Table 3
Values derived analyzing chromatic light curves while considering the detrending model f5(t).
| WC | CW | u1 | u2 | RP/RS | a 0 | a 1 | A 1 | ν 1 | φ 1 | SDR | β N |
|
|
|||||||||||
| 5100–5500 | 20.0 | 0.7527 | 0.0385 | 0.1529 ± 0.0003 | 1.008(9) | 0.014(5) | 0.001(2) | 12.(4) | 0.5(3) | 0.27 | 1.00 |
| 5500–5750 | 12.5 | 0.6922 | 0.0883 | 0.1521 ± 0.0006 | 1.008(6) | 0.016(7) | 0.000(9) | 13.(2) | 0.7(1) | 0.46 | 1.00 |
| 5750–6000 | 12.5 | 0.6579 | 0.1049 | 0.1527 ± 0.0003 | 1.008(6) | 0.016(7) | 0.000(9) | 12.(9) | 0.5(3) | 0.26 | 1.00 |
| 6000–6100 | 5.0 | 0.6337 | 0.1143 | 0.1529 ± 0.0004 | 1.008(6) | 0.016(7) | 0.001(0) | 13.(0) | 0.5(0) | 0.42 | 1.15 |
| 6100–6250 | 7.5 | 0.6106 | 0.1203 | 0.1533 ± 0.0005 | 1.008(6) | 0.016(7) | 0.001(1) | 12.(0) | 0.3(6) | 0.38 | 1.04 |
| 6250–6385 | 6.7 | 0.6013 | 0.1228 | 0.1522 ± 0.0004 | 1.008(6) | 0.016(7) | 0.001(0) | 13.(1) | 0.8(7) | 0.29 | 1.30 |
| 6385–6500 | 5.7 | 0.5862 | 0.1262 | 0.1519 ± 0.0004 | 1.008(6) | 0.016(7) | 0.001(0) | 13.(1) | 0.8(7) | 0.46 | 1.15 |
| 6500–6670 | 8.5 | 0.5582 | 0.1441 | 0.1526 ± 0.0003 | 1.008(6) | 0.016(7) | 0.001(0) | 13.(4) | 0.6(4) | 0.25 | 1.00 |
| 6670–6800 | 6.5 | 0.5527 | 0.1399 | 0.1519 ± 0.0005 | 1.008(6) | 0.016(7) | 0.000(9) | 12.(9) | 0.5(3) | 0.38 | 1.00 |
| 6800–6930 | 6.5 | 0.5408 | 0.1437 | 0.1525 ± 0.0006 | 1.008(6) | 0.016(7) | 0.000(9) | 11.(9) | 0.9(1) | 0.32 | 1.48 |
| 6930–7000 | 3.5 | 0.5349 | 0.1439 | 0.1514 ± 0.0003 | 1.008(6) | 0.016(7) | 0.000(9) | 13.(0) | 0.9(0) | 0.36 | 1.00 |
| 7000–7080 | 4.0 | 0.5238 | 0.1448 | 0.1514 ± 0.0004 | 1.008(6) | 0.016(7) | 0.000(9) | 12.(9) | 0.5(7) | 0.36 | 1.00 |
Notes. From left to right; WC corresponds to the wavelength channel (in nm), indicating the beginning and end of the wavelength band; CW corresponds to the channel width in nm; u1, and u2 show the custom limb-darkening coefficients; RP/RS the best-fit transit depth along with their derived 1σ errors; a0, a1, A1, ν1 and φ1 correspond to the detrending coefficients as specified in Eq. (6); SDR corresponds to the standard deviation of the residual light curve in ppt; and βN accounts for correlated noise in the light curves. For the detrending parameters we specify their precision by adding a parenthesis in their last significant decimal.
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