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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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- Article
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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.
Early Recordings of Jewish Music in Poland
- from IN PRE-WAR POLAND
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- By Michael Aylward, He is also currently working on an anthology of travellers' accounts of Jewish life in Europe.
- Edited by Michael C. Steinlauf, Antony Polonsky, Brandeis University, Massachusetts
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- Book:
- Focusing on Jewish Popular Culture and Its Afterlife
- Published by:
- Liverpool University Press
- Published online:
- 23 November 2019
- Print publication:
- 01 November 2003, pp 59-70
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Summary
FOR seven years I have been working on a discography of commercial recordings of Jewish music made in Europe on cylinders and shellac records. This project has now progressed sufficiently for a work-in-progress report to be issued. I will initially give a general account of the discography as it stands at present and then concentrate on those aspects that apply especially to Poland.
OVERVIEW OF THE DISCOGRAPHY
The aim of the project is to document as far as possible all commercial recordings of Jewish music made in Europe on cylinders or shellac records (broadly speaking, 78 rpm records). When complete, this discography will list them all, together with all standard discographical details such as record label, catalogue number, matrix number, disc size, artist name and title of recording (together with details of composers and arrangers where these are given), precise recording date and recording location, name of recording engineer, and details of any records on which the original recording was later reissued. Every effort will also be made to provide artist biographies and additional information of interest.
The range of musical genres covered by the discography is wide, but may be broadly defined as applying to traditional Jewish music. For example, it excludes works by Jewish composers working in the European classical tradition; art music, even if specifically Jewish in tone and content; and non-Jewish music performed by Jewish artists. It does, however, extend to non-musical recordings such as comic monologues and dramatic recitals. In addition, there are separate appendices dealing with categories such as ‘Jewish’ music performed by non-Jewish artists1 and Jewish parodies performed by non-Jewish artists, the latter a fairly common genre among pre-revolutionary Russian recordings, but rare in Polish ones of the same era.
Tables 1 and 2 give a snapshot of the discography as it currently stands. Although enlightening, they by no means give a representative picture. This is merely a view taken at a particular point in time of a project that is constantly evolving and will, by the time this chapter is published, be hopelessly out of date. The data recorded in these tables is based only on those recordings that have so far been entered onto the database.
When does Huntington's disease begin?
- JEFFREY R. CAMPODONICO, ELIZABETH AYLWARD, ANN-MARIE CODORI, CANDACE YOUNG, LAURA KRAFFT, MICHAEL MAGDALINSKI, NEAL RANEN, PHILLIP R. SLAVNEY, JASON BRANDT
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- Journal:
- Journal of the International Neuropsychological Society / Volume 4 / Issue 5 / September 1998
- Published online by Cambridge University Press:
- 01 September 1998, pp. 467-473
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Recent studies have detected basal ganglia atrophy in clinically asymptomatic persons with the genetic mutation that causes Huntington's disease (HD). Whether reductions in caudate and putamen volume on MRI scans are associated with changes in cognitive and neurologic functioning was examined in 13 healthy adults with the IT-15 mutation. Reduced striatal volume was found to correlate with greater neurologic (largely motor) impairment, slower mental processing speed, and poorer verbal learning, although none of the participants met even liberal criteria for clinical diagnosis of HD. These correlations are strikingly similar to those observed in symptomatic HD patients, possibly reflecting the earliest manifestations of disease. (JINS, 1998, 4, 467–473.)