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Table 3

Fluxes of the Fe-Kα line in units of 10-5 photons cm-2 s-1.

Region Feb. 02 Mar. 04 Sep. 04 Apr. 07 Mar. 08 Apr. 09

A 2.5  ±  0.3 2.2  ±  0.2 2.1  ±  0.1 2.2  ±  0.2 2.2  ±  0.2 2.2  ±  0.2
B1 2.3  ±  0.3 1.7  ±  0.2 1.5  ±  0.1 1.6  ±  0.1 1.3  ±  0.2 1.2  ±  0.1
B2 0.9  ±  0.2 0.7  ±  0.2 1.1  ±  0.1 2.1  ±  0.2 2.1  ±  0.2 2.1  ±  0.2
C 0.8  ±  0.3 0.7  ±  0.2 0.9  ±  0.2 1.2  ±  0.2 1.1  ±  0.3 1.2  ±  0.2
D 0.5  ±  0.2 0.7  ±  0.2 0.8  ±  0.1 1.0  ±  0.1 1.1  ±  0.2 2.1  ±  0.2
E 2.4  ±  0.4 2.2  ±  0.3 1.8  ±  0.2 2.1  ±  0.2 2.2  ±  0.3 2.1  ±  0.2
F 13.1  ±  1.0 11.2  ±  0.8 11.4  ±  0.5 10.0  ±  0.5 9.4  ±  0.7 9.1  ±  0.5
F1 4.4  ±  0.6 4.0  ±  0.5 4.4  ±  0.3 3.4  ±  0.3 3.0  ±  0.4 3.4  ±  0.3
F2 4.1  ±  0.6 3.1  ±  0.4 3.6  ±  0.3 3.7  ±  0.3 3.3  ±  0.4 2.6  ±  0.3
F3 5.2  ±  0.6 4.2  ±  0.5 3.8  ±  0.3 3.5  ±  0.3 3.4  ±  0.4 3.4  ±  0.3
DS1 1.5  ±  0.3 1.5  ±  0.3 1.4  ±  0.1 1.4  ±  0.1 1.4  ±  0.2 1.4  ±  0.2
DS2 2.8  ±  0.4 2.3  ±  0.3 2.4  ±  0.2 2.1  ±  0.2 2.4  ±  0.2 2.5  ±  0.2

Notes. The values are the weighted mean of the MOS1&2 measured fluxes. The different columns refer to different datasets (see text). The Apr07, Mar08 and Apr 09 fluxes for the regions D, DS1 and DS2 are based on MOS 2 data only, as a consequence of the damaged sustained by CCD6 in MOS 1 on 9 March 2005 (Abbey et al. 2006).

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