INTEGRAL hard X-ray spectra of the cosmic X-ray background and Galactic ridge emission

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Table 2:

Numerical values of the obtained spectra shown in Fig. 6.
E	$\Delta E$	$F_{{\rm sky}}$	$\Delta F_{{\rm sky}}$	$F_{{\rm ear}}$	$\Delta F_{{\rm ear}}$	$F_{{\rm gal}}$ ^c	$\Delta F_{{\rm gal}}$ ^c
(keV)^a		(keV cm^-2 s^-1 sr^-1)^b
21.14	1.44	39.57	2.53	7.05	1.58	18.09	2.07
24.01	1.44	42.79	1.92	8.63	1.47	19.94	0.55
27.36	1.91	43.84	1.81	11.23	1.31	19.26	4.88
31.19	1.91	42.90	1.44	13.79	1.21	16.62	2.75
35.02	1.91	41.08	2.45	17.02	1.60	14.35	4.26
38.85	1.91	39.08	2.55	20.31	1.88	12.12	2.63
43.16	2.39	35.42	2.42	23.87	2.46	9.80	0.84
47.95	2.39	38.67	1.95	26.82	2.16	9.70	1.35
52.73	2.39	36.24	2.42	29.30	2.00	8.33	1.40
58.00	2.87	30.88	3.41	30.85	2.14	7.72	1.37
63.74	2.87	28.86	2.81	31.18	2.48	7.17	1.78
71.88	5.27	28.92	3.34	32.47	3.11	6.46	1.31
83.37	6.22	30.01	6.35	33.37	3.23	6.17	0.80
94.86	5.27	27.12	4.89	34.01	2.71	6.64	0.84
112.57	12.45	24.82	5.94	35.04	3.90	6.68	0.99
162.35	37.34	30.65	9.55	37.85	7.46	7.93	2.86

Notes. ^(a) Central energy, E, and half-width, $\Delta E$ , of the bins. ^(b) Fluxes, F, and statistical uncertainties, $\Delta F$ , for the sky background (sky), the Earth (ear) and the Galaxy (gal). ^(c) On average over the region $320^\circ < l < 340 ^\circ$ and $\vert b\vert < 5^\circ$ .

Source LaTeX | All tables | In the text

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