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Table A.1

Collection of hot Jupiter exoplanets with their reported geometric albedo (Ag) and other stellar and planetary parameters.

Object T* [K] Fe/H Teq [K] log(g) [cgs] a/R* Band Ag
CoRotT-2b 5625 ± 120a 0.0 ± 0.1a 1556 ± 27 3.58 ± 0.03e 6.70 ± 0.03e Corot 0.080.04+0.08Mathematical equation: $0.08^{+0.08}_{-0.04}$f
HAT-P-7b 6350 ± 80a 0.26 ± 0.08a 2264 ± 21 3.30 ± 0.09g 4.15450.0025+0.0029Mathematical equation: $4.1545^{+0.0029}_{-0.0025}$g Kepler 0.09 ± 0.02h
Kepler-7b 5933 ± 50a 0.11 ± 0.05a 1670 ± 17 2.612 ± 0.052a 6.637 ± 0.021g Kepler 0.250.02+0.01Mathematical equation: $0.25^{+0.01}_{-0.02}$m
Kepler-41b 5750 ± 100a 0.38 ± 0.11a 1808 ± 32 2.926 ± 0.057a 5.053 ± 0.021g Kepler 0.130.02+0.01Mathematical equation: $0.13^{+0.01}_{-0.02}$h
Qatar-1b 501388+93Mathematical equation: $5013^{+93}_{-88}$k 0.171 ± 0.096k 1400 ± 28 3.39 ± 0.03k 6.410.10+0.11Mathematical equation: $6.41^{+0.11}_{-0.10}$i TESS 0.14 ± 0.11i
TrES-2b 5850 ± 50a −0.15 ± 0.1a 1458 ± 18 3.30 ± 0.03a 7.9030.016+0.019Mathematical equation: $7.903^{+0.019}_{-0.016}$g Kepler 0.010.01+0.00Mathematical equation: $0.01^{+0.00}_{-0.01}$h
TrES-3b 5650 ± 75a −0.19 ± 0.08a 1613 ± 50 3.40 ± 0.03a 5.820.13+0.12Mathematical equation: $5.82^{+0.12}_{-0.13}$j TESS 0.14 ± 0.13i
WASP-4b 5436 ± 34a −0.05 ± 0.04a 1648 ± 13 3.213 ± 0.098a 5.4380.057+0.044Mathematical equation: $5.438^{+0.044}_{-0.057}$q TESS 0.09 ± 0.09q
WASP-5b 5770 ± 65a 0.09 ± 0.04a 1762 ± 41 3.455 ± 0.043a 5.36 ± 0.22q TESS 0.00020.174+0.166Mathematical equation: $0.0002^{+0.166}_{-0.174}$q
WASP-12b 6250 ± 100a 0.32 ± 0.12a 2526 ± 48 3.015 ± 0.059a 3.0620.066+0.063Mathematical equation: $3.062^{+0.063}_{-0.066}$i TESS 0.13 ± 0.06i
WASP-19b 5500 ± 100a 0.02 ± 0.09a 2055 ± 42 3.222 ± 0.048a 3.5820.067+0.074Mathematical equation: $3.582^{+0.074}_{-0.067}$q TESS 0.17 ± 0.07q
WASP-33b 7430 ± 100r 0.1 ± 0.2r 2764 ± 37 3.459 ± 0.098t 3.614 ± 0.009s TESS −0.04 ± 0.04s
WASP-36b 5900 ± 150a −0.26 ± 0.1a 1738 ± 59 3.540 ± 0.023a 5.760.27+0.26Mathematical equation: $5.76^{+0.26}_{-0.27}$q TESS 0.16 ± 0.15q
WASP-43b 4798 ± 216u −0.13 ± 0.08u 1559 ± 71 3.675 ± 0.019a 4.7340.053+0.054Mathematical equation: $4.734^{+0.054}_{-0.053}$q TESS 0.13 ± 0.06q
WASP-46b 5725 ± 39u −0.18 ± 0.03u 1630 ± 36 3.533 ± 0.036a 6.170.24+0.28Mathematical equation: $6.17^{+0.28}_{-0.24}$q TESS 0.38 ± 0.27q
WASP-64b 5550 ± 150a −0.08 ± 0.11a 1669 ± 54 3.272 ± 0.038a 5.530.25+0.14Mathematical equation: $5.53^{+0.14}_{-0.25}$q TESS 0.38 ± 0.26q
WASP-77Ab 5500 ± 80a 0.00 ± 0.11a 1712 ± 30 3.475 ± 0.020a 5.1620.080+0.120Mathematical equation: $5.162^{+0.120}_{-0.080}$q TESS 0.06 ± 0.05q
WASP-100b 6900 ± 120a −0.03 ± 0.1a 2102 ± 39 3.24 ± 0.14a 5.389 ± 0.064q TESS 0.22 ± 0.08q
WASP-121b 6460 ± 140v 0.13 ± 0.09v 2339 ± 51 2.970 ± 0.017w 3.8150.032+0.018Mathematical equation: $3.815^{+0.018}_{-0.032}$q TESS 0.26 ± 0.06q
HD209458b 6065 ± 50a 0.00 ± 0.05a 1445 ± 13 2.958 ± 0.013a 8.807 ± 0.051z CHEOPS 0.096 ± 0.016z
HD189733b 4969 ± 48α −0.08 ± 0.03α 1179 ± 11 3.332 ± 0.026a 8.8843 ± 0.0175β CHEOPS 0.076 ± 0.016β

