Open Access
Table A.1
Physical variables collected for showing their correlation with the latent space extracted by the autoencoder.
| Variable | Description |
|---|---|
| Fs | Average soft band flux (0.5 - 1.2 keV) |
| Fb | Average broad band flux (0.5 - 7 keV) |
| Fm | Average medium band flux (1.2 - 2 keV) |
| Fh | Average hard band flux (2 - 7 keV) |
| hard_hs | hard (2.0-7.0 keV) - soft (0.5-1.2 keV) energy band hardness ratio |
| hard_ms | medium (1.2-2.0 keV) - soft (0.5-1.2 keV) energy band hardness ratio |
| hard_hm | hard (2.0-7.0 keV) - medium (1.2-2.0 keV) energy band hardness ratio |
| var_prob_b | Gregory-Loredo variability probability values |
| var_index_b | Intra-observation Gregory-Loredo variability index |
| powlaw_gamma | photon index, defined as FE ∝ E−γ, of the best fitting absorbed power-law model spectrum to the source region aperture pulse invariant (PI) spectrum |
| powlaw_nh | NH column density of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum |
| bb_kt | temperature (kT) of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum |
| bb_nh | NH column density of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum |
| brems_kt | temperature (kT) of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum |
| brems_nh | NH column density of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum |
| apec_kt | temperature (kT) of the best fitting absorbed astrophysical plasma emission code (APEC) model spectrum to the source region aperture PI spectrum |
| apec_abund | abundance of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum |
| apec_z | redshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum |
| apec_nh | NH column density of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum |
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