Cumulative CMF of IRAS 19410+2336 for core masses above 1 M_⊙. The solid red line and the dashed blue line represent the best fits of Eq. (6) with a power-law index β = −2.2 ± 0.1 and Eq. (5) with β = −2.4 ± 0.1, respectively. The green crosses represent a slight increase of 10 K in the higher-mass end, and the green dash-dotted line is the corresponding new fit of Eq. (6) (see Sect. 5.1). We note the flattening of the “bump” in the distribution, while the slope of the fit remains practically unchanged. In all cases, we have normalized N(>M) by the total number of cores N_tot.