. Four mini-implants were put in the right tibiae of each rabbit and two of then were loaded immediately with 100 gf. Subcutaneous injections of fluorescent labels were administrated in defined periods. The animals were euthanized after 1, 4 and 12 weeks, performing three time analysis and the tibias were dissected and prepared to microcopy analysis and to removal torque test. Results: The results indicated that all the mini-implants remained stable during experimental time. The SEM findings indicated no differences between load and unload group in one and four weeks period, although, the 12 weeks loaded group demonstrated more mature bone formation than the unload group in the same time. These findings suggest that the force can be applied after insertion of the mini-implant without compromises their stability.