This table shows the estimated distances to various BH-LMXBs using the statistical framework developed in the study Abdulghani et. al. 2024.
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Select an instrument to view distance estimates based on that instrument's X-ray spectral data:
Source Name | Outburst Year(s) | Distance (kpc) |
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Sources with an asterisk (*) are obtained through soft-only constraints.
If you use our estimates, please reference our work.
Last updated: 8/6/2024