Observation |
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c1 | 2.1(2) | 3.3 | 11/18 | 1.7(2) | 2.4 | 13/14 |
c3 | ![]() |
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1.4(3) | 3.9 | 16/10 |
c5 | 1.9(3) | 2.5 | 16/12 | 1.5(3) | 4.1 | 20/12 |
c7 | 2.1(4) | 2.2 | 6/9 | 1.8(3) | 2.5 | 6/11 |
c9 | 1.7(3) | 3.4 | 15/15 | 1.5(4) | 3.4 | 12/6 |
c12 | 1.7(2) | 3.0 | 20/11 | 2.3(4) | 0.9 | 6/7 |
c14 | 1.7(2) | 4.0 | 11/11 | 1.5(2) | 3.0 | 10/12 |
c15 | 1.6(2) | 4.5 | 11/16 | 1.8(2) | 3.0 | 12/11 |
c17 | ![]() |
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1.6(2) | 2.0 | 11/10 |
c22 | 2.2(9) | 2.0 | 4/3 | 1.9(5) | 1.8 | 3/6 |
c23 | 2.6(7) | 0.7 | 1/3 | 1.6(2) | 4.0 | 4/11 |
c28 | 1.8(3) | 3.8 | 8/10 | 2.2(6) | 1.9 | 10/6 |
c29 | 1.5(3) | 4.4 | 6/9 | 1.4(2) | 3.5 | 11/11 |
c31 | 2.1(3) | 3.0 | 11/9 | 1.3(2) | 3.7 | 13/9 |
c34 | 1.9(3) | 2.3 | 6/7 | 2.3(4) | 2.0 | 8.5/10 |
c35 | 2.0(4) | 2.7 | 3/7 | 1.7(3) | 3.5 | 5/7 |
a An absorbed power law model was used, with line-of-sight absorption![]() ![]() b 0.3-10 keV luminosity/1037 erg s-1. |