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    71. http://xmm.vilspa.esa.es/sas/6.5.0/doc/epicbscalgen.ps.gz
    ... Formally, the IBS is de ned as follows:  The +X axis points along the optical axis of the telescope of the respective instrument from the focal plane into the sky. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/6.5.0/doc/epicbscalgen.ps.gz -- 79.3 Кб -- 16.08.2005
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    72. http://xmm.vilspa.esa.es/sas/7.0.0/doc/epicbscalgen.ps.gz
    ... Formally, the IBS is de ned as follows:  The +X axis points along the optical axis of the telescope of the respective instrument from the focal plane into the sky. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/7.0.0/doc/epicbscalgen.ps.gz -- 79.1 Кб -- 28.06.2006
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    73. http://xmm.vilspa.esa.es/sas/7.1.0/doc/epicbscalgen.ps.gz
    ... Formally, the IBS is de ned as follows:  The +X axis points along the optical axis of the telescope of the respective instrument from the focal plane into the sky. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/epicbscalgen.ps.gz -- 79.1 Кб -- 09.07.2007
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    74. http://xmm.vilspa.esa.es/sas/8.0.0/doc/epicbscalgen.ps.gz
    ... Formally, the IBS is de ned as follows:  The +X axis points along the optical axis of the telescope of the respective instrument from the focal plane into the sky. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/epicbscalgen.ps.gz -- 79.0 Кб -- 02.07.2008
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    75. How to reduce RGS data and extract spectra of point-like sources
    ... The first part of the expression in the evselect task indicates that only events in CCD number 9 are selected (it is the one closest to the optical axis of the telescope, therefore the most affected by background flares). ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.0.0/documentation/threads/rgs_thread.html -- 17.5 Кб -- 01.06.2007
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    76. Description
    ... source count distribution are performed in all energy bands of each EPIC telescope ... Gaussian sigma), and source count rates in each energy band of each telescope ... Right ascension and declination of the optical axis positions used for the ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/5.4.1/doc/emldetect/node3.html -- 16.0 Кб -- 10.01.2003
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    77. SciSim MOS simulation and analyse
    ... Load the default configuration for the telescope you are going to use. ... SciSim has three different telescopes configurations: . ... Telescope 1 loads the default configuration for MOS1, RGS1 and OM. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/scisim/scisim_threads/mos/SciSimMOSThread.html -- 11.6 Кб -- 01.03.2006
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    78. SciSim RGS simulation and analyse
    ... Load the default configuration for the telescope you are going to use. ... SciSim has three different telescopes configurations: . ... Telescope 1 loads the default configuration for MOS1, RGS1 and OM. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/scisim/scisim_threads/rgs/SciSimRGSThread.html -- 12.8 Кб -- 20.01.2005
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    79. SciSim PN simulation and analyse
    ... Load the default configuration for the telescope you are going to use. ... SciSim has three different telescopes configurations: . ... Telescope 1 loads the default configuration for MOS1, RGS1 and OM. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/scisim/scisim_threads/pn/SciSimPNThread.html -- 11.8 Кб -- 20.01.2005
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    80. Description
    ... source count distribution are performed in all energy bands of each EPIC telescope ... model core radius), and source count rates in each energy band of each telescope ... Right ascension and declination of the optical axis positions used for the ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/6.0.0/doc/emldetect/node3.html -- 19.9 Кб -- 18.03.2004
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