... II: 30њ < declination < 51њ, 08 h 30 m < right ascension < 17 h 30 m . Hales et al. ... III: 48њ < declination < 68њ, 05 h 25 m < right ascension < 18 h 17m . ... 01 h 34 m < right ascension < 6 h 14 m and 17 h 16 m < right ascension < 20 h 24 m ...
... II: 30ТА < declination < 51ТА, 08 h 30 m < right ascension < 17 h 30 m . ... III: 48ТА < declination < 68ТА, 05 h 25 m < right ascension < 18 h 17m . ... 01 h 34 m < right ascension < 6 h 14 m and 17 h 16 m < right ascension < 20 h 24 m ...
... We nd good agreement on cosmologi- cal parameters between galaxy velocities, CMB and Type 1a su- pernovae with 95 per cent con dence limits 0:64 < h < 0:86, 0:17 < m < 0:39 and 0:98 < 8 < 1:37. ...
... 00 11:30 12:30 13:45 Introduction to synthesis imaging and calibration Part II (Tony Willis ) 14:45 15:45 16:15 17:15 M. Introduction to Scientific motivation for 9:00 Registration Break synthesis imaging and deep field imaging 9:30 Welcome talk (30 mins ...
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Ссылки http://www.mrao.cam.ac.uk/projects/skads/mcct/mcct_timetable.pdf -- 120.3 Кб -- 14.08.2008 Похожие документы
... We see that the effect this change on dust emission is to enhance emission at 17 µm when a greater ° fraction of the carbon nuclei are placed in the 3.5 A peak, while reducing emission at 17 µm. A pivoting motion is seen around 17 µm, where the ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2008/dustgal1.pdf -- 1286.9 Кб -- 25.11.2009 Похожие документы