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 (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 = %
q21r6
χ2 = 695.3/447 dof (1.56) NH=Ngal
χ2 = 689.5/446 dof (1.55) NH=Free
Req. Systematic = 1.4 %

10. 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