Effective area calibration of the reflection grating spectrometers of XMM-Newton - II. X-ray spectroscopy of DA white dwarfs

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Table 7:

Comparison of model spectra for the same set of parameters (those of Beuermann et al. 2006). Fluxes are in photons m^-2 s^-1 Å^-1and include interstellar absorption.
	HZ 43A			Sirius B
$\lambda$ (Å)	TMAP	Tlusty	ratio	TMAP	Tlusty	ratio
48	3.00	2.89	0.963	-	0.20	-
60	21.3	20.95	0.984	2.45	2.23	0.910
70	63.2	62.58	0.990	9.38	8.75	0.933
80	139.	137.4	0.988	25.2	23.7	0.940
90	249.	246.7	0.991	53.0	49.8	0.940
100	388.	384.5	0.991	92.0	86.3	0.938
125	795.	792.5	0.997	201.	189.8	0.944
160	1310.	1306.	0.997	237.	220.6	0.931
1300	2652.	2630.	0.992	82000	78660	0.959
4600	-	111.4	-	6611	6450	0.976
5450	70.18	69.11	0.985	-	4192	-

Source LaTeX | All tables | In the text

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