Towards optimal photometric calibration of digital astronomical plates with deep learning
Abstract
Photometric calibration of digitized photographic plates is commonly modeled with separable magnitude-, color-, and position-dependent terms, but this separability can break down when image quality varies across the field in a magnitude-dependent way, leaving coupled spatial systematics in the residuals. We introduce a deep-learning calibration framework, the Multi-Feature Fused Network (MFF-Net), which takes instrumental magnitude, color, and pixel coordinates as input and learns a single nonlinear correction that jointly captures their coupled dependencies. Tests on 1{,}200 digitized Chinese plates show that MFF-Net consistently outperforms the MYX25 method (Ma et al. 2025), improving the 5th--95th percentile precision from 0.11--0.26~mag to 0.08--0.18~mag and delivering an approximately factor-of-two gain for bright sources. The learned correction largely removes the magnitude--position coupling seen in post-calibration residual maps, enabling higher-precision plate photometry and more reliable use of large historical plate archives.
Cite
@article{arxiv.2608.01391,
title = {Towards optimal photometric calibration of digital astronomical plates with deep learning},
author = {Mingyang Ma and Haibo Yuan and Lin Yang and Kai Xiao and Bowen Huang and Shiyin Shen and Zhengjun Shang and Yong Yu and Meiting Yang and Zhenghong Tang and Jianhai Zhao},
journal= {arXiv preprint arXiv:2608.01391},
year = {2026}
}
Comments
This manuscript has been accepted by The Astrophysical Journal Supplement Series (ApJS)