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Table 5

Parameters of the Gaussian (Models 1a, 1b, 1c, and 1d) and laor (Models 2a, 2b, 2c and 2d) components used to model the Fe emission at  ~ 6 keV.

Target Observation gau2 laor
E gau σ k gau EW E laor β r in i k laor EW
(keV) (keV) (eV) (keV) ° (eV)

4U 0614 + 09 0111040101 6.79  ±  0.16 0.94 8 185 6.50  ±  0.10 2.1  ±  0.3 4.0 70 7 160
4U 1543 − 62 0061140201 6.77 0.33  ±  0.13 0.97 23 6.56 3.6 64 63 1.21  ±  0.35 32  ±  9
4U 1636 − 536 0303250201 6.78  ±  0.01 1.15  ±  0.17 14.6  ±  9 210  ±  129 6.40 2.3  ±  0.2  < 6.25 70 9  ±  1 130  ±  14
0500350301 6.97 0.6  ±  0.3 3  ±  2 28  ±  19 6.97 (f) 2.2  < 64 50 3.5 36
0500350401 6.97 0.94 8.3 59 6.95 4.8 (f) 205.8 (f) 14 (f) 0.9  ±  0.5 6  ±  3
GX 340 + 0 0505950101 6.72  ±  0.06 0.17 22.0 17 6.82 2.56 (f)  >  16  < 34 19.7 15  ±  5
GX 349 + 2 0506110101 6.72  ±  0.06 0.32 96 82 6.94 3.1 11 17  ±  9 104 96
4U 1705 − 44 0402300201 6.53  ±  0.07 0.34 1.4  ±  0.4 57  ±  16 6.51  ±  0.08  < 3.1  < 110 45  ±  12 1.4  ±  0.4 58  ±  16
0551270201 6.56  ±  0.05 0.44  ±  0.06 61 92 6.45 1.8  < 9.1 65 83 135
Ser X − 1 0084020401 6.61  ±  0.05 0.22 22 52 6.79 2.84 13.3  < 33 25.2  ±  4.8 63  ±  12
0084020501 6.58  ±  0.07 0.25  ± 0.08 15.7 50 6.6  ±  0.1 2.03 (f) 11.15 (f) 28  ±  9 17.5  ±  4 59  ±  13.5
0084020601 6.59 0.27 18.7 51 6.73 2.6 11  < 25 19.4 57  ±  18
4U 1728 − 34 0149810101 6.72  ±  0.10 0.98 21 189 6.53 2.6  ±  0.4 20 70 7.7 80
4U 1735 − 44 0090340201 6.74  ±  0.10 0.38  ±  0.11 22  ±  7 46  ±  14 6.73  < 2.94 5.41 (f) 44 20  ±  6 43  ±  13
SAX J1808.4 − 3658 0560180601 6.94 0.26 1.5 23 6.50 3 6.3 46 3.1 51
0560180601** 6.77  ±  0.13 0.39 1.9  ±  0.7 30  ±  11 6.96 5.0 33 26 1.8  ±  0.6 31  ±  10

Notes. Egau and σ represent the energy and width of the Gaussian feature. The parameters of the laor component Elaor, β, rin, i and klaor account for energy, emissivity index, inner radius (in units of rg), inclination and normalisation. β is constrained to be  < 5. The inner radius is constrained to be  > 1.235 rg (GM / c2). The inclination is constrained to be  < 70°, since none of the sources is a known dipper or eclipsing system. The outer radius has been fixed to 400 rg for all sources, since it is not well constrained. The normalisation is in units of (10-4 ph cm-2 s-1) for both components. Parameters that are completely unconstrained when the errors are calculated have been fixed at their best value and are indicated in the table with “(f)”. A star (*) means that the error has reached the maximum or minimum allowed value of the parameter. For SAX J1808.4 − 3658 we show results for two spectra, which only differ in the pile-up treatment (see text).

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