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    1. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200610/Abbey_testing.pdf
    ... This damage causes low energy redistribution changes Enhanced dark current at raised temperatures has been seen in CCDs illuminated with a focussed beam at the Panter facility (EPIC EOBB and Swift XRT) Have so far not been able to detect the low energy ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200610/Abbey_testing.pdf -- 1549.2 Кб -- 14.05.2014
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    2. Radiation Hardness
    ... For example, after krads of low energy protons, around 60 dark spike pixels were found in an EEV TV format CCD, with -70 C dark current generation rates of ~5-10 electrons per second [Holland et al]. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/user/socpub/ccd_review/node14.html -- 7.2 Кб -- 30.08.1996
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    3. Dark current and cooling
    ... The temperature dependence of dark current is of the form . ... bandgap energy, but for individual generation sites E may be a trapping state energy ... defects which give rise to individual dark current spikes , most dark current arises ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/user/socpub/ccd_review/node12.html -- 8.6 Кб -- 30.08.1996
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    4. http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0074-1-0.ps.gz
    ... Dark Frames D Lumb April 27, 2001 1 CCF components Name of CCF VALDATE List of Blocks changed CAL VERSION XSCS flag EMOS1 DARKFRAME 0007.CCF 2000­01­01 DARKFRAME CCDn NO OFFSET CCD1 EMOS1 DARKFRAME 0007.CCF 2000­01­01 DARKFRAME CCDn NO OFFSET CCD1 2 ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0074-1-0.ps.gz -- 43.6 Кб -- 04.05.2001
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    5. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200904/chen-anomalous-states.pdf
    ... Low energy noise on the MOS CCDs ­ p. 9/1 No correlation w/ RAWY periodicity Noise appears as dark/bright rows (same RAWY), but all noise tracks brighten/darken together. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200904/chen-anomalous-states.pdf -- 2304.0 Кб -- 14.05.2014
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    6. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201203/pagani-cal-2012.pdf
    ... energy resolution Trap depths = f(T) Temperature XRT CCD relies on passive cooling after TEC failure, operating between -75 and ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201203/pagani-cal-2012.pdf -- 1262.1 Кб -- 13.05.2014
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    7. CCD Scientific Performance
    ... Next: Energy resolution Up: Charge Coupled Devices (CCDs) Previous: Contrasting ... Energy resolution . Detection Efficiency . Deep Depletion . Front Illumination . ... Field of View . Dark current and cooling . Modes of Operation . ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/user/socpub/ccd_review/node4.html -- 3.4 Кб -- 30.08.1996
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    8. Field of View
    ... Next: Dark current and cooling Up: CCD Scientific Performance Previous: Particle Background Rejection . ... To attain high sensitivity, particularly at the highest energies, designs of the X-ray optics for the major observatories ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/user/socpub/ccd_review/node11.html -- 5.7 Кб -- 30.08.1996
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    9. Energy resolution
    ... where E is the photon energy, =3.68eVper electron is the charge conversion factor, r the system noise in electrons (which may include readout and dark current noise), and F the Fano factor for silicon (0.115 [Alig et al]). ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/user/socpub/ccd_review/node5.html -- 12.5 Кб -- 30.08.1996
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    10. Description
    ... All the E are then corrected for the difference between the dark map and the local offset, before building the internal background map (as described above) and building the PHA energy (in MAKE_E). ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/5.4.1/doc/emenergy/node3.html -- 13.9 Кб -- 10.01.2003
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