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Table A.1

Radial velocities at times out of transit for MASCARA-3 using the SONG telescope.

Time (BJD) RV + 6 000 (m s−1)
2 458 223.357685 613.1
2 458 224.382018 183.3
2 458 225.434460 67.3
2 458 233.607846 704.9
2 458 234.418452 770.2
2 458 235.720058 234.6
2 458 236.641036 32.2
2 458 237.678446 153.1
2 458 238.692052 603.9
2 458 241.674223 −70.7
2 458 243.368995 265.3
2 458 245.410918 805.6
2 458 246.571993 240.1
2 458 247.398019 −31.2
2 458 248.368253 82.6
2 458 249.365280 470.8
2 458 250.368275 844.0
2 458 250.681785 837.2
2 458 251.366037 687.0
2 458 251.666389 485.7
2 458 252.366480 192.9
2 458 253.365122 120.4
2 458 254.365100 237.8
2 458 255.374490 605.4
2 458 256.384282 796.1
2 458 257.382395 330.0
2 458 259.383303 18.0
2 458 263.567251 154.9
2 458 265.589542 291.4
2 458 267.372280 829.5
2 458 268.609046 306.4
2 458 270.572919 5.0
2 458 274.379165 192.8
2 458 280.423224 17.1
2 458 283.600292 812.6
2 458 418.763646 161.4
2 458 426.556824 222.3
2 458 434.627715 639.1
2 458 439.611331 713.9
2 458 448.692687 285.5
2 458 449.708606 658.2
2 458 450.690659 709.9
2 458 453.742034 106.8
2 458 454.745732 493.1
2 458 586.621310 20.0
2 458 594.703421 710.9
2 458 598.446201 150.2
2 458 600.395783 819.7
2 458 602.394577 19.7
2 458 604.398027 462.9
2 458 606.403578 680.6
2 458 608.402462 − 36.2
2 458 610.402961 656.7
2 458 612.656473 323.0
2 458 614.640588 99.4
2 458 616.679269 892.4
2 458 621.434468 611.2
2 458 623.623973 586.7
2 458 625.668018 199.2
2 458 627.634024 974.2
2 458 629.638527 312.8
2 458 631.621685 345.4
2 458 633.654485 949.8
2 458 638.605001 913.8
2 458 643.571329 579.7

Notes. We list the barycentric time of mid-exposure and the RVs corrected for barycentric motion. All spectra were taken with the iodine cell as reference. Although the individual uncertainties have some dependence on the flux level (which is near 30 m sec−1 at the highest and 60 m sec−1 at the lowest flux level), the overall instrumental uncertainty (σRV) is estimated to be ~ 40 m sec−1. To account for the possibility of underestimating this error, we introduced an additional jitter term during the fitting procedure (see Table 4).

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