Summary of the no pooling analysis. Shown are the upper bounds (99.85th perc.) on the ejecta mass of ²²Na for each object with known (orange) and unknown (black) distance. The dependence on distance lets the bounds on mass appear along the lines of constant flux (dashed lines). Full posteriors are given for objects with the best flux bound (V5115 Sgr), the best mass bound (V5113 Sgr), and whenever the significance is higher than 2σ (V1535 Sco). Theoretical expectations (Starrfield et al. 2009) are indicated by the green bands for 1.25 and 1.35 M_⊙ ONe novae. Other theoretical expectations are bound to values below ≈ 10⁻⁸ M_⊙ (e.g., José & Hernanz 1998). See text for a discussion of individual objects.