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The goal of this Research Note is to provide the theoretical calculations of the limb-darkening coefficients and gravity-darkening coefficients (GDC) for the space mission  CHEOPS . We use two stellar atmosphere models:  ATLAS  (plane-parallel) and  PHOENIX  with spherical symmetry covering a wide range of effective temperatures, local gravities, and hydrogen/metal. These grids cover 19 metallicities ranging from 10 −5  up to 10 +1  solar abundances, 0 ≤ log  g  ≤ 6.0 and 2300 K ≤  T eff  ≤ 50,000 K. The specific intensity distribution was fitted using six approaches: linear, quadratic, square root, logarithmic, power-2, and a series with four terms. The calculations of the GDC were performed for both stellar atmosphere models adopting an improved formulation.

Limb and Gravity-darkening Coefficients for the Space Mission CHEOPS