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    91. http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/RXTE_PCA_JAHoda.pdf
    ... of the Rossi X-ray Timing Explorer Proportional Counter Array" Jahoda, Markwardt, Radeva, Rots, Stark, Strohmayer, Swank, and Zhang, 2006, ApJS, 163, 401 ­ Energy: residuals < 1% (E< 10 keV); < 2% (below 20 keV) ­ Background: (excess variance)1/2 < 2 ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/RXTE_PCA_JAHoda.pdf -- 1349.8 Кб -- 19.06.2006
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    92. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201504/Santos_Cal_2015.pdf
    ... him to continue with the on-going progress on stray-light in-orbit calibration activities b. Make progress on the characterisation of the particle-generated background (either through protons or reflected X-rays) in the EPIC cameras Science Operations ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201504/Santos_Cal_2015.pdf -- 299.1 Кб -- 10.04.2015
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    93. Field of View
    ... Next: Dark current and cooling Up: CCD Scientific Performance Previous: Particle Background Rejection . ... particularly at the highest energies, designs of the X-ray optics for the major observatories mentioned in section 1 require ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/user/socpub/ccd_review/node11.html -- 5.7 Кб -- 30.08.1996
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    94. XMM-Newton Trainee Project 2004
    ... Initially, I did some background reading about the XMM-Newton spacecraft, its X-ray cameras and relevant astronomy topics. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_links/trainee/2005/student_summaries.shtml -- 18.5 Кб -- 13.04.2016
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    95. http://xmm.vilspa.esa.es/sas/5.4.1/doc/evigweight.ps.gz
    ... is approximately the same for all CCDs. xmmsas 20030110 1802-5.4.1 XMM-Newton Science Analysis System Page: 4 3.8 Background correction One important issue for the spectral analysis with X-ray detectors is the treatment of background for extended sources ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/5.4.1/doc/evigweight.ps.gz -- 62.9 Кб -- 10.01.2003
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    96. http://xmm.vilspa.esa.es/scisim/release/latest/help/postscript/scisim.ps
    ... 7.7 Background In addition to discrete sources, the background level (in the x-ray and optical) and the column density across the whole eld of view need to be de ned. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/scisim/release/latest/help/postscript/scisim.ps -- 1408.7 Кб -- 12.01.2005
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    97. http://xmm.vilspa.esa.es/sas/7.0.0/doc/evigweight.ps.gz
    ... 3.8 Background correction One important issue for the spectral analysis with X-ray detectors is the treatment of background for extended sources. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/7.0.0/doc/evigweight.ps.gz -- 63.2 Кб -- 28.06.2006
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    98. http://xmm.vilspa.esa.es/sas/6.0.0/doc/evigweight.ps.gz
    ... 3.8 Background correction One important issue for the spectral analysis with X-ray detectors is the treatment of background for extended sources. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/6.0.0/doc/evigweight.ps.gz -- 63.3 Кб -- 18.03.2004
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    99. http://xmm.vilspa.esa.es/sas/6.5.0/doc/evigweight.ps.gz
    ... 3.8 Background correction One important issue for the spectral analysis with X-ray detectors is the treatment of background for extended sources. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/6.5.0/doc/evigweight.ps.gz -- 63.4 Кб -- 16.08.2005
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    100. http://xmm.vilspa.esa.es/sas/6.1.0/doc/evigweight.ps.gz
    ... 3.8 Background correction One important issue for the spectral analysis with X-ray detectors is the treatment of background for extended sources. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/6.1.0/doc/evigweight.ps.gz -- 63.3 Кб -- 22.11.2004
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