XMM EPIC SAS EPIC Calibration meeting 2-4 April 2002 SAS v5.3 Detector Response Matrix Calculation Richard Saxton, Uwe Lammers.

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Presentation transcript:

XMM EPIC SAS EPIC Calibration meeting 2-4 April 2002 SAS v5.3 Detector Response Matrix Calculation Richard Saxton, Uwe Lammers

XMM EPIC SAS EPIC Calibration meeting 2-4 April 2002 Major Changes in SAS 5.3 •All event patterns supported •Observing mode dependencies for RMF/ARF •All box shapes handled by arfgen & backscale •Epic-pn ccd gaps handled correctly •Epic-pn out-of-time event exposure correction •Accurate encircled energy correction for annuli •Rmfgen makes variable format RMFs to save space •CAL changes produce faster processing

XMM EPIC SAS EPIC Calibration meeting 2-4 April 2002 PN RMF with pattern fractions

XMM EPIC SAS EPIC Calibration meeting 2-4 April 2002 Pattern fractions

XMM EPIC SAS EPIC Calibration meeting 2-4 April 2002 RMF pattern averaging

XMM EPIC SAS EPIC Calibration meeting 2-4 April 2002 How close is it to “canned” matrices ? MOS-1 m1_thin1v9q20t5r6_all_15.rsp

XMM EPIC SAS EPIC Calibration meeting 2-4 April 2002 MOS-2 m2_thin1v9q20t5r6_all_15.rsp

XMM EPIC SAS EPIC Calibration meeting 2-4 April 2002 PN epn_ff20_sY9_thin.rsp

XMM EPIC SAS EPIC Calibration meeting 2-4 April 2002 CCF elements REDISTRIBUTION: EMOS1_REDIST_ new low-energy shape EMOS2_REDIST_ new low-energy shape EPN_REDIST_ more energies (1319) QUANTUM EFFICIENCY: EMOS1_QUANTUMEF_ reworking above 1.5 keV EMOS2_QUANTUMEF_ reworking above 1.5 keV EPN_QUANTUMEF_ essentially no change

XMM EPIC SAS EPIC Calibration meeting 2-4 April 2002 MOS low-energy redistribution

XMM EPIC SAS EPIC Calibration meeting 2-4 April 2002 Relative MOS effective area

XMM EPIC SAS EPIC Calibration meeting 2-4 April 2002 TELESCOPE AREAS: XRT1_XAREAEF_ unchanged XRT2_XAREAEF_ unchanged XRT3_XAREAEF_ unchanged VIGNETTING: XMM_MISCDATA_ boresight reset to detx=0, dety=0 PSF: XRT1_XPSF_ King parameters from EPIC-MCT-TN-011 XRT2_XPSF_ King parameters from EPIC-MCT-TN-011 XRT3_XPSF_ King parameters from LUX (on-axis only) CCF elements (II)

XMM EPIC SAS EPIC Calibration meeting 2-4 April 2002 Coming soon…  Line broadening in the MOS RMF due to evolving CTI  Spatial averaging of RMFs  Full treatment of event selection flags  Better handling of offset columns  Enhanced support for extended sources