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New grids of  atlas 9 models have been calculated using revised convection parameters and updated opacity‐distribution functions (ODFs), for chemical compositions intended to be representative of solar, [M/H] =+0.3, +0.5, Large Magellanic Cloud and Small Magellanic Cloud abundances. The grids cover   T  eff = 3.5–50  kK, from  log  g = 5.0  to the effective Eddington limit. Limb‐darkening coefficients and synthetic photometry are presented in the  UBVRIJHKLM ,  uvby ,  ugriz , WFCAM,  Hipparcos /Tycho and  Kepler  passbands for these models and for Castelli’s comparable ‘new‐ODF’ grids. Flux distributions are given for the new models. The sensitivity of limb‐darkening coefficients to the adopted physics is illustrated.

New limb‐darkening coefficients and synthetic photometry for model‐atmosphere grids at Galactic, LMC and SMC abundances