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 |
f
|
| HAT-P-7b | 6350 ± 80a | 0.26 ± 0.08a | 2264 ± 21 | 3.30 ± 0.09g |
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 |
m
|
| Kepler-41b | 5750 ± 100a | 0.38 ± 0.11a | 1808 ± 32 | 2.926 ± 0.057a | 5.053 ± 0.021g | Kepler |
h
|
| Qatar-1b |
k
|
0.171 ± 0.096k | 1400 ± 28 | 3.39 ± 0.03k |
i
|
TESS | 0.14 ± 0.11i |
| TrES-2b | 5850 ± 50a | −0.15 ± 0.1a | 1458 ± 18 | 3.30 ± 0.03a |
g
|
Kepler |
h
|
| TrES-3b | 5650 ± 75a | −0.19 ± 0.08a | 1613 ± 50 | 3.40 ± 0.03a |
j
|
TESS | 0.14 ± 0.13i |
| WASP-4b | 5436 ± 34a | −0.05 ± 0.04a | 1648 ± 13 | 3.213 ± 0.098a |
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 |
q
|
| WASP-12b | 6250 ± 100a | 0.32 ± 0.12a | 2526 ± 48 | 3.015 ± 0.059a |
i
|
TESS | 0.13 ± 0.06i |
| WASP-19b | 5500 ± 100a | 0.02 ± 0.09a | 2055 ± 42 | 3.222 ± 0.048a |
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 |
q
|
TESS | 0.16 ± 0.15q |
| WASP-43b | 4798 ± 216u | −0.13 ± 0.08u | 1559 ± 71 | 3.675 ± 0.019a |
q
|
TESS | 0.13 ± 0.06q |
| WASP-46b | 5725 ± 39u | −0.18 ± 0.03u | 1630 ± 36 | 3.533 ± 0.036a |
q
|
TESS | 0.38 ± 0.27q |
| WASP-64b | 5550 ± 150a | −0.08 ± 0.11a | 1669 ± 54 | 3.272 ± 0.038a |
q
|
TESS | 0.38 ± 0.26q |
| WASP-77Ab | 5500 ± 80a | 0.00 ± 0.11a | 1712 ± 30 | 3.475 ± 0.020a |
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 |
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 |
c,d
|
| HAT-P-7b | 6350 ± 80a | 0.26 ± 0.08a | 2264 ± 21 | 3.30 ± 0.09g |
g
|
TESS |
i
|
| Kepler-5b | 6297 ± 60a | 0.04 ± 0.06a | 1763 ± 17 | 3.410 ± 0.034a |
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 |
g
|
Kepler |
g,n
|
| Kepler-12b | 5950 ± 100a | 0.07 ± 0.04a | 1480 ± 15 | 2.572 ± 0.045a |
g
|
Kepler | 0.084 ± 0.040g,o |
| Kepler-43b | 6050 ± 100a | 0.4 ± 0.1a | 1620 ± 27 | 3.766 ± 0.028a |
g
|
Kepler | 0.036 ± 0.250g,n |
| Kepler-76b | 6409 ± 95a | −0.1 ± 0.2a | 2145 ± 33 | 3.499 ± 0.082a |
g
|
Kepler |
g,n
|
| Kepler-91b | 4550 ± 75p | 0.11 ± 0.07p | 2036 ± 38 | 3.0 ± 0.1g |
g
|
Kepler |
g,n
|
| Kepler-412b | 5750 ± 90a | 0.27 ± 0.12a | 1848 ± 29 | 3.117 ± 0.043a |
g
|
Kepler |
g,n
|
| WASP-3b | 6400 ± 100a | 0.0 ± 0.2a | 1947 ± 46 | 3.368 ± 0.039a | 5.40 ± 0.19i | TESS |
i
|
| WASP-5b | 5770 ± 65a | 0.09 ± 0.04a | 1762 ± 41 | 3.455 ± 0.043a | 5.36 ± 0.22q | TESS |
q
|
| WASP-18b | 6400 ± 100a | 0.00 ± 0.09a | 2406 ± 40 | 4.323 ± 0.058a |
q
|
TESS |
q
|
| WASP-78b | 6100 ± 150a | −0.35 ± 0.14a | 2219 ± 59 | 2.903 ± 0.064a |
q
|
TESS |
q
|
| WASP-189b | 8000 ± 80x | 0.29 ± 0.13x | 2641 ± 28 | 3.27 ± 0.05x |
y
|
CHEOPS |
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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