Dataset for "From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction"

This deposit contains the data related to the manuscript "From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction" submitted to the Astrophysical Journal. It includes the basic SDSS identifier, stellar mass, star formation rate, fractional formation time, and their errors. A detailed description can be found in Table 1 of the manuscript.

The data is stored in a CSV file. It can be read with standard data analysis packages like Pandas in Python. 

This deposit has also be updated to include a machine-readable table that follows the standards of the AAS Journals and Vizier (datafile1_ApJ57534.mrt). More information on this standard can be found in the AAS or CDS documentation. This format can be read in Python with packages like astropy.

本数据集存档包含与投稿至《天体物理学杂志》的论文《从晕到星系. X：利用物理先验与精确恒星形成历史重建解码星系光谱能量分布（Spectral Energy Distributions, SEDs）》相关的科研数据。其中包含基础的斯隆数字巡天（Sloan Digital Sky Survey, SDSS）标识符、恒星质量、恒星形成率、分数形成时间及其对应的误差值，详细说明可参见该论文的表1。
本数据以逗号分隔值（CSV）文件格式存储，可通过Python的Pandas等标准数据分析库读取。
本存档还已更新，新增了符合美国天文学协会（American Astronomical Society, AAS）期刊与Vizier天文数据服务标准的机器可读表格（datafile1_ApJ57534.mrt）。有关该标准的更多信息可参阅AAS或法国斯特拉斯堡天文数据中心（Centre de Données astronomiques de Strasbourg, CDS）的官方文档，该格式可通过Python的Astropy等库进行读取。