... observations was to determine which of the sources in the VSOP continuum list were sufficiently strong on the longest VLBA baseline (usually MK-SC, MaunaKea to Saint Croix) for probable detection in a typical HALCA observation (detection level is ~0.1 Jy ...
... 2011 CCD в Polarizer2 -- after July 2011 (new polarizer) b Three atmospheric extinction wavelength dependences are used: 1) no atmosphere (or "gray" atmosphere) ; 2) Atmospheric extinction properties above MaunaKea (Buton et al. 2013) for air mass unity ...
... A few phone calls later, McDonald Observatory and MaunaKea Observatory were able to mimic Irv's alignment and achieve success with ranging Tranquility Base. ...
... Разглаядеть новую планету удалось с помощью телескопа Samuel Oschin в обсерватории Паломар (Palomar) и 8-метрового телескопа Gemini North в обсерватории (MaunaKea). ...
... The planet was discovered by Brown, Chad Trujillo of the Gemini Observatory in MaunaKea, Hawaii, and David Rabinowitz of Yale University in New Haven, Conn. ...
... and mm-bands (Effelsberg and Metsahovi radio teleи scopes, IRAM (Plateau de Bure and Pico Veleta), and the Smithsonian Submillimeter Array at MaunaKea), in near-IR and optical bands by a WEBT campaign, and additional high-energy coverage (UV, X-rays) by ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/D35_Collmar01-27Feb07_19:21:51.pdf -- 260.7 Кб -- 27.02.2007 Похожие документы
... WFCAM uses the existing UKIRT telescope on MaunaKea Hawaii from late 2004, whereas VISTA was designed as a single purpose survey facility l ocated at ESO's Cerro Paranal Observator y in Chile from late 2006. ...
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Ссылки http://www.vista.ac.uk/Files/docs/vdfs/spie-5493-30_VDFS-Overview.pdf -- 144.7 Кб -- 20.04.2011 Похожие документы