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This meeting in Mallorca, Spain, in March 31 - April 1, 2009, focused on EPIC CCD monitoring and calibration, including discussions on energy resolution before and after satellite contact losses for Al-K and Mn-K, charge transfer inefficiency, and FWHM for different CCDs and energy levels. Trends in CTI and FF for EPIC CCDs were analyzed from 2000 to 2009, showing improvements in performance over the years with specific attention to energy resolution and quadrant FWHM measurements for Mn-K and Al-K. The meeting emphasized the importance of long-term monitoring and calibration practices for maintaining data quality in astronomical observations.
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Update of EPIC pn long-term monitoring EPIC Calibration & Operations Meeting Mallorca, Spain, 2009 March 31 – April 1
Energy resolution @ Al-K before/after satellite contact loss
Energy resolution @ Mn-K before/after satellite contact loss
Al-K FF Mn-K FF Al-K eFF Mn-K eFF
Mn-K FF CTI(t) 2002
Mn-K FF CTI(t) 2003
Mn-K FF CTI(t) 2004
Mn-K FF CTI(t) 2005
Mn-K FF CTI(t) 2006
Mn-K FF CTI(t) 2007
Mn-K FF CTI(t) 2008
Mn-K FF CTI(t) 2009
30 ks in 2000 300 ks in 2009 30 ks 10 ks
Update of EPIC pn long-term monitoring EPIC Calibration & Operations Meeting Mallorca, Spain, 2009 March 31 – April 1