Table 2.
X-ray properties of ABC sources.
| Name ALMA | Detector | EXP | Count rate | S/N | Flux0.1−2.4 | ΓX | K | χ2 (d.o.f.) |
|---|---|---|---|---|---|---|---|---|
| ks | 10−3 s−1 | 10−13 erg cm2 s−1 | 10−4 keV cm−2 s−1 | |||||
| J0010−0433 | XRT | 1.3 | ||||||
| J0011−8706 | XRT | 4.9 | 2.55 ± 0.84 | 3.0 | 0.87 ± 0.29 | |||
| J0019−5641 | XRT | 2.9 | ||||||
| J0024−6820 | XRT | 0.7 | 13.25 ± 5.00 | 2.6 | 3.82 ± 1.44 | |||
| J0025+3919 | ACIS | 19.7 | 15.70 ± 1.00 | 15.7 | 2.04 ± 0.35 |  |
 |
0.8(24) |
| J0028+2000 | XRT | 3.0 | ||||||
| J0029+3456 | EPIC | 28.2 | 66.77 ± 3.08 | 21.7 | 2.15 ± 0.10 | |||
| J0034−0054 | ACIS | 2.0 | 14.60 ± 2.90 | 5.0 | 2.54 ± 0.50 | |||
| J0039−2220 | XRT | 0.8 | 12.42 ± 4.30 | 2.9 | 3.51 ± 1.21 | |||
| J0045−3705 | XRT | 2.2 |
Notes. For each source we list the name (Name ALMA), the X-ray detector (Detector) and the observation exposure (EXP). If the source is detected we also list the count-rate (Count rate) and the signal to noise ratio (S/N). We then list the unabsorbed source flux (Flux0.1−2.4) in the 0.1−2.4 KeV band, obtained from the count-rate assuming a power-law model with a spectral index 1.8 or, if a spectrum is available, from the spectral fit. For the sources adequately fitted with a power-law model, we also list the power-law spectral index ΓX and normalization K, together with the fit χ2 and degrees of freedom (χ2, d.o.f.). The full table is available in electronic form at the CDS.
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