Table 7
X-ray sources detected with the Swift-XRT.
| ID | Name | σ90 | S/N | fabs(0.2–2 keV) | NH | φ0 | Γ | funabs(0.2–2 keV) |
| SWIFT J | [arcsec] | [10-14 erg cm-2 s-1] | [1020 cm-2] | [10-5 keV-1 cm-2 s-1] | [10-14 erg cm-2 s-1] | |||
|
|
||||||||
| A | 003000.3+072301a | 6 | 3.5 |
|
3.98 | 1.4 ± 0.4 | 2.0 | 5.2 ± 1.5 |
| B | 003017.8+072142 | 5 | 5.4 |
|
3.71 |
|
1.4 ± 0.3 |
|
| C | 003022.1+072623a | 6 | 3.1 |
|
3.10 |
|
2.0 |
|
| D | 003030.0+072013a | 5 | 5.1 |
|
3.71 |
|
2.0 |
|
| E | 003049.8+072316a | 6 | 3.0 |
|
3.10 |
|
2.0 |
|
| F | 003054.9+072328a | 6 | 2.8 |
|
3.10 |
|
2.0 |
|
| G | 003119.8+072454 | 5 | 6.5 |
|
3.10 |
|
1.6 ± 0.3 |
|
Notes. The FoV is centred on (RA,Dec) = (7.6315,7.4211) deg with a radius of 13′. We give an internal ID, the position (SWIFT JHHMMSS.s ± DDMMSS) and its corresponding error at 90% confidence level σ90 (determined with xrtcentroid), and the signal-to-noise ratio S/N (Ximage) of the observed flux fabs. If constraining, a power-law model corrected for photoelectric absorption was fitted to the spectrum, dφ/dE = φ0 (E/keV) − Γ. The hydrogen column density NH was fixed during the fit. The unabsorbed flux funabs was derived from the power-law fit.
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