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Table A.1

All the determined planetary transit parameters for the modelling process of the spectrophotmetric channels for the transit of WASP-19b.

Channela Rp/R⋆ Linear LD coefficient Quadratic LD coefficient
(nm) γ1 γ2
560 ± 10 0.1424 0.424 0.228
570 ± 10 0.1425 0.440 0.225
581 ± 11 0.1429 0.421 0.230
590 ± 10 0.1432 0.406 0.227
601 ± 9 0.1419 0.409 0.221
610 ± 10 0.1431 0.415 0.221
620 ± 10 0.1429 0.420 0.221
630 ± 10 0.1407 0.420 0.222
640.5 ± 10.5 0.1427 0.365 0.225
650 ± 10 0.1434 0.366 0.225
660.5 ± 9.5 0.1419 0.384 0.222
670 ± 10 0.1407 0.385 0.223
681.25 ± 11.2 0.1412 0.385 0.223
690 ± 10 0.1396 0.387 0.225
701.25 ± 8.75 0.1388 0.401 0.222
711.25 ± 11.25 0.1417 0.387 0.221
720 ± 10 0.1422 0.379 0.225
731.25 ± 8.75 0.1400 0.405 0.229
740 ± 10 0.1400 0.414 0.227
748 ± 8 0.1405 0.364 0.222
760 ± 10 0.1394 0.351 0.227
768 ± 12 0.1398 0.350 0.224
780 ± 10 0.1409 0.363 0.223
790 ± 10 0.1421 0.368 0.224
800 ± 10 0.1435 0.371 0.225
810 ± 10 0.1460 0.368 0.229
820 ± 10 0.1433 0.371 0.227

Notes. All other non-wavelength-dependent parameters are fixed to the broadband light curve model solution, values for which are given in Table 1.

(a)

The central wavelength and the width of some channels had to be adjusted slightly to avoid having integration limits that intersect with any telluric lines. Such an event could cause artificial trends in the light curve, due to uncertainties in the wavelength calibration.

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