The GAPS Programme at TNG - LXIX. The dayside of WASP-76 b revealed by GIANO-B, HARPS-N, and ESPRESSO: Evidence of 3D atmospheric effects

Open Access

Table A.2

S/N values measured at the expected planetary position (K_p = 196.52 km s⁻¹ and V_rest = 0 km s⁻¹) for each model in Fig. A.6.

Model	SN pre-eclipse	SN post-eclipse
1D pRT model	2.0	4.0
3D without dynamics	2.4	3.2
3D GCM	3.6	7.3

Notes. In all cases, the post-eclipse phase exhibits a higher S/N compared to the pre-eclipse phase.

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