EMU: Evolutionary Map of the Universe Ray Norris 13 September 2011.
Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.
The VLTI view of compact dusty environments around evolved stars Olivier CHESNEAU Observatoire de la Côte dAzur (OCA)
I. OUR OWN SUN (Space Climate School, Saariselka, March, 2009) Eric Priest (St Andrews)
The Liverpool Telescope Chris Davis .
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.
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)
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.
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.
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.
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.
Radio and spectroscopic properties of miniature radio- galaxies: revealing the bulk of radio-loud AGN population Ranieri D. Baldi 1, and Alessandro Capetti.