Table 5
Spectral fits of other bright X-ray sources.
| Name | XID | tbabs × apec | tbabs × pow | |||||||||
|
|
|
|||||||||||
| N H | kT (keV) | Norm | χ2(d.o.f.) | f X | N H | Γ | Norm | χ2 (d.o.f.) | f X | |||
| (1022 cm-2) | (keV) | (10-4 cm-5) | (10-13 erg cm-2 s-1) | (1022 cm-2) | (10-13 erg cm-2 s-1) | |||||||
|
|
||||||||||||
| XMMU J023200.4+612038 | 3 | 1.35 ± 0.16 | 12.3 ± 4.1 | 4.31 ± 0.20 | 1.09(211) | 5.84 ± 0.42 | 1.84 ± 0.23 | 1.86 ± 0.14 | 1.76 ± 0.38 | 0.95(211) | 5.51 ± 0.34 | |
| CXOU 023200.45+612039.0 | 1.19 ± 0.25 | >10.5 | 3.03 ± 0.54 | 1.18(118) | 4.19 ± 0.33 | 1.47 ± 0.28 | 1.59 ± 0.22 | 0.80 ± 0.27 | 1.13(118) | 3.98 ± 0.40 | ||
| XMMU J023230.2+611747 | 5 | 0.07 ± 0.02 | 0.64 ± 0.15 | 0.20 ± 0.03 | 1.20(80) | 0.92 ± 0.06 | ||||||
| +1.65 ± 0.26 | 0.48 ± 0.06 | |||||||||||
| CXOU 023230.26+611748.6 | 0.73 ± 0.18 | 0.33 ± 0.08 | 3.96 ± 3.15 | 1.20(72) | 1.26 ± 0.40 | 0.39 ± 0.12 | 3.81 ± 0.41 | 1.09 ± 0.31 | 1.26(74) | 1.24 ± 0.10 | ||
| +2.26 ± 1.08 | 0.70 ± 0.17 | |||||||||||
| XMMU J023407.5+612817 | 8 | 0.02 ± 0.02 | 0.26 ± 0.02 | 0.18 ± 0.04 | 1.31(54) | 0.39 ± 0.03 | ||||||
| +1.20 ± 0.17 | 0.13 ± 0.03 | |||||||||||
| XMMU J023300.0+612503 | 9 | 0.54 ± 0.22 | 3.34 ± 1.07 | 0.39 ± 0.78 | 0.91(37) | 0.40 ± 0.05 | 0.86 ± 0.27 | 2.48 ± 0.39 | 0.23 ± 0.11 | 0.86(37) | 0.39 ± 0.06 | |
| XMMU J023237.2+612810 | 10 | 0.29 ± 0.14 | 1.85 ± 0.27 | 0.22 ± 0.03 | 1.06(27) | 0.20 ± 0.06 | 0.82 ± 0.25 | 3.63 ± 0.76 | 0.27 ± 0.18 | 1.07(27) | 0.19 ± 0.03 | |
| CXOU 023237.01+612811.9 | 1.45 ± 0.33 | 0.81 ± 0.21 | 0.36 ± 0.23 | 0.77(9) | 0.10 ± 0.04 | 0.74 ± 0.49 | 3.35 ± 1.10 | 0.14 ± 0.17 | 1.15(9) | 0.12 ± 0.05 | ||
| XMMU J023208.0+612203 | 11 | 0.78 ± 0.28 | 5.44 ± 1.30 | 0.44 ± 0.34 | 1.17(32) | 0.19 ± 0.04 | ||||||
| CXOU 023208.03+612203.6 | 0.90 ± 0.17 | 0.75 ± 0.12 | 0.41 ± 0.16 | 1.13(23) | 0.19 ± 0.03 | 0.44 ± 0.28 | 3.63 ± 0.99 | 0.21 ± 0.17 | 1.05(23) | 0.23 ± 0.04 | ||
| XMMU J023245.8+612959 | 12 | 0.31 ± 0.19 | 3.69 ± 2.26 | 0.19 ± 0.04 | 0.57(20) | 0.22 ± 0.05 | 0.50 ± 0.29 | 2.19 ± 0.53 | 0.081 ± 0.052 | 0.66(20) | 0.23 ± 0.05 | |
| XMMU J023155.3+612249 | 13 | 2.39 ± 2.67 | > 3.75 | 0.61 ± 0.21 | 1.19(11) | 0.75 ± 0.65 | 2.35 ± 2.75 | 1.33 ± 0.86 | 0.11 ± 0.34 | 1.19(11) | 0.77 ± 0.10 | |
| XMMU J023300.9+613737 | 14 | 0.34 ± 0.12 | 5.07 ± 3.15 | 0.43 ± 0.06 | 1.06(33) | 0.58 ± 0.12 | 0.49 ± 0.19 | 1.97 ± 0.38 | 0.16 ± 0.07 | 1.07(33) | 0.59 ± 0.11 | |
