1941 20220914135156.0 10.1023/A:1023262813348 DOI ASTROimport-98 Dupret, M.-A. 2003 An Improved Method of Photometric Mode Identification: Applications to Slowly Pulsating B, ß Cephei, δ Scuti and γ Doradus Stars We present an improved version of the method of photometric mode identification based upon the inclusion of non-adiabatic eigenfunctions determined in the stellar atmosphere, according to the formalism recently proposed by Dupret et al. (2002). We apply our method to ß Cephei, Slowly Pulsating B, δ Scuti and γ Doradus stars. Besides identifying the degree l of the pulsating stars, our method is also a tool for improving the knowledge of stellar interiors and atmospheres, by imposing constraints on the metallicity for ß Cephei and SPBs, the characteristics of the superficial convection zone for δ Scuti and γ Doradus stars and the limb-darkening law. Scuflaire, R. Noels, A. Thoul, A. Garrido, R. Moya, A. De Ridder, J. De Cat, P. Aerts, C. Astrophysics and Space Science 284 1 2003 129-132 http://esoads.eso.org/abs/2003Ap%26SS.284..129D published in REFERD