{ "name": "Radio Source Classification Tree", "description": "A decision tree for classifying radio sources based on physical diagnostics and multi-Gaussian fitting.", "version": "2.0-GaussianFit", "parameters": { "SNR": "Signal-to-Noise Ratio (Peak Flux / Error)", "DC_Maj_arcsec": "Major axis of detected component in arcseconds", "BMAJ_arcsec": "Beam major axis in arcseconds", "Dist_Peak_Core": "Euclidean distance between the brightest pixel and the geometric center (pixels)", "Diag_Radius": "Threshold for peak offset diagnosis (0.5 * Beam in pixels)", "Flux_Ratio": "Ratio of the brightest residual (after excising 2.0*Beam core) to the original peak flux", "Best_N": "The number of Gaussian components (1, 2, or 3) in the best-fit model selected by BIC" }, "decision_tree": [ { "step": 1, "condition": "SNR < 5.0", "description": "Signal Quality Check", "if_true": "Classification: 噪声 (Noise)", "if_false": "Go to step 2" }, { "step": 2, "condition": "DC_Maj_arcsec <= 1.5 * BMAJ_arcsec", "description": "Morphological Compactness Check", "if_true": "Classification: 致密源 (Compact)", "if_false": "Go to step 3" }, { "step": 3, "condition": "Dist_Peak_Core > Diag_Radius (0.5 * Beam)", "description": "Peak Location Diagnosis (Physical Center vs. Hotspot)", "if_true": "Go to step 4 (Branch A: Peak Outside / FR II Family)", "if_false": "Go to step 5 (Branch B: Peak Inside / FR I Family)" }, { "step": 4, "condition": "Best_N == 3", "description": "Branch A (FR II Family): Check Best_N from Fitting", "if_true": "Classification: FR II (Triple)", "if_false": "Classification: FR II (Double)" }, { "step": 5, "condition": "Flux_Ratio < 0.3", "description": "Branch B (FR I Family): Check core excision residual (Compactness)", "if_true": "Classification: FR I (Compact)", "if_false": "Go to step 6" }, { "step": 6, "condition": "Flux_Ratio > 0.5", "description": "Branch B (FR I Family): Check core excision residual (Structure Strength)", "if_true": "Go to step 7 (High Residual Structure)", "if_false": "Go to step 8 (Marginal Structure)" }, { "step": 7, "condition": "Best_N == 2", "description": "Branch B - High Residual: Check for Core-Jet morphology", "if_true": "Classification: FR I (Core-Jet)", "if_false": "Go to step 9" }, { "step": 8, "condition": "Best_N == 1", "description": "Branch B - Marginal Residual: Check for Resolution", "if_true": "Classification: FR I (Compact)", "if_false": "Classification: FR I (Resolved)" }, { "step": 9, "condition": "Best_N == 3", "description": "Branch B - High Residual: Check for Complex morphology", "if_true": "Classification: FR I (Complex)", "if_false": "Classification: FR I (Extended Blob)" } ], "classification_mapping": { "噪声 (Noise)": "信噪比不足,无法确认源结构", "致密源 (Compact)": "尺寸极小,未被波束分辨的点源", "FR II (Triple)": "边缘增亮,且模型识别出核心与双瓣共存 (N=3)", "FR II (Double)": "边缘增亮,核心不可见或极暗,仅识别出双瓣结构", "FR I (Core-Jet)": "核心主导,挖核后残留显著,模型拟合为双组件 (核心+喷流)", "FR I (Complex)": "核心主导,挖核后残留显著,模型拟合为三组件 (核心+晕/复杂结构)", "FR I (Resolved)": "核心主导,中等残留比,模型认为多组件拟合优于单组件 (边缘可分辨)", "FR I (Compact)": "核心主导,挖核后几乎无残留,或模型偏向单高斯 (本质致密)" }, "references": [ { "id": "ref1", "citation": "Fanaroff, B. L., & Riley, J. M. 1974, MNRAS, 167, 31P", "description": "Original definition of the Fanaroff-Riley (FR) classification, distinguishing FR I and FR II radio galaxies based on the relative position of high-brightness regions." }, { "id": "ref2", "citation": "Best, P. N., & Heckman, T. M. 2012, MNRAS, 421, 1569", "description": "Investigates the fundamental dichotomy in the radio-AGN population (HERG vs. LERG), linking radio source evolution to accretion modes and host galaxy properties." }, { "id": "ref3", "citation": "Hancock, P. J., Murphy, T., Gaensler, B. M., Hopkins, A., & Curran, J. R. 2012, MNRAS, 422, 1812", "description": "Introduces AEGEAN for radio surveys: uses a curvature map to detect component peaks and perform constrained multi-elliptical-Gaussian fitting of islands, improving characterization of blended/multi-component sources." }, { "id": "ref4", "citation": "Mingo, B., et al. 2019, MNRAS, 488, 2701", "description": "Revisits the Fanaroff-Riley dichotomy using the LOFAR Two-Metre Sky Survey (LoTSS), analyzing morphological parameters like the Concentration Index to classify complex sources." }] }