“…Various peak models have been proposed in the past (Trivedi, 1969;Baba, 1978;Wätzig and Westmeier, 1978;García-Toraño and Aceña, 1981;L'Hoir, 1984;Bortels and Collaers, 1987;Koskelo et al, 1996;García-Toraño, 1997, 2003Lozano et al, 2000;Pommé and Sibbens, 2008;Semkow et al, 2010) and in recent work an attempt was made to include more physics in spectrum deconvolution (Siiskonen and Pöllänen, 2011;Westmeier and Siemon, 2012;Pöllänen and Siiskonen, 2014) or to use an artificial neural network (Baeza et al, 2011). One of the most successful analytical models to represent the shape of a mono-energetic alpha peak is the convolution of an exponential low-energy tail with a Gaussian distribution, as suggested by L'Hoir (1984) and introduced by Bortels and Collaers (1987) where A is the peak area, u À μ is the distance to the peak position, s is the standard deviation of the Gaussian and τ is the tailing parameter.…”