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Table 4
Summary of the cases with different photometric bands for the mutual information decomposition. Galactic reddening E(B – V) is included in all the datasets.
| <IX, I\X> | The set IX contains images from one single optical band or two adjacent bands, and the set I\X contains images from the remaining bands, running over all the five optical bands u, 𝑔, r, i, ɀ. For example, < I𝑔r, I\𝑔r > refers to the case in which one set contains images in the 𝑔 and r bands, and the other set contains images in the u, i, and ɀ bands. In total, there are five possibilities of separating out one band and four possibilities of separating out two bands. |
| <MX,M\X> | The set MX contains magnitudes and errors from one single band or two adjacent bands, and the set M\X contains those from the remaining bands, running over all the five optical bands u, 𝑔, r, i, ɀ and the three infrared bands W1, W2, W3 (except errors in the W3 band). In total, there are eight possibilities of separating out one band and seven possibilities of separating out two bands. |
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