论文标题
Sedbys：一个基于Python的SED Builder，用于年轻星星
SEDBYS: A python-based SED Builder for Young Stars
论文作者
论文摘要
光谱能分布（SED）在分析年轻恒星的观察结果中是有用的主要和互补工具。然而，整理，检查和转换档案光度法和光谱的过程以建立年轻恒星的光谱能量分布可能很耗时。在这里，我介绍了Sedbys（年轻恒星的光谱能量分配构建器），这是一个基于Python的命令行工具的存储库，该存储库构建了（i）在线查询在线光度和光谱目录以及档案光度计的分布式数据库，（II）使用零点的零点来查找零点，以供您使用的零点（III）（III）（III III）（III III）（III III）。 Bibtex格式的参考。该代码是通过GIT分发的，并配备了其他工具，使用户可以将现有或即将到来的目录添加到查询的来源列表中，从而确保Sedbys的寿命为Star Formation社区的工具。
Spectral energy distributions (SEDs) are useful primary and complementary tools in the analysis of observations of young stars. However, the process of collating, inspecting, and flux-converting archival photometry and spectroscopy to build spectral energy distributions for young stars can be time-consuming. Here, I present SEDBYS (Spectral Energy Distribution Builder for Young Stars), a python-based repository of command-line tools built to (i) query online photometric and spectroscopic catalogs and a distributed database of archival photometry, (ii) use a look-up table of zero points to flux-convert the acquired data, (iii) enable visual inspection of the SED and (iv) handle book-keeping to collate references in bibTeX format. The code is distributed via git and is equipped with additional tools to enable users to add existing or forthcoming catalogs to the list of sources queried, ensuring the longevity of SEDBYS as a tool for the star formation community.
