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    • Пред. | 1 | 2 | 3

    21. http://xmm.vilspa.esa.es/sas/7.0.0/doc/asmooth.ps.gz
    ... This implies that the detail which one wishes to preserve from smoothing should be bright rather than dark - it would not be advisable, for example, to adaptively smooth an image of absorbing dust laments on a bright background. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/7.0.0/doc/asmooth.ps.gz -- 93.2 Кб -- 28.06.2006
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    22. http://xmm.vilspa.esa.es/sas/7.1.0/doc/asmooth.ps.gz
    ... This implies that the detail which one wishes to preserve from smoothing should be bright rather than dark - it would not be advisable, for example, to adaptively smooth an image of absorbing dust laments on a bright background. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/asmooth.ps.gz -- 93.1 Кб -- 09.07.2007
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    23. http://xmm.vilspa.esa.es/sas/8.0.0/doc/asmooth.ps.gz
    ... This implies that the detail which one wishes to preserve from smoothing should be bright rather than dark - it would not be advisable, for example, to adaptively smooth an image of absorbing dust laments on a bright background. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/asmooth.ps.gz -- 93.0 Кб -- 02.07.2008
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    24. http://xmm.vilspa.esa.es/scisim/release/latest/config/telescope-1.cfg
    ... 2 # reflections other than mirror shells reflectCoefficient 1 # take reflection coeff into account, 0/1 reflectDust 1 # use dust shadowing, 0/1 reflectTransmission 1 # use transmission table, 0/1 disteps 1e-7 # distance tolerance (mm) parabolicRollOff 1 ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/scisim/release/latest/config/telescope-1.cfg -- 32.3 Кб -- 12.01.2005
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    25. http://xmm.vilspa.esa.es/scisim/release/latest/config/telescope-2.cfg
    ... 2 # reflections other than mirror shells reflectCoefficient 1 # take reflection coeff into account, 0/1 reflectDust 1 # use dust shadowing, 0/1 reflectTransmission 1 # use transmission table, 0/1 disteps 1e-7 # distance tolerance (mm) parabolicRollOff 1 ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/scisim/release/latest/config/telescope-2.cfg -- 32.3 Кб -- 12.01.2005
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    26. http://xmm.vilspa.esa.es/sched_tour/too_paper.pdf
    ... If GRB's are indeed associated with massive progenitors and therefore lie in regions of star formation, it is likely that in a large fraction of events, the optical emission is heavily absorbed by dust. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sched_tour/too_paper.pdf -- 30.7 Кб -- 07.11.2001
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    27. http://xmm.vilspa.esa.es/external/xmm_sched/sched_tour/ESA_bulletin_107.pdf
    ... If GRBs are indeed associated with massive progenitors and therefore lie in regions of star formation, it is likely that in a large fraction of events the optical emission is heavily absorbed by dust. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_sched/sched_tour/ESA_bulletin_107.pdf -- 881.3 Кб -- 13.04.2004
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    28. http://xmm.vilspa.esa.es/scisim/release/latest/config/scisim.cfg
    ... Faster, same accuracy debugGapGuess 0 # write debug file with Guess gap info end rfcdot_config begin estimatedRays 0 # dummy illumArea 0 # dummy illumRays 0 # dummy raytraceMode 1 seed 0 # seed for photonmode transform 1 # whether ... rotation...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/scisim/release/latest/config/scisim.cfg -- 65.7 Кб -- 13.01.2005
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    29. http://xmm.vilspa.esa.es/scisim/release/latest/data/msim/fm1model.dat.v2_0_2
    ; Model file automatically generated from fm1.config medium gold begin ; gold index of refraction table ; < 100 eV from D.W. Lynch and W.R. Hunter, Optical Constants of Metals, ; in Handbook op Optical Constants of Solids, ed. E.D. Palik, ; Academic...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/scisim/release/latest/data/msim/fm1model.dat.v2_0_2 -- 268.7 Кб -- 12.01.2005
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    Пред. | 1 | 2 | 3

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