File Name : fig.s1.jpg Caption : variation of lattice constant of cubic lamo3 (m=al, ga, sc, fe, co, cr, ti, v) and asno₃ (a=ba, ca, cd, co, fe, mn, mg, ni, sr, ti, v, zn). File Name : fig.s2.jpg Caption : fig. s2. average solar absorptivity (250–2500 nm) of 76 abo₃perovskites. File Name : fig. s3.jpg Caption : fig. s3. reflectivity (250–2500 nm) of 76 abo₃perovskites. File Name : fig. s4.jpg Caption : fig. s4. absorption spectra (0–1000nm) of laalo₃-c, laalo₃-t, laalo₃-tric, laalo₃-m, laalo₃-o, lacro₃-o, lafeo₃-o, lagao₃-o, lasco₃-o, and latio₃-o. File Name : fig.s5.jpg Caption : the ratio of solar absorption (250-2500 nm) to ir emittance (2.5-25 μm) (α_s/ε) of 76 abo₃ perovskites. File Name : fig. s6.jpg Caption : fig. s6. the atomic models of cubic (a), hexhagonal (b), tetragonal (c), rhombohedral (d), trigonal (e), triclinic (f), orthorhombic (g), and monoclinic (h) for abo₃ perovskites. the small turquoise balls are oxygen atoms, big darkslateblue balls are b-site atoms, and grey-pink balls are a-site atoms.