Luo Wei, Xie Xiaoyao, Jiang Jiatao, Zhou Linyong, Hu Zhijun
School of Computer Science and Technology, Guizhou University, Huaxi Avenue, Huaxi District, Guiyang 550025, China.
Key Laboratory of Information and Computing Science of Guizhou Province, Guizhou Normal University, Baoshan North Road, Yunyan District, Guiyang 550001, China.
Sensors (Basel). 2025 Jun 26;25(13):3963. doi: 10.3390/s25133963.
To enhance pulsar candidate recognition performance and improve model generalization, this paper proposes the cross-feature hybrid associative prior network (CFHAPNet). CFHAPNet incorporates a novel architecture and strategies to integrate multi-class heterogeneous feature subimages from each candidate into multi-channel data processing. By implementing cross-attention mechanisms and other enhancements for multi-view feature interactions, the model significantly strengthens its ability to capture fine-grained image texture details and weak prior semantic information. Through comparative analysis of feature weight similarity between subimages and average fusion weights, CFHAPNet efficiently identifies and filters genuine pulsar signals from candidate images collected across astronomical observatories. Additionally, refinements to the original loss function enhance convergence, further improving recognition accuracy and stability. To validate CFHAPNet's efficacy, we compare its performance against several state-of-the-art methods on diverse datasets. The results demonstrate that under similar data scales, our approach achieves superior recognition performance. Notably, on the FAST dataset, the accuracy, recall, and F1-score reach 97.5%, 98.4%, and 98.0%, respectively. Ablation studies further reveal that the proposed enhancements improve overall recognition performance by approximately 5.6% compared to the original architecture, achieving an optimal balance between recognition precision and computational efficiency. These improvements make CFHAPNet a strong candidate for future large-scale pulsar surveys using new sensor systems.
为了提高脉冲星候选体识别性能并提升模型泛化能力,本文提出了交叉特征混合关联先验网络(CFHAPNet)。CFHAPNet采用了一种新颖的架构和策略,将每个候选体的多类异构特征子图像整合到多通道数据处理中。通过为多视图特征交互实现交叉注意力机制和其他增强措施,该模型显著增强了其捕捉细粒度图像纹理细节和弱先验语义信息的能力。通过对特征子图像之间的特征权重相似性与平均融合权重进行对比分析,CFHAPNet能够从跨天文台收集的候选图像中高效识别并滤除真正的脉冲星信号。此外,对原始损失函数的优化增强了收敛性,进一步提高了识别准确率和稳定性。为了验证CFHAPNet的有效性,我们在不同数据集上将其性能与几种先进方法进行了比较。结果表明,在相似的数据规模下,我们的方法实现了卓越的识别性能。值得注意的是,在FAST数据集上,准确率、召回率和F1分数分别达到了97.5%、98.4%和98.0%。消融研究进一步表明,与原始架构相比,所提出的增强措施使整体识别性能提高了约5.6%,在识别精度和计算效率之间实现了最佳平衡。这些改进使CFHAPNet成为未来使用新传感器系统进行大规模脉冲星巡天的有力候选者。