Table 9.
Energetics of the FXRT sample (fluxes are corrected for Galactic and intrinsic absorption, and calculated over the energy range 0.3–10 keV).
| FXRT | ID | Fpeak(erg cm−2 s−1) | LX, peak(erg s−1) | MEdd(M⊙) |
|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) |
| Nearby sample | ||||
| 1 | XRT 000519 (††) | (1.9 ± 0.1) × 10−10 | (6.1 ± 0.3) × 1042 | (4.9 ± 0.3) × 104 |
| 2 | XRT 010908 (††) | (1.7 ± 0.5) × 10−13 | (1.8 ± 0.5) × 1039 | 13.9 ± 4.1 |
| 3 | XRT 070530 (††) | (2.7 ± 1.1) × 10−12 | (5.3 ± 2.1) × 1039 | 41.8 ± 17.0 |
| 4 | XRT 071203 (††) | (6.4 ± 2.5) × 10−14 | (3.6 ± 1.4) × 1038 | 2.9 ± 1.1 |
| 5 | XRT 080331 (††) | (1.7 ± 0.3) × 10−12 | (1.3 ± 0.2) × 1040 | 105.9 ± 18.7 |
| 6 | XRT 130822 (††) | (2.3 ± 0.9) × 10−13 | (2.4 ± 0.9) × 1040 | 187.5 ± 73.4 |
| Distant sample | ||||
| 7 | XRT 030511 (†) | (2.3 ± 0.3) × 10−12 | (1.3 ± 0.2) × 1046 | (9.9 ± 1.3) × 107 |
| 8 | XRT 041230 (††) | (6.9 ± 3.4) × 10−14 | (1.1 ± 0.5) × 1044 | (8.8 ± 4.3) × 105 |
| 9 | XRT 080819 (††) | (6.5 ± 2.9) × 10−13 | (1.5 ± 0.7) × 1045 | (1.2 ± 0.5) × 107 |
| 10 | XRT 100831 (†) | (8.9 ± 3.4) × 10−13 | (4.8 ± 1.8) × 1045 | (3.8 ± 1.5) × 107 |
| 11 | XRT 110103 (a) | (2.2 ± 0.2) × 10−10 | (2.4 ± 0.2) × 1044 | (1.9 ± 0.2) × 106 |
| 12 | XRT 110919 (†) | (5.6 ± 1.3) × 10−13 | (3.0 ± 0.7) × 1045 | (2.4 ± 0.6) × 107 |
| 13 | XRT 140327 (†) | (1.2 ± 0.5) × 10−13 | (6.3 ± 2.8) × 1044 | (4.9 ± 2.3) × 106 |
| 14 | XRT 141001 (b) | (4.3 ± 1.1) × 10−12 | (1.7 ± 0.4) × 1047 | (1.3 ± 0.3) × 109 |
Notes. Column 1: FXRT candidate number. Column 2: Candidate ID. Column 3 and 4: X-ray peak flux and isotropic luminosity in cgs units (corrected for Galactic and intrinsic absorption). Column 5: Eddington mass (defined as MEdd = 7.7 × 10−39LX, peak) in solar mass units (M⊙).
Assuming an association with Abell 3581 at 94.9 Mpc (Glennie et al. 2015).
Assuming a mean redshift of z = 2.23 (Bauer et al. 2017).
The distance or redshift is taken from Table 8.
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