Table 6.
Features selected as the ones that better disentangles obscured AGN and inactive galaxies based on the results of the K-S test comparing, for each feature, the corresponding distributions for these two classes of sources.
| Feature | D | prob |
|---|---|---|
| Autocor_length_r | 0.611 | 10−31 |
| SF_ML_amplitude_r | 0.577 | 10−28 |
| SF_ML_gamma_r | 0.547 | 10−25 |
| Autocor_length_g | 0.448 | 10−17 |
| i-z | 0.376 | 10−12 |
| r-i | 0.366 | 10−11 |
| MedianBRP_diff | 0.353 | 10−10 |
| Rcs_r | 0.334 | 10−9 |
| u-B | 0.317 | 10−8 |
| z-y | 0.315 | 10−8 |
| Autocor_length_diff | 0.296 | 10−7 |
| ch21 | 0.295 | 10−7 |
| Etae_r | 0.291 | 10−7 |
| class_star_hst | 0.287 | 10−7 |
| Pvar_r | 0.285 | 10−7 |
| ExcessVar_r | 0.283 | 10−7 |
| MHAOV_Period_r | 0.283 | 10−7 |
| GP_DRW_tau_r | 0.281 | 10−7 |
| GP_DRW_sigma_r | 0.275 | 10−6 |
| SF_ML_amplitude_diff | 0.269 | 10−6 |
| Q31_g | 0.267 | 10−6 |
| MedianAbsDev_g | 0.262 | 10−6 |
| MaxSlope_diff | 0.258 | 10−6 |
| Period_fit_r | 0.256 | 10−5 |
| IARϕ_r | 0.251 | 10−5 |
Notes. The features are listed in descending order of the distance D returned by the test, which represents the maximum distance between the two cumulative distributions compared; the table also reports the corresponding probability to obtain by chance a larger value for this distance.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.