Cross-calibrating X-ray detectors with clusters of galaxies: an IACHEC study

J. Nevalainen; L. David; M. Guainazzi

doi:10.1051/0004-6361/201015176

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Volume 523 (November-December 2010)

A&A, 523 (2010) A22

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Table 11

The relative difference and its significance of temperatures and fluxes for different combinations of instruments and methods.

Instruments

T _hard^a

flux_hard^a

T _soft^b

flux_soft^b

T_soft/T_hard

T _wide^c

T _Fe^d

T_cont^e/T_Fe

μ^e

sig.^f

μ ^e

sig.^f

μ ^e

sig.^f

μ ^e

sig.^f

μ ^e

sig.^f

μ ^e

sig.^f

μ ^e

sig.^f

μ ^e

sig.^f

MOS2/MOS1

−5

3.4

−3

6.2

−6

3.6

2

5.2

...

−5

9.9

...

MOS1/pn

1

0.7

7

15.4

5

3.7

6

11.8

...

5

10.3

...

MOS2/pn

−4

2.6

5

10.0

−1

0.5

6

24.3

...

0

0.2

...

MECS/pn

−1

0.9

...

ACIS/pn

−1

0.6

11

24.7

18

8.6

2

10.6

...

14

18.0

...

ACIS/MOS1

...

3

6.1

...

−3

9.8

...

8

10.0

...

ACIS/MOS2

...

6

12.8

...

−5

16.7

...

15

18.9

...

MOS/pn

...

−6

2.2

...

pn

...

−36

29.9

...

1

0.2

MOS

...

7

1.6

MOS1

...

−32

21.8

...

MOS2

...

−32

23.1

...

ACIS

...

−12

1.6

...

Notes. The values correspond to the best-fit single temperature models in the

^(a)

2−7 keV band;

^(b)

0.5−2 keV band;

^(c)

0.5−7 keV band;

^(d)

~6.0−7.0 keV band; and

^(e)

2−6 keV band. The ACIS values are obtained using CALDB 4.2.0. (e) μ gives the weighted mean of the relative difference between the two measurements in percentages;

^(f)

sig. gives the significance of the relative difference in terms of σ.

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