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EMU: Evolutionary Map of the Universe Ray Norris 13 September 2011
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Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden
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The VLTI view of compact dusty environments around evolved stars Olivier CHESNEAU Observatoire de la Côte dAzur (OCA)
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I. OUR OWN SUN (Space Climate School, Saariselka, March, 2009) Eric Priest (St Andrews)
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The Liverpool Telescope Chris Davis
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Page 1 Lecture 14 Part 1: AO System Optimization Part 2: How to be a savvy user and consumer of AO Claire Max Astro 289, UC Santa Cruz Feburary 21, 2013
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PLATO - TOU Thermal analyses Summary of previous thermal analyses performed in 2010-2011 S.Basso – F. Borsa (I.N.A.F. – Osservatorio Astronomico di Brera)
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Leiden 29 Nov 2001Harry van der Laan Symposium From Radio to X-ray Galaxy-Cluster-Galaxy From 1973 Lectures Ph D. thesis Radio Investigations of Cluster
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Star Properties. Apparent Magnitude System of Hipparchus Group of brightest stars1 m Stars about ½ as bright as 1 m 2 m Stars about ½ as bright as 2 m
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The Focusing Optics X-ray Solar Imager (FOXSI) Steven Christe 1, S. Krucker 2, L. Glesener 2, S. Ishikawa 3, B. Ramsey 4, T. Takahashi 3, R.P. Lin 2 1
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Red Planet Mars Chapter Thirteen. Introducing Astronomy (chap. 1-6) Introduction To Modern Astronomy I Planets and Moons (chap. 7-17) ASTR 111 – 003 Fall
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Radio and spectroscopic properties of miniature radio- galaxies: revealing the bulk of radio-loud AGN population Ranieri D. Baldi 1, and Alessandro Capetti
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