О»ї . Publiц© le 26/02/2014 par Aurц©lien Lepanot . Date : 23/02/2014 . Lieu : Besanц§on . Matц©riel de prise de vue : Telescope Newton Orion 203/1000 - imageur: Webcam Philips SPC900NC flashц© + Powermate X5 . Commentaires : Une jupiter capturц©e avec la petite webcam Philips SPC900 comme quoi une config modeste peut faire des miracles :) . Date : 23/02/2014 . Lieu : Besanц§on . Matц©riel de prise de vue : Telescope Newton Orion 203/1000 - imageur: Webcam Philips SPC900NC flashц© + Powermate X5 .

... The first book is about observing ­ really a great "how to" guide designed to make one aware of all that can be fine tuned with respect to observing skills. ... For any of you who attended Bill Murray's excellent talk at our March meeting this is a "must read." ... We are truly fortunate to be able to mark the conclusion of the 2002 ­ 2003 series of meetings at Peyton Hall by having as a guest speaker, Dr David N. Spergel of Princeton University's Department of Astrophysical Sciences. ...

... 2 Telescop e finder Do not rely on that the nominal alignment of coordinate system Auto Alignment made on stars will serve a long time. ... The Meade telesc tages: 1) there is no possibility to common error in the telescope soft system, when telescope moving in ope parking using command :hP# has the following disadvanobtain information on the completion of this procedure, 2) a often leads to tripping-over a limiter and to loss of coordinate a horizontal coordinate system. ... Home Position. ...

... 295, 2003 H. E. Payne, R. I. Jedrzejewski, and R. N. Hook, eds. The COBRA/CARMA Correlator Data Pro cessing System Stephen L. Scott1 , Rick Hobbs1 , Andrew D. Beard1 , Paul Daniel1 , David M. Mehringer2 , Raymond Plante2 , J. Colby Kraybill3 , Melvyn Wright3 , Erik Leitch4 , N. S. Amarnath5 , Marc W. Pound5 , Kevin P. Rauch5 , Peter J. Teuben5 Abstract. ... The COBRA hardware and computing architecture described here will be the basis for the two CARMA correlators. ... CARMA Scott et al. ... 2003). ...

Rep ort by the ESA-ESO Working Group on Galactic p opulations, chemistry and dynamics Abstract Between the early 40s, when Baade showed the first evidence for the existence of two distinct stellar populations, and today, with our Galaxy surprising us with new substructures discovered almost on a monthly basis, it is clear that a remarkable progress has been achieved in our understanding of the Galaxy, of its structure and stellar populations, and of its chemical and dynamical signatures. Yet, some questions