Table 3
Results from modelling spectrophotometric light curves produced with 100 Å integration bins, for both data sets.
Band | Spectrophotometric LC set | |||||
|
||||||
Centre | RAW | CMC | ||||
|
||||||
[Å] | Rp/R ⋆ | c 1 | c 2 | Rp/R ⋆ | c 1 | c 2 |
|
||||||
5750 | 0.1207 ± 0.0023 | 0.0866 ± 0.3687 | 0.5760 ± 0.6236 | 0.1212 ± 0.0022 | 0.0921 ± 0.0604 | 0.5687 ± 0.1396 |
5800 | 0.1222 ± 0.0032 | 0.0902 ± 0.1368 | 0.5799 ± 0.2794 | 0.1229 ± 0.0038 | 0.0953 ± 0.0630 | 0.5805 ± 0.1485 |
5850 | 0.1248 ± 0.0018 | 0.0880 ± 0.1404 | 0.6034 ± 0.2849 | 0.1223 ± 0.0020 | 0.0833 ± 0.0605 | 0.5959 ± 0.1419 |
5900 | 0.1214 ± 0.0023 | 0.1415 ± 0.1136 | 0.5714 ± 0.2347 | 0.1210 ± 0.0011 | 0.1436 ± 0.0753 | 0.5685 ± 0.1666 |
5950 | 0.1234 ± 0.0032 | 0.2407 ± 0.1366 | 0.4574 ± 0.2537 | 0.1226 ± 0.0014 | 0.2300 ± 0.0855 | 0.4552 ± 0.1636 |
6000 | 0.1239 ± 0.0014 | 0.1706 ± 0.0846 | 0.4926 ± 0.1748 | 0.1235 ± 0.0013 | 0.1679 ± 0.0722 | 0.4825 ± 0.1373 |
6050 | 0.1246 ± 0.0014 | 0.1195 ± 0.0665 | 0.5695 ± 0.1387 | 0.1242 ± 0.0011 | 0.1173 ± 0.0613 | 0.5533 ± 0.1213 |
6100 | 0.1249 ± 0.0015 | 0.1511 ± 0.0833 | 0.4923 ± 0.1803 | 0.1247 ± 0.0014 | 0.1529 ± 0.0760 | 0.4878 ± 0.1544 |
6150 | 0.1255 ± 0.0028 | 0.1618 ± 0.1428 | 0.5370 ± 0.2924 | 0.1250 ± 0.0022 | 0.1539 ± 0.0836 | 0.5249 ± 0.1644 |
6200 | 0.1237 ± 0.0020 | 0.1195 ± 0.0590 | 0.6025 ± 0.1184 | 0.1236 ± 0.0008 | 0.1018 ± 0.0557 | 0.5837 ± 0.1114 |
6250 | 0.1260 ± 0.0033 | 0.1030 ± 0.1534 | 0.6200 ± 0.2926 | 0.1246 ± 0.0012 | 0.0736 ± 0.0472 | 0.5971 ± 0.1029 |
6300 | 0.1239 ± 0.0021 | 0.0944 ± 0.0639 | 0.6260 ± 0.1266 | 0.1229 ± 0.0013 | 0.0784 ± 0.0480 | 0.6074 ± 0.1017 |
6350 | 0.1218 ± 0.0015 | 0.1252 ± 0.0657 | 0.5344 ± 0.1347 | 0.1219 ± 0.0004 | 0.1314 ± 0.0625 | 0.5205 ± 0.1243 |
6400 | 0.1235 ± 0.0015 | 0.1463 ± 0.0663 | 0.4382 ± 0.1358 | 0.1228 ± 0.0011 | 0.1424 ± 0.0616 | 0.4168 ± 0.1272 |
6450 | 0.1240 ± 0.0017 | 0.1813 ± 0.0897 | 0.3792 ± 0.1746 | 0.1244 ± 0.0023 | 0.1767 ± 0.0821 | 0.3679 ± 0.1587 |
6500 | 0.1228 ± 0.0017 | 0.1932 ± 0.0940 | 0.3895 ± 0.1896 | 0.1243 ± 0.0024 | 0.1874 ± 0.0893 | 0.3776 ± 0.1579 |
6600 | 0.1225 ± 0.0015 | 0.1168 ± 0.0552 | 0.4415 ± 0.1206 | 0.1229 ± 0.0006 | 0.1067 ± 0.0508 | 0.4298 ± 0.1094 |
6650 | 0.1227 ± 0.0015 | 0.1600 ± 0.0593 | 0.4636 ± 0.1274 | 0.1229 ± 0.0011 | 0.1589 ± 0.0703 | 0.4542 ± 0.1478 |
6700 | 0.1227 ± 0.0011 | 0.2447 ± 0.0866 | 0.3224 ± 0.1793 | 0.1230 ± 0.0008 | 0.2325 ± 0.0645 | 0.3166 ± 0.1363 |
6750 | 0.1225 ± 0.0011 | 0.1929 ± 0.0707 | 0.3577 ± 0.1430 | 0.1223 ± 0.0009 | 0.1913 ± 0.0609 | 0.3463 ± 0.1212 |
6800 | 0.1228 ± 0.0018 | 0.1136 ± 0.1253 | 0.4925 ± 0.2640 | 0.1224 ± 0.0006 | 0.1083 ± 0.0488 | 0.4858 ± 0.1047 |
