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- making the Figure and Table for AGN-MAESTLO in the same format with Fig. 1 and Tab. 1 of the MAESTLO paper
- evaluating the contribution of the power-law component on the SED fitting (ref. Caputi 2013, ApJ, 768, 103) for one AGN-MAESTLO (e.g., ID 608131) at least.
- checking whether there are emission-line objects classified as AGN (IRAC, X-ray, radio) in the sample with reduced chi-square > 3 in steps 2 & 3.
- Tab. 1:
as of xxx †
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