Evidence of apsidal motion and a possible co-moving companion star detected in the WASP-19 system

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Table C.2

Occultations found in the literature.

Cycle number	T_mid [days]	Uncertainty [days]	Observations	Reference
N	BJD_TDB - 2 450 000
2	4777.313572		HAWK-I (VLT)	Anderson et al. (2010)
185	4921.66849	0.00190	HAWK-I (VLT)	Gibson et al. (2010)
1018	5578.7684	0.0039	ULTRACAM on NTT	Burton et al. (2012)
1199	5721.5508		DFOSC on 1.54m - Danish Telescope	Mancini et al. (2013)
1269	5776.77020	0.00083	IRAC on Spitzer	Wong et al. (2016)
1270	5777.55733	0.00092	IRAC on Spitzer	Wong et al. (2016)
1282	5787.02383	0.00077	IRAC on Spitzer	Wong et al. (2016)
1283	5787.81228	0.00076	IRAC on Spitzer	Wong et al. (2016)
1549	5997.6440	0.001	MMIRS on Magellan II telescope	Bean et al. (2013)
1582	6023.6763	0.001	MMIRS on Magellan II telescope	Bean et al. (2013)

Notes. The cycle number is referred to the previous transit (half phase before the occultation). Light travel time across the system (around 16.3 s) is subtracted from all mid-occultation times.

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