Introduction <p>A graph neural network (GNN)-based method is developed for track finding in gamma-ray reconstruction within the HERD Fiber Tracker.</p> Materials and methods <p>Using Monte Carlo simulations at 0.5, 1 and 10&#xa0;GeV gamma-ray, tracks are transformed into graph representations. Two edge labeling strategies are compared: The original labeling strategy treats all spatially connected edges from <InlineEquation ID="IEq1"> <EquationSource Format="TEX">\(e^+e^-\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msup> <mi>e</mi> <mo>+</mo> </msup> <msup> <mi>e</mi> <mo>-</mo> </msup> </mrow> </math></EquationSource> </InlineEquation> pair equally as signal, whereas the refined labeling strategy uses Monte Carlo information to reclassify non-physical edges intersecting between positron and electron trajectories as background, thereby suppressing “ghost edges” in pair production events. Systematic evaluation of four architectures—graph convolutional network, graph sample and aggregate (GraphSAGE), Multi-GraphSAGE and GraphSAGE with jumping knowledge (JK-GraphSAGE)—shows that JK-GraphSAGE has optimal edge classification performance by mitigating over-smoothing in deep networks through adaptive layer aggregation. Electron–positron pairs produced via photon conversion deposit tracks, which are reconstructed as distinct topological shapes. Topology aware linear fitting is applied to signal edges found by the GNN to reconstruct track endpoints. Although refined labels marginally reduce edge classification capability due to increased class imbalance, they enhance angular resolution by suppressing ghost edge influence.</p> Results <p>Under quality-filtered selection, the JK-GraphSAGE model achieves <InlineEquation ID="IEq2"> <EquationSource Format="TEX">\(\theta _{68}=0.10^{\circ }\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msub> <mi>θ</mi> <mn>68</mn> </msub> <mo>=</mo> <mn>0</mn> <mo>.</mo> <msup> <mn>10</mn> <mo>∘</mo> </msup> </mrow> </math></EquationSource> </InlineEquation> at 10&#xa0;GeV with a reconstruction efficiency of 97.8%.</p> Conclusion <p>These results validate the feasibility of GNN-based track finding, establishing a robust foundation for future end-to-end reconstruction frameworks that integrate track finding, fitting within unified deep learning architectures.</p>

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Gev gamma-ray track reconstruction with graph neural networks for a pair-conversion space telescope

  • Jian-yi Sun,
  • Jun-jing Wang,
  • Yong-wei Dong,
  • Chuan-li Liao,
  • Zheng Quan,
  • Xiao-fan Tang,
  • Ming Xu

摘要

Introduction

A graph neural network (GNN)-based method is developed for track finding in gamma-ray reconstruction within the HERD Fiber Tracker.

Materials and methods

Using Monte Carlo simulations at 0.5, 1 and 10 GeV gamma-ray, tracks are transformed into graph representations. Two edge labeling strategies are compared: The original labeling strategy treats all spatially connected edges from \(e^+e^-\) e + e - pair equally as signal, whereas the refined labeling strategy uses Monte Carlo information to reclassify non-physical edges intersecting between positron and electron trajectories as background, thereby suppressing “ghost edges” in pair production events. Systematic evaluation of four architectures—graph convolutional network, graph sample and aggregate (GraphSAGE), Multi-GraphSAGE and GraphSAGE with jumping knowledge (JK-GraphSAGE)—shows that JK-GraphSAGE has optimal edge classification performance by mitigating over-smoothing in deep networks through adaptive layer aggregation. Electron–positron pairs produced via photon conversion deposit tracks, which are reconstructed as distinct topological shapes. Topology aware linear fitting is applied to signal edges found by the GNN to reconstruct track endpoints. Although refined labels marginally reduce edge classification capability due to increased class imbalance, they enhance angular resolution by suppressing ghost edge influence.

Results

Under quality-filtered selection, the JK-GraphSAGE model achieves \(\theta _{68}=0.10^{\circ }\) θ 68 = 0 . 10 at 10 GeV with a reconstruction efficiency of 97.8%.

Conclusion

These results validate the feasibility of GNN-based track finding, establishing a robust foundation for future end-to-end reconstruction frameworks that integrate track finding, fitting within unified deep learning architectures.