SEDBYS：一个基于Python的SED年轻明星构建器
SEDBYS: A python-based SED Builder for Young Stars
摘要：
光谱能量分布（SED）是分析年轻恒星观测数据的主要和补充工具。然而，整理，检查和通量转换档案测光和光谱学的过程中建立光谱能量分布的年轻恒星可以是耗时的。在这里，我介绍SEDBYS（Spectral Energy Distribution Builder for Young Stars），一个基于Python的命令行工具库，用于（i）查询在线光度和光谱目录以及分布式档案光度数据库，（ii）使用零点查找表对获取的数据进行通量转换，（iii）实现SED的目视检查，以及（iv）处理簿记以整理bibTeX格式的参考文献。该代码通过git分发，并配备了额外的工具，使用户能够将现有或即将推出的目录添加到查询的源列表中，确保SEDBYS作为恒星形成社区的工具的寿命。
英文摘要：
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.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
