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This technical note describes the design and modular implementation of a one-dimensional convolutional neural network (1D CNN) adapted from residual networks (ResNet), developed for photometric regression tasks with an emphasis on low star formation rate surface density () inference. The model features residual block structures optimized for sparse targets, with optional loss weighting and diagnostic tools for analyzing residual behavior. The implementation (version ) originated during a collaborative project and is documented here independently. No external data are reproduced or analyzed. This note provides a reusable architectural reference for scalar regression problems in astronomy and related domains.

生成讲解博客的中文版本

生成AI智能校验的中文版本