X-raying the AU Microscopii debris disk | Astronomy & Astrophysics (A&A)

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Table C.1:

Strong lines and measured fluxes.
Ions	Wavelength	Flux (10^-5ph/cm²/s)
Si XIII	6.65	4.5 $\pm$ 0.7
Ne X	10.24	6.3 $\pm$ 1.0
Ne IX	11.54	6.3 $\pm$ 1.0
Ne X	12.13	44.1 $\pm$ 2.1
Ne IX	13.45	32.8 $\pm$ 1.9
Ne IX	13.54	11.2 $\pm$ 1.3
Ne IX	13.70	22.9 $\pm$ 1.6
Fe XVIII	14.21	6.3 $\pm$ 1.4
Fe XVII	15.01	18.0 $\pm$ 1.4
Fe XIX/O VIII	15.18	6.4 $\pm$ 1.1
Fe XVII/Fe XX	15.26	8.4 $\pm$ 1.1
O VIII	16.01	17.6 $\pm$ 1.5
Fe XVIII	16.08	5.7 $\pm$ 1.3
Fe XVII	16.78	12.1 $\pm$ 1.2
Fe XVII	17.10	30.2 $\pm$ 1.9
O VIII	18.97	110.3 $\pm$ 3.3
O VII	21.61	29.2 $\pm$ 2.3
O VII	21.79	10.0 $\pm$ 1.6
O VII	22.10	19.4 $\pm$ 2.0
N VII	24.79	16.6 $\pm$ 2.0
C VI	33.73	33.9 $\pm$ 2.9
Fe XVIII	93.89	28.9 $\pm$ 3.7
Fe XVIII	103.92	11.1 $\pm$ 3.4
Fe XIX	108.33	26.2 $\pm$ 4.3
Fe XX	118.66	14.1 $\pm$ 4.2
Fe XX	121.85	17.0 $\pm$ 5.0
Fe XXI	128.75	<16.2
Fe XX	132.85	37.7 $\pm$ 8.6
Fe XXII	135.78	27.6 $\pm$ 7.9

Source LaTeX | All tables | In the text

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