Limb-darkening coefficients for four-term and power-2 laws for the JWST mission adopting spherical PHOENIX models at high resolution - NIRCam, NIRISS, and NIRSpec passbands

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Fig. 1

Angular distribution of the specific intensity for a model with T_eff = 5800 K, log g = 4.5, [M/H] = 0.0, and ξ = 1.0 km s^-1 (blue line), for the NIRISS SOSS Order 2 passband. The fits provided by the four-term and power-2 laws are displayed for comparison. The inset shows an enlargement around the drop-off region.

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