Iris：一个用于建立和分析光谱能量分布的可扩展应用程序
Iris: an Extensible Application for Building and Analyzing Spectral Energy Distributions
摘要：
Iris是一个可扩展的应用程序，为天文学家提供了一个用户友好的界面，能够从许多不同的来源获取宽带数据，以建立，探索和建模光谱能量分布（SED）。Iris利用了国际虚拟天文台联盟定义的标准，但通过在这些标准之上实现不同的抽象层来隐藏这些标准的技术细节。这些中间层提供了用户和开发人员可以利用的钩子，以便扩展Iris提供的功能。例如，自定义Python模型可以以任意方式与Iris内置模型或其他自定义函数组合。因此，Iris提供了一个平台，用于开发和集成来自用户系统或Web的SED数据、服务和应用程序。在本文中，我们描述了Iris提供的用于构建和分析SED的内置功能。我们还详细探讨了Iris框架和软件开发工具包，展示了天文学家和软件开发人员如何将其代码插入集成的SED分析环境。
英文摘要：
Iris is an extensible application that provides astronomers with a user-friendly interface capable of ingesting broad-band data from many different sources in order to build, explore, and model spectral energy distributions (SEDs). Iris takes advantage of the standards defined by the International Virtual Observatory Alliance, but hides the technicalities of such standards by implementing different layers of abstraction on top of them. Such intermediate layers provide hooks that users and developers can exploit in order to extend the capabilities provided by Iris. For instance, custom Python models can be combined in arbitrary ways with the Iris built-in models or with other custom functions. As such, Iris offers a platform for the development and integration of SED data, services, and applications, either from the user's system or from the web. In this paper we describe the built-in features provided by Iris for building and analyzing SEDs. We also explore in some detail the Iris framework and software development kit, showing how astronomers and software developers can plug their code into an integrated SED analysis environment.
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