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Table 7
2–10 keV luminosities in units of 1036 erg s-1 and corresponding Eddington ratios (L2 − 10 keV/LEddington) for all the observations in the sample.
Source | Observation | d | L 36 | R Edd |
ID | [kpc] | erg s-1 | ||
|
||||
4U 0614 + 09 | 0111040101 | 3.2 ± 0.5 (Kuulkers et al. 2009) | 0.73 | 0.004 |
4U 1543 − 62 | 0061140201 | 7 (Wang & Chakrabarty 2004) | 2.87 | 0.016 |
4U 1636 − 536 | 0303250201 | 6.0 ± 0.1 (Galloway et al. 2008) | 3.41 | 0.019 |
0500350301 | 6.01 | 0.033 | ||
0500350401 | 8.17 | 0.045 | ||
GX 340 + 0 | 0505950101 | 11 (Grimm et al. 2002) | 230.72 | 1.264 |
GX 349 + 2 | 0506110101 | 9.2 (Grimm et al. 2002) | 127.64 | 0.701 |
4U 1705 − 44 | 0402300201 | 5.8 ± 0.2 (Galloway et al. 2008) | 1.05 | 0.006 |
0551270201 | 27.25 | 0.150 | ||
GX 9 + 9 | 0090340101 | 4.4 (Grimm et al. 2002) | 10.98 | 0.060 |
0090340601 | 12.14 | 0.067 | ||
4U 1728 − 34 | 0149810101 | 4.0 ± 0.4 (Galloway et al. 2008) | 0.48 | 0.003 |
4U 1735 − 44 | 0090340201 | 6.6 ± 1.0 (Galloway et al. 2008) | 24.97 | 0.137 |
Ser X − 1 | 0084020401 | 7.7 ± 0.9 (Galloway et al. 2008) | 32.59 | 0.179 |
0084020501 | 26.45 | 0.145 | ||
0084020601 | 29.33 | 0.161 | ||
Aql X − 1 | 0303220201 | 3.9 ± 0.7 (Galloway et al. 2008) | 1.91 | 0.010 |
XTE J1807 − 294 | 0157960101 | 8 (assumed) | 1.36 | 0.007 |
SAX J1808.4 − 3658 | 0560180601 | 2.77 ± 0.11 (Galloway et al. 2008) | 0.79 | 0.004 |
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