... The FUSE (Far Ultraviolet Spectrographic Explorer) team selected OPUS for their pipeline even though they will be receiving only a moderate amount of data that will processed on a single workstation. ...
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Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/rosej.pdf -- 89.7 Кб -- 12.06.2006 Похожие документы
... The FUSE (Far Ultraviolet Spectrographic Explorer) team selected OPUS for their pipeline even though they will be receiving only a moderate amount of data that will processed on a single workstation. ...
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Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/rosej.ps.gz -- 77.7 Кб -- 12.06.2006 Похожие документы
... F., Fontana A., Giallongo E., 1999, MNRAS, 310, 540 Bruzual, G., Charlot, S., 2001 (GISSEL) in preparation Calzetti D., 1997, in Waller W.H. et al. eds., The Ultraviolet Universe at Low and High Redshift: Probing the Progress of Galaxy Evolution, AIP Conf ...
... Facilities · Soft X-rays and far ultraviolet space observatories · Far infrared observatory with very high resolution ... census of the (cold) gas content · X-ray and far ultraviolet space missions for a census of the hot gas content · Direct ...
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Ссылки http://www.stecf.org/coordination/esa_eso/galpops/report.pdf -- 2038.4 Кб -- 04.09.2008 Похожие документы
Report by the ESA-ESO Working Group on Fundamental Cosmology Abstract In September 2003, the executives of ESO and ESA agreed to establish a number of working groups to explore possible synergies between these two major European astronomical...
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Ссылки http://www.stecf.org/coordination/esa_eso/cosmology/report.pdf -- 1894.6 Кб -- 04.09.2008 Похожие документы
... Using HST/ACS, it has probed the rest-frame ultraviolet (UV) to optical portion of high-redshift galaxies through obser- vations in the F435W , F606W , F775W , and F850LP bandpasses, with a goal of achieving extended source sen- sitivities only 0.5{0.8 ...
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Ссылки http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/strolger04.ps -- 1023.9 Кб -- 16.09.2004 Похожие документы