Table A.1.
Measurements of Chandra X-ray fluxes and luminosities based on the absorbed model flux. Luminosity range within the 90% interval is presented in the parentheses. We assume a power law model with a power law index of 2. The last two source have very few photons, 4303-41 has three and 1566-5 only has one. Qualitatively these are likely incidental and the fluxes are just an absolute upper limit. Distances to the host galaxies are adopted from Anand et al. (2021).
| Source Name | Absorbed model flux | Flux 90% conf. | Lx 0.5-7.0 keV | Adopted distance |
|---|---|---|---|---|
| [erg/cm2/s] | [erg/cm2/s] | [⋅ 1037 erg/s] | [Mpc] | |
| 4303-46 | 1.74e-14 | (1.47e-14, 2.01e-14) | 60.1 (50.0,69.4) | 16.99±3.04 |
| 4303-20 | 1.21e-15 | (5.82e-16, 2.12e-15) | 4.18 (2.0,7.3) | 16.99±3.04 |
| 3627-1 | 7.14e-15 | (5.43e-15, 8.86e-15) | 10.9 | 11.32±0.48 |
| 3351-5 | 4.02e-15 | (2.82e-15, 5.51e-15) | 4.78 (3.3,6.5) | 9.96±0.33 |
| 3627-17 | 1.22e-14 | (9.97e-15, 1.44e-14) | 18.7 (15.3,22.1) | 11.32±0.48 |
| 4303-41 | 6.73e-16 | (1.83e-16, 1.44e-15) | 2.32 (0.6,5.0) | 16.99±3.04 |
| 1566-4 | 3.82e-15 | (1.22e-16, 1.57e-14) | 14.3 (0.4,58.8) | 17.69±2.00 |
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