CoRoT-1b 6298 ± 66a 0.06 ± 0.07a 2039 ± 24 3.06 ± 0.07b 4.92 ± 0.08b Corot 0.0640.139+0.110Mathematical equation: $0.064^{+0.110}_{-0.139}$c,d
HAT-P-7b 6350 ± 80a 0.26 ± 0.08a 2264 ± 21 3.30 ± 0.09g 4.15450.0025+0.0029Mathematical equation: $4.1545^{+0.0029}_{-0.0025}$g TESS 0.0780.103+0.102Mathematical equation: $0.078^{+0.102}_{-0.103}$i
Kepler-5b 6297 ± 60a 0.04 ± 0.06a 1763 ± 17 3.410 ± 0.034a 6.4500.025+0.021Mathematical equation: $6.450^{+0.021}_{-0.025}$g Kepler 0.097 ± 0.037g,l
Kepler-6b 5647 ± 44a 0.34 ± 0.04a 1461 ± 16 3.062 ± 0.018a 7.503 ± 0.022g Kepler 0.059 ± 0.035g,l
Kepler-8b 6210 ± 150a −0.055 ± 0.03a 1669 ± 16 2.84 ± 0.12a 6.8540.017+0.018Mathematical equation: $6.854^{+0.018}_{-0.017}$g Kepler 0.1090.052+0.050Mathematical equation: $0.109^{+0.050}_{-0.052}$g,n
Kepler-12b 5950 ± 100a 0.07 ± 0.04a 1480 ± 15 2.572 ± 0.045a 8.0190.013+0.014Mathematical equation: $8.019^{+0.014}_{-0.013}$g Kepler 0.084 ± 0.040g,o
Kepler-43b 6050 ± 100a 0.4 ± 0.1a 1620 ± 27 3.766 ± 0.028a 6.9750.047+0.041Mathematical equation: $6.975^{+0.041}_{-0.047}$g Kepler 0.036 ± 0.250g,n
Kepler-76b 6409 ± 95a −0.1 ± 0.2a 2145 ± 33 3.499 ± 0.082a 4.4640.049+0.041Mathematical equation: $4.464^{+0.041}_{-0.049}$g Kepler 0.1480.025+0.028Mathematical equation: $0.148^{+0.028}_{-0.025}$g,n
Kepler-91b 4550 ± 75p 0.11 ± 0.07p 2036 ± 38 3.0 ± 0.1g 2.4960.050+0.043Mathematical equation: $2.496^{+0.043}_{-0.050}$g Kepler 0.3620.234+0.250Mathematical equation: $0.362^{+0.250}_{-0.234}$g,n
Kepler-412b 5750 ± 90a 0.27 ± 0.12a 1848 ± 29 3.117 ± 0.043a 4.8410.024+0.023Mathematical equation: $4.841^{+0.023}_{-0.024}$g Kepler 0.0660.042+0.047Mathematical equation: $0.066^{+0.047}_{-0.042}$g,n
WASP-3b 6400 ± 100a 0.0 ± 0.2a 1947 ± 46 3.368 ± 0.039a 5.40 ± 0.19i TESS 0.1810.197+0.190Mathematical equation: $0.181^{+0.190}_{-0.197}$i
WASP-5b 5770 ± 65a 0.09 ± 0.04a 1762 ± 41 3.455 ± 0.043a 5.36 ± 0.22q TESS 0.00020.174+0.166Mathematical equation: $0.0002^{+0.166}_{-0.174}$q
WASP-18b 6400 ± 100a 0.00 ± 0.09a 2406 ± 40 4.323 ± 0.058a 3.5390.035+0.039Mathematical equation: $3.539^{+0.039}_{-0.035}$q TESS 0.0380.070+0.076Mathematical equation: $-0.038^{+0.076}_{-0.070}$q
WASP-78b 6100 ± 150a −0.35 ± 0.14a 2219 ± 59 2.903 ± 0.064a 3.7780.098+0.060Mathematical equation: $3.778^{+0.060}_{-0.098}$q TESS 0.1890.211+0.207Mathematical equation: $0.189^{+0.207}_{-0.211}$q
WASP-189b 8000 ± 80x 0.29 ± 0.13x 2641 ± 28 3.27 ± 0.05x 4.5870.034+0.037Mathematical equation: $4.587^{+0.037}_{-0.034}$y CHEOPS 0.2020.048+0.046Mathematical equation: $0.202^{+0.046}_{-0.048}$n,y

Notes. Objects in the top half of the table have their albedos taken directly from previous analyses (where thermal decontamination has been carried out). For objects in the lower half, using measured eclipse depths and dayside temperatures from the references specified, we have calculated the thermally decontaminated geometric albedos (see method in Section 2.1). The ‘Band’ column details which bandpass the planet’s eclipse depth was measured in, and therefore which bandpass the geometric albedo corresponds to. Teq refers to the equilibrium temperature of the planet, calculated from the other values in this table using Equation 6. (a)Bonomo et al. (2017), (b)Barge et al. (2008), (c)Deming et al. (2011), (d) Alonso et al. (2009), (e)Alonso et al. (2008), (f)Dang et al. (2018), (g)Esteves et al. (2015), (h)Morris et al. (2024), (i)Wong et al. (2021), (j)Patel & Espinoza (2022), (k)Collins et al. (2017), (l)Désert et al. (2011), (m)Heng et al. (2021), (n)Beatty et al. (2019), (o)Fortney et al. (2011), (p)Lillo-Box et al. (2014), (q)Wong et al. (2020), (r)Collier Cameron et al. (2010), (s)von Essen et al. (2020), (t)Turner et al. (2016), (u)Sousa et al. (2018), (v)Delrez et al. (2016), (w)Bourrier et al. (2020), (x)Lendl et al. (2020), (y)Deline et al. (2022), (z)Brandeker et al. (2022), (α)Sousa et al. (2021), (β)Krenn et al. (2023)

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