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    41. http://www.adass.org/adass/proceedings/adass03/reprints/P1-9.pdf
    ... 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 ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P1-9.pdf -- 221.0 Кб -- 27.08.2004
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    42. Pipeline Processing of Data in the VLT Era
    ... 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 ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass98/grosbolp/ -- 13.5 Кб -- 16.07.1999
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    43. GIGAWULF: Powering the Isaac Newton Group's Data Pipeline
    ... 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. ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass00/O8-04/ -- 15.3 Кб -- 29.05.2001
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    44. http://www.adass.org/adass/proceedings/adass03/reprints/P6-6.pdf
    ... 1. The resolution of this image on the sky is ab out 0.1 ", i.e. diffraction limited for a 8-m telescop e in the L-band. ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P6-6.pdf -- 581.0 Кб -- 30.08.2004
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    45. http://www.adass.org/adass/proceedings/adass98/reprints/marism1.pdf
    ... o g th sl v 8h ©q o l G ej Y f Tk ej ©m Vo f ¶i ё m pi ih tr l «f Tq 8 Tv gj 8g ©q o Tk ej ©m o Uq Yi sm cq Ѕ Ц |ч ¶Д |Ц А ёч Б ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass98/reprints/marism1.pdf -- 151.0 Кб -- 16.07.1999
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    46. http://www.adass.org/adass/proceedings/adass97/reprints/rosam.pdf
    ... Left for an 8 m 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 ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass97/reprints/rosam.pdf -- 109.5 Кб -- 14.04.1998
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    47. http://www.adass.org/adass/proceedings/adass96/reprints/grosbolp.pdf
    ... The VLT is a very large, complex facility which consists not only of four 8 m telescop es, but also of several smaller auxiliary telescop es for interferometry. ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass96/reprints/grosbolp.pdf -- 123.3 Кб -- 14.01.1998
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    48. http://www.adass.org/adass/proceedings/adass97/reprints/otts.pdf
    ... 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 ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass97/reprints/otts.pdf -- 266.8 Кб -- 14.04.1998
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    49. http://www.adass.org/adass/proceedings/adass02/reprints/O2-3.pdf
    ... 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. ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass02/reprints/O2-3.pdf -- 197.3 Кб -- 11.03.2003
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    50. http://www.adass.org/adass/proceedings/adass03/reprints/O7-3.pdf
    ... 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 ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/O7-3.pdf -- 66.0 Кб -- 27.08.2004
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