... 1.6 Ms: z=0.4 blazar for WHIM 1.4Ms: Draco dwarf galaxy: dark matter line ... area calibration b) The Timing Mode energy scale calibration which is now accurate ... and correct for the timeevolution of energy resolution. c. Continue the Burst Mode ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201504/Santos_Cal_2015.pdf -- 299.1 Кб -- 10.04.2015 Похожие документы
... dark_current 2.2e-2 # e/s (1x1 pixel) doping default subtract_level 0 pixelSurface PixelBackSurfaceCcd1 end end # CCD id 1 begin ## ------------------------------------------------ ## CCD 2 ## gain, noise and CTE set from SRON CCD 6111-13-02 ...
... dark_current 2.2e-2 # e/s (1x1 pixel) doping default subtract_level 0 pixelSurface PixelBackSurfaceCcd1 end end # CCD id 1 begin ## ------------------------------------------------ ## CCD 2 ## gain, noise and CTE set from SRON CCD 6111-13-02 ...
... X . XMM-CCF-REL-323 . EPIC-pn Long-Term CTI and Energy Scale . 09-Dec-2014 . X . ... X . XMM-CCF-REL-313 . Refinement of the high-energy XRT3 PSF . 18-Mar-2014 . X . ... PN telescope effective area modification at high energies . 07-Apr-2007 . X . ...
... X . XMM-CCF-REL-323 . EPIC-pn Long-Term CTI and Energy Scale . 09-Dec-2014 . X . ... X . XMM-CCF-REL-313 . Refinement of the high-energy XRT3 PSF . 18-Mar-2014 . X . ... PN telescope effective area modification at high energies . 07-Apr-2007 . X . ...
... dark_current 2.2e-2 # e/s (1x1 pixel) doping default subtract_level 0 pixelSurface ... Elow 10 # lowest energy to produce (eV) Ehigh 30e3 # highest energy to produce (eV ...
... Detector Energy Resp onse and Redistribution Monitoring To monitor the EPIC energy ... 8908 E6, Flat low, Dark low 13736 E6, Flat high 17411 E6, Dark low, Flat high 24360 ...
... energy of the OVII line during the CAL-Thin exposure is statistically ... energy scale" A spatially dependent comparison between the measured and the nominal ... for higher energies (0.85 keV), some evolution is seen at lower energies (<0.85 keV ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201003/minutes-cal-2010.pdf -- 66.3 Кб -- 13.05.2014 Похожие документы
... consists of low energy protons ("soft" protons), with energies ranging up to 300 keV ... energy-independent impacts on the effective area, and molecular contamination, the ... energy resolution was improved by 13% and 17% for EPIC-MOS1 and EPIC-MOS2 ...
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Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0062-1-0.pdf -- 673.9 Кб -- 10.11.2005 Похожие документы