| XMMU J023243.0+613059 | 15 | 0.33 ± 0.12 | 3.12 ± 0.87 | 0.28 ± 0.04 | 1.02(35) | 0.31 ± 0.05 | 0.59 ± 0.19 | 2.47 ± 0.36 | 0.15 ± 0.06 | 1.02(35) | 0.31 ± 0.04 | |
| XMMU J023240.7+612801 | 16 | 0.24 ± 0.14 | 2.50 ± 1.29 | 0.15 ± 0.03 | 1.13(15) | 0.16 ± 0.03 | 0.52 ± 0.25 | 2.73 ± 0.73 | 0.097 ± 0.069 | 1.05(15) | 0.16 ± 0.04 | |
| CXOU 023240.76+612800.2 | 1.58 ± 0.70 | 1.56 ± 0.83 | 1.21 ± 0.52 | 1.01(14) | 0.53 ± 0.13 | 1.05 ± 0.69 | 2.64 ± 0.64 | 0.44 ± 0.52 | 1.35(14) | 0.61 ± 0.17 | ||
| XMMU J023209.2+613039 | 17 | 0.76 ± 0.53 | 2.69 ± 1.31 | 0.46 ± 0.18 | 1.21(17) | 0.38 ± 0.09 | 1.02 ± 0.49 | 2.60 ± 0.59 | 0.27 ± 0.22 | 1.29(17) | 0.39 ± 0.11 | |
| XMMU J023243.3+612803 | 18 | 0.33 ± 0.13 | 2.58 ± 0.93 | 0.22 ± 0.03 | 0.69(24) | 0.22 ± 0.04 | 0.60 ± 0.22 | 2.59 ± 0.49 | 0.13 ± 0.07 | 0.79(24) | 0.23 ± 0.04 | |
| XMMU J023243.7+612631 | 19 | 0.44 ± 0.44 | 2.78 ± 1.86 | 0.31 ± 0.12 | 0.36(10) | 0.30 ± 0.07 | 0.70 ± 0.43 | 2.55 ± 0.67 | 0.18 ± 0.16 | 0.39(10) | 0.31 ± 0.09 | |
| CXOU 023243.54+612632.0 | 1.34 ± 0.85 | 1.48 ± 1.35 | 0.69 ± 0.47 | 1.07(11) | 0.32 ± 0.12 | 0.95 ± 0.59 | 2.72 ± 0.77 | 0.29 ± 0.33 | 1.63(11) | 0.38 ± 0.14 | ||
| XMMU J023317.6+612808 | 20 | 0.29 ± 0.17 | 2.91 ± 1.19 | 0.18 ± 0.04 | 1.27(18) | 0.20 ± 0.04 | 0.67 ± 0.30 | 2.79 ± 0.63 | 0.13 ± 0.09 | 1.08(18) | 0.19 ± 0.04 | |
| XMMU J023254.0+612803 | 21 | 0.35 ± 0.56 | 3.93 ± 4.40 | 0.15 ± 0.08 | 0.98(11) | 0.18 ± 0.05 | 0.56 ± 0.58 | 2.20 ± 0.72 | 0.066 ± 0.082 | 0.98(11) | 0.18 ± 0.06 | |
| XMMU J023300.9+612608 | 22 | 0.38 ± 0.21 | 3.21 ± 1.82 | 0.18 ± 0.04 | 1.16(15) | 0.20 ± 0.04 | 0.63 ± 0.17 | 2.43 ± 0.60 | 0.097 ± 0.068 | 1.19(15) | 0.20 ± 0.05 | |
Notes.For each source, all existing EPIC spectra were fitted simultaneously. When available, the results of the associated Chandra source are presented immediately below the best-fit to the XMM-Newton data. Errors correspond to 90% confidence intervals (derived from the error command for parameters and flux err for fluxes) − when asymmetric, the larger error is indicated. The quoted fluxes are the observed values in the 0.5–10. keV energy band. The normalization of the power-law models is expressed as the number of photons keV-1 cm-2 s-1 at an energy of 1 keV, whilst the normalization of the apec models is presented in Table 4.
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