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XMM-Newton CCF Release Note XMM-CCF-REL-174 pn telescope e ective area modi cation M. Kirsch June 9, 2004 1 CCF components Name of CCF VALDATE List of Blocks changed CAL VERSION XSCS ag XRT3 XAREAEF 0009 2000-01-13T00:00:00 ONAXISXAREAEF 3.169 NO 2 Changes XMM EPIC-pn observations with very high statistic show residuals at the Silicon edge around 1.8 keV and gold edge around 2.2 keV (see Figure 1). The gold edge feature can be explained by not perfect calibration of the telescope e ective area. ...
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Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0174-1-0.ps.gz -- 154.5 Кб -- 09.06.2004 Похожие документы
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... Institute of Astronomy of Russian Academy of Sciences . 119017, Pyatnitskaya str., 48, Moscow, Russia . ... About me: . ... I observed different objects (minor planets, satellites, variable stars, gamma bursts, etc.) by myself at Zeiss-600 and 2-m telescope. Also I had some experience with observational data from the 6-m telescope BTA (SAO, Russia), VLT (ESO, Chile), 1.5-m telescope in Maidanak (Uzbekistan) and infrared space telescopes Spitzer and Herschel. ...