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Table B.2
Planetary radius (in stellar radius units) as a function of wavelength (transmission spectrum), as obtained from our analysis (four-slice binning).
| Central λ | Rp∕R⋆ |
|---|---|
| (nm) | |
| 381 | 0.1151 |
| 386 | 0.1201 |
| 391 | 0.1198 |
| 396 | 0.1198 |
| 401 | 0.1203 |
| 406 | 0.1206 |
| 412 | 0.1203 |
| 417 | 0.1199 |
| 423 | 0.1193 |
| 429 | 0.1203 |
| 435 | 0.1214 |
| 441 | 0.1208 |
| 448 | 0.1199 |
| 455 | 0.1197 |
| 461 | 0.1217 |
| 468 | 0.1216 |
| 476 | 0.1217 |
| 483 | 0.1200 |
| 491 | 0.1192 |
| 499 | 0.1203 |
| 507 | 0.1203 |
| 516 | 0.1198 |
| 523 | 0.1199 |
| 530 | 0.1207 |
| 539 | 0.1204 |
| 549 | 0.1226 |
| 559 | 0.1205 |
| 569 | 0.1238 |
| 580 | 0.1225 |
| 588 | 0.1220 |
| 603 | 0.1240 |
| 615 | 0.1240 |
| 627 | 0.1223 |
| 641 | 0.1218 |
| 661 | 0.1254 |
| 680 | 0.1218 |
| 746 | 0.1193 |
| 779 | 0.1171 |
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