Characterization of exoplanetary atmospheres through a model-unbiased spectral survey methodology

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Table 2

Ephemeris of each planet analyzed in this work.

Object	T_C	P	T₁₄	Reference
HD 209458b	2452826.6285 ± 0.000087	3.52474 ± 0.00000038	2.978 ± 0.051	Knutson et al. (2007) Richardson et al. (2006)
HD 189733b	2454279.436714 ± 0.000015	2.21857567 ± 0.00000015	0.07527 ± 0.00037	Agol et al. (2010) Triaud et al. (2009)
TrES-2b	2453957.63479 ± 0.00038	2.470621 ± 0.000017	0.07408 ± 0.0008	Turner et al. (2016)
WASP-74b	2456506.8918 ± 0.0002	2.13775 ± 0.000001	0.0955 ± 0.0008	Hellier et al. (2015)
HAT-P-2b	2454387.49375 ± 0.00074	5.6334729 ± 0.0000061	0.1787 ± 0.0013	Pál et al. (2010)

Notes. The references listed correspond to ephemeris and transit duration. If the former is lacking, then the reference of the ephemeris and the transit duration is the same. We used the same values of ephemeris for both datasets of HD 189733 b.

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