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Modifications to MOS Response File:

Modifications to MOS Response File:. Current Fixed Response Matrix is: m<1/2>_<thin1/med/thick>v9q19t5r5_<p0/all>_15.rsp Modifications to rmf below 0.7 keV………………….…...r6 Modifications to QE around O edge……………………..q20 Modifications to High Energy QE to force MOS-PN

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Modifications to MOS Response File:

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  1. Modifications to MOS Response File: Current Fixed Response Matrix is: m<1/2>_<thin1/med/thick>v9q19t5r5_<p0/all>_15.rsp Modifications to rmf below 0.7 keV………………….…...r6 Modifications to QE around O edge……………………..q20 Modifications to High Energy QE to force MOS-PN agreement………………………………………………….q21 ftp files from ftp.star.le.ac.uk in /pub/sse/<q19/q20/q21>

  2. q19r5: Multiple Gaussian model fit to MOS1 mono-pixel and bi-pixel spectra of 1E 0102.2-7219 (spectra supplied by Paul Bennie (LUX))

  3. q19r6: Multiple Gaussian model fit to mono-pixel and bi-pixel spectra

  4. q19r6: Multiple Gaussian model fit to MOS2 mono-pixel and bi-pixel spectra

  5. Comparison of rmf for q19r5, q19r6 and Ground

  6. q19r5 versus q19r6 in Mrk 421 Single Power Law, NH = Ngal (1.6x1020 cm-2)

  7. q20r6 versus q19r6 in Mrk 421 Single Power Law, NH = Ngal (1.6x1020 cm-2)

  8. Broken Power Law Fit (0.2-8 keV) q19r5 χ2 = 861.1/447 dof (1.93) NH=Ngal χ2 = 779.2/446 dof (1.75) NH=Free Req. Systematic = 1-6-1.7% q21r6 χ2 = 695.3/447 dof (1.56) NH=Ngal χ2 = 689.5/446 dof (1.55) NH=Free Req. Systematic = 1.4 %

  9. Comparison of MOS v PN spectrum of NGC 5548 Spectral Data supplied by James Reeves (LUX) q21: high energy QE modification derived (independently of this source) by Richard Saxton (LUX/SOC) q19r5 q21r6

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