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Multicolor Active Galactic Nuclei Monitoring : ウィキペディア英語版 | Multicolor Active Galactic Nuclei Monitoring Multicolor Active Galactic Nuclei Monitoring or MAGNUM was a project completed in 2008, that used a 2 meter (78.7 inch) telescope at Haleakala, Hawaii. The project started in 1995, and with telescope observations starting in 2000 for the scientific study of active galactic nuclei.〔http://adsabs.harvard.edu/abs/2003AAS...202.3803Y〕 It was run by the University of Tokyo, the National Astronomical Observatory of Japan, and Australian National University.〔〔http://www.ifa.hawaii.edu/info/press-releases/GRB-09-05.htm〕 MAGNUM was one of the telescopes that observed a cosmic explosion billions of years away in 2005.〔http://www.redorbit.com/news/space/239453/hawaii_telescopes_record_cosmic_explosion/〕 The telescope was used for a long-term study of the size of the universe;〔http://archives.starbulletin.com/2004/07/25/news/story4.html〕 for example it studied the Seyfert 1 galaxies NGC 5548, NGC 4051, NGC 3227, and NGC 7469〔http://www.journals.uchicago.edu/doi/abs/10.1086/499326 ''The Astrophysical Journal'', 639:46–63, 2006 March 1 "Reverberation Measurements of the Inner Radius of the Dust Torus in Nearby Seyfert 1 Galaxies"〕 The telescope was located at the Haleakala Observatory and was installed in north dome previously used by LURE.〔 == References ==
抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「Multicolor Active Galactic Nuclei Monitoring」の詳細全文を読む
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