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    11. Adaptive smoothing
    ... 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 filaments on a bright background. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/asmooth/node11.html -- 9.9 Кб -- 02.07.2008
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    12. http://xmm.vilspa.esa.es/external/xmm_links/trainee/alumni/n_fonseca.pdf
    ... AGN emissions: Optical/UV band: "big blue bump" Accretion Disk IR band: thermal emission Dust (torus) Radio Jet X-ray Comptonization of disk photons Soft: 0.5-2keV Hard: 2-10keV Wide spectrum Emission in all bands An X-ray/radio sample of Active Galactic ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_links/trainee/alumni/n_fonseca.pdf -- 670.0 Кб -- 16.08.2006
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    13. http://xmm.vilspa.esa.es/scisim/release/latest/help/postscript/msim.ps
    ... The value fmult determines the ratio between successive f values. Dust is speci ed as the fractional coverage D of the surface by dust. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/scisim/release/latest/help/postscript/msim.ps -- 1150.7 Кб -- 12.01.2005
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    14. http://xmm.vilspa.esa.es/scisim/release/latest/config/telescope-3.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-3.cfg -- 9.5 Кб -- 12.01.2005
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    15. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0061-1-0.pdf
    ... the nebula has a significant dust-scattering halo22 which may scatter a wavelength ... probably a consequence Fe 0.456 0.019 0.00060 0.00003 17.39 0.05 of dust scattering ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0061-1-0.pdf -- 1023.2 Кб -- 10.11.2005
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    16. XMM Science Objectives
    ... of Hale-Bopp, evidence has been found that the X-ray emission arises from an interaction of Solar X-rays with cometary dust ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/user/sciobj/science_top1.html -- 30.1 Кб -- 24.09.1998
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    17. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-7.pdf
    ... The events are interpreted as a dust micrometeoroid scattered off the mirror surface ... most probably from interplanetary (or interstellar) dust but not linked to a meteor ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-7.pdf -- 1722.6 Кб -- 11.08.2008
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    18. http://xmm.vilspa.esa.es/sas/6.0.0/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/6.0.0/doc/asmooth.ps.gz -- 92.7 Кб -- 18.03.2004
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    19. http://xmm.vilspa.esa.es/sas/6.1.0/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/6.1.0/doc/asmooth.ps.gz -- 92.7 Кб -- 22.11.2004
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    20. http://xmm.vilspa.esa.es/sas/6.5.0/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/6.5.0/doc/asmooth.ps.gz -- 92.8 Кб -- 16.08.2005
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