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Table 6

Thermal phase-curve parameters of UHJs observed with Spitzer/IRAC.

Planet Wavelength (µm) Tday (K) Tnight (K) Ab () ɛ ()
WASP-19 b (i) 3.6 −10.5 ± 4.0
4.5 2357 ± 64 −12.9 ± 3.6

HAT-P-7 b(i) 3.6 2632 ± 77 <1360 (2σ) 6.8 ± 7.5 <0.02 (2σ)
4.5 2682 ± 49 1710 ± 180 4.1 ± 7.5

WASP-76 b(ii) 3.6 2471 ± 27 1518 ± 61 −0.68 ± 0.48 0.31 ± 0.04
4.5 2699 ± 32 1259 ± 44 −0.67 ± 0.20 0.05 ± 0.09

WASP-33 b(iii) 3.6 3082 ± 92 −12.8 ± 5.8 0.34 ± 0.06
4.5 −19.8 ± 3.0 0.12 ± 0.03

WASP-121 b(iv) 3.6 5.9 ± 1.6
4.5

KELT-1b (v) 3.6 2988 ± 60 −28.4 ± 3.5
4.5 2902 ± 74 −18.6 ± 5.2

WASP-103 b(vi) 3.6 2995 ± 159 1523 ± 153 −2.0 ± 0.7
4.5 3154 ± 99 1288 ± 118 −1.0 ± 0.4

WASP-12 b(vii) 3.6 2744 ± 48 1510 ± 210 N.A.
3.6 2813 ± 48 1760 ± 97 N.A. 0.33 ± 0.06
4.5 2989 ± 66 790 ± 150 N.A.
4.5 2854 ± 74 1340 ± 180 N.A.

KELT-9 b(viii) 4.5 0.23 ± 0.04

Notes. The brightness temperatures and hot-spot offsets were extracted from the literature, and used to calculate the Bond albedo and circulation efficiency.

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