1. XMM-Newton 1 Michael Smith, ESAC PN Monitoring MPE, May 2006

2. XMM-Newton 2 Michael Smith, ESAC Hot Pixels

3. XMM-Newton 3 Michael Smith, ESAC Noisy Pixels

4. XMM-Newton 4 Michael Smith, ESAC Noisy Pixels FF 50-Iteration Offset Introduction

5. XMM-Newton 5 Michael Smith, ESAC Noisy Pixels

6. XMM-Newton 6 Michael Smith, ESAC Offset Median

7. XMM-Newton 7 Michael Smith, ESAC Offset Variance

8. XMM-Newton 8 Michael Smith, ESAC Offset Variance First Observations per Revolution Eclipse Season Boundaries

9. XMM-Newton 9 Michael Smith, ESAC Offset Maps Normal Variance Excessive Variance

10. XMM-Newton 10 Michael Smith, ESAC Mean Row Offset vs RAWY Normal Variance

11. XMM-Newton 11 Michael Smith, ESAC Mean Row Offset vs RAWY Excessive Q0 & Q2 Variance

12. XMM-Newton 12 Michael Smith, ESAC Mean Row Offset vs RAWY Excessive Q1 & Q3 Variance

13. XMM-Newton 13 Michael Smith, ESAC CalClosed Line Widths vs Offset Map Variance Quadrant 0Quadrant 1

14. XMM-Newton 14 Michael Smith, ESAC Rev 1114 Temperature Excursions Rev 1114: 07/01/2006 22:48z SEU causes spurious switch-on of EPIC substitution heater during observation 0302160401 Resulted in PN CCD temperature excursions of +3.6 to –2.7 deg C with respect to nominal value of –89.8 deg C

15. XMM-Newton 15 Michael Smith, ESAC

16. XMM-Newton 16 Michael Smith, ESAC

17. XMM-Newton 17 Michael Smith, ESAC

18. XMM-Newton 18 Michael Smith, ESAC

19. XMM-Newton 19 Michael Smith, ESAC

20. XMM-Newton 20 Michael Smith, ESAC

21. XMM-Newton 21 Michael Smith, ESAC

22. XMM-Newton 22 Michael Smith, ESAC

23. XMM-Newton 23 Michael Smith, ESAC

24. XMM-Newton 24 Michael Smith, ESAC

25. XMM-Newton 25 Michael Smith, ESAC

26. XMM-Newton 26 Michael Smith, ESAC

27. XMM-Newton 27 Michael Smith, ESAC Individual noisy pixel spectrum at warm, cool and nominal T

28. XMM-Newton 28 Michael Smith, ESAC CCD 11 Column 63 segment spectrum at warm, cool and nominal T

29. XMM-Newton 29 Michael Smith, ESAC Overall spectrum: warm w.r.t. nominal T

30. XMM-Newton 30 Michael Smith, ESAC Overall spectrum: cool w.r.t. nominal T

31. XMM-Newton 31 Michael Smith, ESAC Energy Scale vs Time very good, esp. for FF mode. Still slight over-correction for EFF mode. SW mode under-correction, esp. at Mn (Result of SAS 6.1 Processing) M. Kirsch

32. XMM-Newton 32 Michael Smith, ESAC Line width trend is stable ~0.5 ADU/year increase at Mn (Result of SAS 6.1 Processing) M. Kirsch

33. XMM-Newton 33 Michael Smith, ESAC MOS Monitoring MPE, May 2006

34. XMM-Newton 34 Michael Smith, ESAC MOS1 Bad Pixels MOS2

35. XMM-Newton 35 Michael Smith, ESAC