This paper introduces the Variational Conditional Scattering-Flow (VCSF) framework to detect simulation mismatch in weak-lensing convergence maps by casting it as an out-of-distribution (OoD) detection problem (Sec. 1–2). Each map is encoded via a Wavelet Scattering Transform (WST) into 417 non-Gaussian coefficients, compressed with PCA to 3 dimensions (>97% variance explained), and then “whitened” using an intra-cosmology covariance intended to reduce sensitivity to baryonic nuisance parameters (Sec. 2.2, Sec. 3.1). A conditional Neural Spline Flow (NSF) models the density p(z|θ) of the resulting 3D features conditioned on five physical parameters (Ω_m, S_8, T_AGN, f_0, Δz), and an anomaly score is defined by profiling over parameters via gradient-based minimization of NLL, initialized by an MLP regressor (Sec. 2.3). Experiments on the NeurIPS 2025 FAIR Universe challenge data evaluate OoD detection using Gaussian-blurred maps (σ=1.5 pixels) as a proxy mismatch, reporting ROC AUC 0.925 and pAUC 0.1488 over FPR∈[0.001,0.05] with visually clear InD/OoD score separation (Sec. 3.3), plus suggestive robustness to extreme AGN settings (Sec. 3.4). The pipeline is conceptually coherent and promising, but key components are under-specified (especially whitening and θ-optimization), the OoD evaluation is narrow (single blur proxy within one simulation suite, with potential leakage concerns), and baseline comparisons/metrics are not yet presented in a fully quantitative and reproducible way—making some broader claims in Sec. 1 and Sec. 4 premature without additional validation.