• A method to deconvolve stellar profiles The non-rotating line utilizing Gaussian sum approximation 

      Escárate, P.; Curé, M.; Araya, I. [Univ Mayor, Ctr Opt & Informac Cuant, Vicerrectoria Invest, Chile]; Coronel, M.; Cedeño, AL.; Celedón, L.; Cavieres, J.; Agüero, JC.; Arcos, C; Cidale, LS.; Levenhagen, RS.; Pezoa, R.; Simón-Díaz, S. (EDP SCIENCES S A, 2023-08-04)
      Context. Currently, one of the standard procedures used to determine stellar and wind parameters of massive stars involves to comparing the observed spectral lines with a grid of synthetic lines. These synthetic lines are ...


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