Table A.5
Best fit parameters for GRS 1758-258, GX 17+2, and 4U 1705-44.
Source | GRS 1758-258 | GX 17+2 | 4U 1705-44 | ||||
---|---|---|---|---|---|---|---|
Obsid | 2429 | 2750 | 11088 | 5500 | 18086 | 19451 | 20082 |
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2.5 ± 0.1 | 2.0 ± 0.1 | 2.0 ± 0.1 | ||||
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kBThot (keV) | ![]() |
0.12 ± 0.02 | ![]() |
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kBTbb (keV) | 0.38 ± 0.01 | 0.42 ± 0.01 | – | – | – | – | – |
Γpow | ![]() |
2.7 ± 0.1 | – | – | – | – | – |
Tdbb (keV) | – | – | ![]() |
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kBT0 comt (keV) | – | – | 0.60 ± 0.01 | 0.41 ± 0.01 | ![]() |
0.54 ± 0.02 | 0.49 ± 0.01 |
kBT1 comt (keV) | – | – | ![]() |
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τcomt | – | – | ![]() |
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F0.5−2 keV (10−10 erg cm−2 s−1) | 0.8 ± 0.2 | 1.2 ± 0.2 | 4.3 ± 0.8 | 1.4 ± 0.1 | 3.6 ± 0.4 | 2.3 ± 0.2 | 2.3 ± 0.2 |
F2−10 keV (10−9 erg cm−2 s−1) | 0.12 ± 0.04 | 0.44 ± 0.08 | 13 ± 2 | 1.7 ± 0.2 | 7.1 ± 0.7 | 3.9 ± 0.4 | 3.0 ± 0.3 |
C2∕ν | 4182/3770 | 1393/1109 | 5838/4459 |
Notes. The fit of GRS 1758-258 was produced using the following SPEX model components: a blackbody, a power law, AMOL, the cold gas model (i.e., HOT with kBT = 5 × 10−4), and hot gas (HOT). The fit of GX 17+2 was produced using the following SPEX model components: a disk blackbody, a comptonization, AMOL, the cold gas model, and hot gas (HOT). The fit of 4U 1705-44 was produced using the following SPEX model components: a disk blackbody, a comptonization, AMOL, the cold gas model, and hot gas (HOT).
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