... Maximum redshift of the cosmic string detected by this method as a function of limiting magnitude (R band) of observations. is provided by the Numerical Galaxy Catalog ( GC) based on a N-body/semianalytic model with a -CDM cosmology, = 0.7, m = 0.3, 8 = 1 ...
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Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P1-9.pdf -- 221.0 Кб -- 27.08.2004 Похожие документы
... from a given instrument, the main challenge for the DFS pipeline is to create a unique infrastructure which can serve all of the more than 15 different instruments on the four 8.2 m telescopes plus ancillary units for interferometry and wide field imaging ...
... In the era of 8-m telescopes, there is increasing pressure to operate 4-m class telescopes in the most economic, efficient, and effective manner possible. ...
... Left for an 8m filled pupil, right for the notched GSFC design. sources to be selected and identified, and because the field will be accessible in general only for a few weeks, ob ject selection and the configuring data for the micro-mirror array have to ...
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Ссылки http://www.adass.org/adass/proceedings/adass97/reprints/rosam.pdf -- 109.5 Кб -- 14.04.1998 Похожие документы
... The VLT is a very large, complex facility which consists not only of four 8m telescop es, but also of several smaller auxiliary telescop es for interferometry. ...
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Ссылки http://www.adass.org/adass/proceedings/adass96/reprints/grosbolp.pdf -- 123.3 Кб -- 14.01.1998 Похожие документы
... 6 , C. Delattre2 , T. Deschamps2 , F-X. Dґ ert3, es P. Didelon2 , D. Elbaz2 , P. Gallais3, K. Ganga7 , S. Guest1,8 , G. Helou7 , M. Kong7 , F. Lacombe9 , D. Landriu2 , O. Laurent2 , P. Lecoupanec9 , J. Li7 , L. Metcalfe1 , K. Okumura1 , M. Pґ ault3, A ...
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Ссылки http://www.adass.org/adass/proceedings/adass97/reprints/otts.pdf -- 266.8 Кб -- 14.04.1998 Похожие документы
... Using the most sensitive instrumental configuration (the broad band filter LW2, covering a wavelength range between 58.5µm, and 6 PFOV), sources with a flux down to 0.5 mJy can be detected. ...
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Ссылки http://www.adass.org/adass/proceedings/adass02/reprints/O2-3.pdf -- 197.3 Кб -- 11.03.2003 Похожие документы
... GLIMPSE has used Montage as an engine to co-register 2MASS images in the J, H and K bands and MSX images at 8 µm. Montage: A Grid Enabled Image Mosaic Service 595 SWIRE will perform a wide area imaging survey of high galactic latitude fields to study the ...
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Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/O7-3.pdf -- 66.0 Кб -- 27.08.2004 Похожие документы