Digitization of Astronomical Photographic Plates from China: Photometric Calibration of Single-exposure Plates and Release of Photometric Catalogs

Digitization of Astronomical Photographic Plates from China: Photometric Calibration of Single-exposure Plates and Release of Photometric Catalogs

The Chinese Plate-Digitizing Project has digitized a total number of about 30,000 astronomical plates from 11 telescopes of five observatories (Shanghai Astronomical Observatory (SHAO), Astronomical Observatory of the Chinese Academy of Sciences (NAOC), Purple Mountain Observatory (PMO), Yunnan Astr...

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Main Authors: Mingyang Ma, Haibo Yuan, Kai Xiao, Bowen Huang, Tao Wang, Yang Huang, Shiyin Shen, Zhengjun Shang, Yong Yu, Liangliang Wang, Meiting Yang, Jing Yang, Min Liu, Quanfeng Xu, Chenzhou Cui, Dongwei Fan, Zhenghong Tang, Jianhai Zhao
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Supplement Series
Subjects:
Astronomy data analysis
Stellar photometry
Calibration
Variable stars
Online Access:https://doi.org/10.3847/1538-4365/adec7e
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Summary:The Chinese Plate-Digitizing Project has digitized a total number of about 30,000 astronomical plates from 11 telescopes of five observatories (Shanghai Astronomical Observatory (SHAO), Astronomical Observatory of the Chinese Academy of Sciences (NAOC), Purple Mountain Observatory (PMO), Yunnan Astronomical Observatory (YNAO), and Qingdao Observatory (QDO)) in China, spanning nearly 100 yr of observations. In this work, we present a photometric calibration method to calibrate about 15,000 single-exposure plates to the JKC photometric system. Using standard stars constructed from the BEST database, we have identified and corrected various systematic effects (including the magnitude term, color term, and flat-field term) to a high precision. The final photometric precision is typically 0.15, 0.23, 0.17, 0.11, 0.19 mag for plates collected in SHAO, NAOC, PMO, YNAO, and QDO, respectively, with best cases reaching 0.07, 0.08, 0.06, 0.05, and 0.11 mag, respectively. Candidates of variable sources are also identified. The catalogs are publicly available at the China National Astronomical Data Center. Such a data set will provide a valuable resource for conducting long-term, temporal-scale astronomical research. Our calibration method can also be applied to other digitized astronomical plates in general.
ISSN:0067-0049

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