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    11. Photometric Performance of NICMOS
    ... The absolute calibration of the ultraviolet and optical instruments onboard HST is based on the existence of absolute flux ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node11.html -- 33.3 Кб -- 12.06.2006
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    12. Pipeline Processing and Quality Control for Echelle Data
    ... In order to verify if a pipeline was feasible for echelle data, in particular for UVES (Ultraviolet-Visible Echelle Spectrograph), a test on EMMI (ESO Multi-Mode Instrument) data acquired in echelle mode and extracted from the NTT archive was performed: . ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/morganteg.html -- 12.5 Кб -- 12.06.2006
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    13. 2048 x 2048 HgCdTe Arrays for Astronomy at Visible and Infrared Wavelengths
    ... could also be hybridized to Si PIN diode arrays, providing sensitivity down through the visible into the ultraviolet ... wavelengths as long as17 m, thus providing the option of wavelength coverage from the ultraviolet through much of the MIR ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node39.html -- 35.2 Кб -- 12.06.2006
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    14. http://www.stecf.org/conferences/adass/adassVII/reprints/polubekg.ps.gz
    ... We present a computer program for modelling energy flux distribution and light curves of eclipsing binaries from far ultraviolet to infrared regions. ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/polubekg.ps.gz -- 194.4 Кб -- 12.06.2006
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    15. A Posteriori Guidance for Astronomical Images
    ... Astronomical ultraviolet images were obtained from a balloon-borne telescope equipped with a photon-counting detector. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/llebariaa.html -- 16.0 Кб -- 12.06.2006
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    16. OPUS-97: A Generalized Operational Pipeline System
    ... 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. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/rosej.html -- 13.8 Кб -- 12.06.2006
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    17. http://www.stecf.org/conferences/adass/adassVII/reprints/morganteg.pdf
    ... In order to verify if a pipeline was feasible for echelle data, in particular for UVES1 (Ultraviolet-Visible Echelle Spectrograph), a test on EMMI2 (ESO Multi-Mode Instrument) data acquired in echelle mode and extracted from the NTT archive was performed ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/morganteg.pdf -- 101.7 Кб -- 12.06.2006
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    18. http://www.stecf.org/conferences/adass/adassVII/reprints/morganteg.ps.gz
    ... In order to verify if a pipeline was feasible for echelle data, in particular for UVES 1 (Ultraviolet­Visible Echelle Spectrograph), a test on EMMI 2 (ESO Multi­Mode Instrument) data acquired in echelle mode and extracted from the NTT archive was ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/morganteg.ps.gz -- 89.0 Кб -- 12.06.2006
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    19. A Color Analysis of NICMOS Parallel Observations
    ... Our efforts to derive object colors are not yet complete, and in particular we are currently working on deriving the colors of high-redshift supernovae using their optical and ultraviolet spectra. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node28.html -- 19.5 Кб -- 12.06.2006
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    20. http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/dickinson04.pdf
    ... with fainter luminosities, higher space density, and similar comoving ultraviolet emissivity to that at z p 3, but this depends ...
    [ Текст ]  Ссылки http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/dickinson04.pdf -- 1221.6 Кб -- 16.09.2004
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