6850 | 0.1224 ± 0.0013 | 0.1323 ± 0.1089 | 0.4441 ± 0.2315 | 0.1224 ± 0.0006 | 0.1284 ± 0.0490 | 0.4453 ± 0.1030 |
6900 | 0.1226 ± 0.0015 | 0.1553 ± 0.0876 | 0.4365 ± 0.1818 | 0.1224 ± 0.0010 | 0.1530 ± 0.0624 | 0.4320 ± 0.1255 |
6950 | 0.1236 ± 0.0021 | 0.1792 ± 0.0937 | 0.4279 ± 0.1759 | 0.1226 ± 0.0013 | 0.1730 ± 0.0728 | 0.4104 ± 0.1383 |
7000 | 0.1225 ± 0.0014 | 0.2107 ± 0.0926 | 0.3906 ± 0.1845 | 0.1230 ± 0.0011 | 0.2049 ± 0.0846 | 0.3826 ± 0.1751 |
7050 | 0.1225 ± 0.0015 | 0.1615 ± 0.0776 | 0.5082 ± 0.1579 | 0.1217 ± 0.0012 | 0.1498 ± 0.0638 | 0.4881 ± 0.1244 |
7100 | 0.1230 ± 0.0012 | 0.1782 ± 0.0843 | 0.4435 ± 0.1782 | 0.1232 ± 0.0014 | 0.1830 ± 0.0839 | 0.4398 ± 0.1704 |
7150 | 0.1233 ± 0.0012 | 0.2003 ± 0.0837 | 0.3785 ± 0.1791 | 0.1238 ± 0.0009 | 0.1963 ± 0.0735 | 0.3733 ± 0.1527 |
7200 | 0.1241 ± 0.0018 | 0.1881 ± 0.0879 | 0.3795 ± 0.1697 | 0.1238 ± 0.0011 | 0.1774 ± 0.0674 | 0.3754 ± 0.1308 |
7250 | 0.1232 ± 0.0012 | 0.2840 ± 0.0928 | 0.1941 ± 0.1906 | 0.1232 ± 0.0010 | 0.2777 ± 0.0662 | 0.1884 ± 0.1334 |
7300 | 0.1230 ± 0.0019 | 0.2174 ± 0.0878 | 0.3023 ± 0.1639 | 0.1223 ± 0.0010 | 0.2045 ± 0.0626 | 0.2919 ± 0.1247 |
7350 | 0.1222 ± 0.0013 | 0.1704 ± 0.0809 | 0.4045 ± 0.1555 | 0.1225 ± 0.0004 | 0.1567 ± 0.0549 | 0.3862 ± 0.1014 |
7400 | 0.1225 ± 0.0016 | 0.1314 ± 0.0922 | 0.4483 ± 0.1680 | 0.1222 ± 0.0006 | 0.1132 ± 0.0468 | 0.4338 ± 0.0899 |
7450 | 0.1222 ± 0.0017 | 0.2164 ± 0.0996 | 0.3218 ± 0.1787 | 0.1233 ± 0.0004 | 0.1995 ± 0.0640 | 0.3082 ± 0.1105 |
7500 | 0.1222 ± 0.0018 | 0.1780 ± 0.0511 | 0.3904 ± 0.1049 | 0.1240 ± 0.0015 | 0.1652 ± 0.0797 | 0.3758 ± 0.1461 |
7700 | 0.1267 ± 0.0037 | 0.1024 ± 0.1140 | 0.4673 ± 0.1980 | 0.1244 ± 0.0009 | 0.1015 ± 0.0831 | 0.4703 ± 0.1635 |
7750 | 0.1237 ± 0.0025 | 0.0691 ± 0.0975 | 0.5359 ± 0.1698 | 0.1231 ± 0.0006 | 0.0680 ± 0.0396 | 0.5373 ± 0.0822 |
7800 | 0.1227 ± 0.0025 | 0.1053 ± 0.0932 | 0.4935 ± 0.1570 | 0.1225 ± 0.0011 | 0.1004 ± 0.0621 | 0.4931 ± 0.1110 |
7850 | 0.1253 ± 0.0036 | 0.1225 ± 0.1267 | 0.4833 ± 0.2386 | 0.1222 ± 0.0017 | 0.1229 ± 0.0765 | 0.4814 ± 0.1331 |
7900 | 0.1227 ± 0.0025 | 0.1632 ± 0.0769 | 0.3366 ± 0.1724 | 0.1227 ± 0.0017 | 0.1591 ± 0.0918 | 0.3217 ± 0.1978 |
7950 | 0.1305 ± 0.0035 | 0.1006 ± 0.1259 | 0.3853 ± 0.2108 | 0.1245 ± 0.0018 | 0.0832 ± 0.0587 | 0.3697 ± 0.1072 |
Notes. The corresponding CMC light curves are given in Figs. 7. The three transit parameters, taken as free during the MCMC analysis, namely the relative planetary radius (Rp/R⋆) and the two coefficients of the quadratic limb darkening law (c1 and c2) are shown. Other free components for each channel were the 3 coefficients of the polynomial fit, as well as the 3 noise model parameters.
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