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    • 1. http://xmm.vilspa.esa.es/external/xmm_links/trainee/alumni/n_fonseca.pdf
    ... objects in the Palomar Br ight Quasar Survey ABS (reference in Veron for data, some with upper limit (#) <0.25mJy) (3) Gregory ...
    [ 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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    2. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200610/Sembay.pdf
    ... Test #1: Resolution at Al K "Red" wing is due to incomplete charge collection rather than intrinsic broadening Al K = K 1(1.4867) + 0.5 x K 2(1.4863) In our analytic rmf model we model this by splitting the profile "Red" side = Gaussian( ) + Gaussian(R x ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200610/Sembay.pdf -- 2605.5 Кб -- 14.05.2014
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    3. http://xmm.vilspa.esa.es/sched_tour/too_paper.pdf
    ... In this paper , we present what kind of objects are suitable to be observed as ToO ... in astrophysics, e.g. newly detected objects that are of high scientific interest ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sched_tour/too_paper.pdf -- 30.7 Кб -- 07.11.2001
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    4. http://xmm.vilspa.esa.es/external/xmm_sched/sched_tour/ESA_bulletin_107.pdf
    ... Here we discuss the kinds of objects that are suitable for observation as ToOs with ... in astrophysics, for example newly detected objects that are of high scientific ...
    [ 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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    5. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200904/Minutes-cal-000409.pdf
    ... Objective 2: OFF axis calibration a) 2-D parametrization of the PSF (AR): the new CCF shall be released to the public after successful completion of the test on the elliptical envelope (SOC) and the source detection efficiency SSC by the next BOC b) a ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200904/Minutes-cal-000409.pdf -- 92.0 Кб -- 13.05.2014
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    6. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0062-1-0.pdf
    ... atmosphere of the Earth suffer from extreme conditions due to radiation, temperature ... 2-0.3 m. These particles are either (red), patch location rev. 636 (dark blue), off ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0062-1-0.pdf -- 673.9 Кб -- 10.11.2005
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    7. http://xmm.vilspa.esa.es/sas/8.0.0/doc/omdetect.ps.gz
    ... red 1 READ-OUT STREAK 2 magenta 2 SMOKE-RING 4 yellow 3 SOURCE ON STAR-SPIKE 8 white 4 Mod-8 pattern 16 black 5 Source within ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/omdetect.ps.gz -- 122.7 Кб -- 29.01.2009
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    8. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0073-1-0.pdf
    ... in these systems, as well as of the physical processes close to the compact object ... Burst mode is not appropriate for PSD studies, due to its extreme window function14 ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0073-1-0.pdf -- 407.1 Кб -- 10.07.2007
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    9. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0012-1-0.ps.gz
    ... Its primary objective is to perform high throughput spectroscopy of cosmic x­ray ... matches exactly that which would be predicted for the known red­shift of the cluster ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0012-1-0.ps.gz -- 336.8 Кб -- 11.01.2001
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