Research Article
An Improved Infrared/Visible Fusion for Astronomical Images
Table 1
Quantitative comparison.
| Dataset | Technique | | | | | | | | |
| Andromeda galaxy (M31) | Proposed | 0.8220 | 0.8319 | 0.7707 | 0.4804 | 0.6461 | 0.3487 | 0.6612 | 0.4615 | Ellmauthaler et al. [8] | 0.7179 | 0.8444 | 0.7345 | 0.3647 | 0.6350 | 0.2229 | 0.5610 | 0.3387 | MSVD [28] | 0.6452 | 0.6946 | 0.6243 | 0.4148 | 0.4535 | 0.4432 | 0.0045 | 0.2675 | NSCT [27] | 0.6259 | 0.6003 | 0.5576 | 0.2641 | 0.4606 | 0.1777 | 0.3432 | 0.2689 | DTCWT [26] | 0.7085 | 0.8134 | 0.6573 | 0.3113 | 0.5436 | 0.1682 | 0.2682 | 0.2290 | RP [25] | 0.4706 | 0.5416 | 0.5102 | 0.2514 | 0.3970 | 0.5282 | 0.2075 | 0.2026 |
| Jupiter’s moon | Proposed | 0.7927 | 0.7255 | 0.7814 | 0.4622 | 0.7566 | 0.3433 | 0.6725 | 0.5617 | Ellmauthaler et al. [8] | 0.2832 | 0.6477 | 0.6343 | 0.4230 | 0.7398 | 0.1768 | 0.5672 | 0.5614 | MSVD [28] | 0.4780 | 0.4970 | 0.5217 | 0.5243 | 0.5292 | 0.4599 | 0.0065 | 0.4923 | NSCT [27] | 0.4155 | 0.4083 | 0.4631 | 0.5279 | 0.5212 | 0.2672 | 0.5001 | 0.6139 | DTCWT [26] | 0.4571 | 0.5932 | 0.5851 | 0.3476 | 0.5973 | 0.1805 | 0.4785 | 0.4844 | RP [25] | 0.3467 | 0.3989 | 0.4022 | 0.4749 | 0.3919 | 0.4825 | 0.0183 | 0.3634 |
| Nabula (M16) | Proposed | 0.7399 | 0.4896 | 0.8461 | 0.8587 | 0.8645 | 0.7646 | 0.7553 | 0.5652 | Ellmauthaler et al. [8] | 0.7318 | 0.4230 | 0.8446 | 0.8494 | 0.8563 | 0.5736 | 0.5424 | 0.5494 | MSVD [28] | 0.4918 | 0.4120 | 0.6466 | 0.6704 | 0.6539 | 0.5598 | 0.0051 | 0.4331 | NSCT [27] | 0.5204 | 0.2980 | 0.6037 | 0.5899 | 0.6013 | 0.4916 | 0.3953 | 0.5058 | DTCWT [26] | 0.6736 | 0.3608 | 0.8023 | 0.8225 | 0.8125 | 0.4477 | 0.4631 | 0.5079 | RP [25] | 0.5885 | 0.3099 | 0.6834 | 0.6818 | 0.6934 | 0.6597 | 0.1708 | 0.4639 |
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