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Table 9

SPICES performance summary for exoplanet spectroscopic characterization.

Planet Probed property Stellar type Sections
A0 G2 M0

Jupiter Rayleigh scattering 1 AU  ≤ a  ≤  4.2 AU 0.25 AU  ≤  a  ≤  0.8 AU 2.4.1, 4.2, and 5
5 pc  ≤  d  ≤  17 pc 1.3 pc  ≤  d  ≤  4 pc
0.5 RJ  ≤  Rp  ≤  1.1 RJ 0.5 RJ  ≤  Rp  ≤  1.1 RJ
Solar metallicity 1x/3x 1 AU  ≤  a  ≤  4.2 AU 0.25 AU  ≤  a  ≤  5 AU 0.25 AU  ≤  a  ≤  3 AU
5 pc  ≤  d  ≤  17 pc 1.3 pc  ≤  d  ≤  10 pc 1.3 pc  ≤  d  ≤  7.5 pc
0.6 RJ  ≤  Rp  ≤  1.1 RJ 0.5 RJ  ≤  Rp  ≤  1.1 RJ 0.5 RJ  ≤  Rp  ≤  1.1 RJ

Neptune Rayleigh scattering 0.25 AU  ≤  a  ≤  0.8 AU 2.4.1, 4.3, and 5
1.3 pc  ≤  d  ≤  4 pc
0.5 RN  ≤  Rp  ≤  1.5 RN
Solar metallicity 10x/30x 0.25 AU  ≤  a  ≤  2 AU 0.25 AU  ≤  a  ≤  1.5 AU
1.3 pc  ≤  d  ≤  8.5 pc 1.3 pc  ≤  d  ≤  3 pc
0.5 RN  ≤  Rp  ≤  1.5 RN 0.5 RN  ≤  Rp  ≤  1.5 RN

Earth Cloud coverage 0/50/100% 0.25 AU  ≤  a  ≤  1 AU 0.25 AU  ≤  a  ≤  0.6 AU 2.4.2, 4.4, and 5
1.3 pc  ≤  d  ≤  5 pc 1.3 pc  ≤  d  ≤  3 pc
RE  ≤  Rp  ≤  2.5 RE 1.1 RE  ≤  Rp  ≤  2.5 RE
Forest coverage 0/50/100% clouds = 0% 0.25 AU  ≤  a  ≤  1 AU 0.25 AU  ≤  a  ≤  0.6 AU
1.3 pc  ≤  d  ≤  5 pc 1.3 pc  ≤  d  ≤  3 pc
1.1 RE  ≤  Rp  ≤  2.5 RE 1.2 RE  ≤  Rp  ≤  2.5 RE
Forest coverage 0/50/100% clouds = 50% 0.25 AU  ≤  a  ≤  1 AU 0.25 AU  ≤  a  ≤  0.6 AU
1.3 pc  ≤  d  ≤  4 pc 1.3 pc  ≤  d  ≤  2.8 pc
1.1 RE  ≤  Rp  ≤  2.5 RE 1.4 RE  ≤  Rp  ≤  2.5 RE

Notes. We strongly encourage the reader to refer to the rest of the paper to access the assumptions and the detail of the studies.

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