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Table A.1

Fit results and systematics for the central observation.

Annulus Nominal CXB CXB NXB NXB Abundance table
Anders & Grevesse (1989)

T (keV)

1
2
3
4

Mg

1
2 < 0.80 < 0.82 < 0.73 < 0.80 < 0.80 < 0.76

Si

1
2
3 <0.44 <0.46 <0.38 <0.44 <0.44 <0.36

S

1
2
3

Ar

1

Ca

1

Fe

1
2
3
4

Norma

1
2
3
4

XRBG

NormCXBc fix fix
NormMWHb
TLHB (10-2 keV)
NormLHBb

Notes. The CXB in Cols. 3 and 4 was scaled according to Table 3. The NXB was scaled by ± 3%. Upper limits are given at 90% confidence level.

(a)

with DA being the angular diameter distance to the source.

(b)

Normalization of the apec component scaled to area 400π assumed in the uniform-sky ARF calculation. Norm =  cm-5.

(c)

In units of 10-3 photons/s/cm2 at 1 keV scaled to the area 400π.

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