Pipe3D，分析积分场spectroscopy数据的管道：II。分析序列和CALIFA数据产品
Pipe3D, a pipeline to analyse integral field spectroscopy data: II. Analysis sequence and CALIFA dataproducts
摘要：
介绍了一个基于FIT 3D拟合工具的Pipe 3D分析管道，用于研究积分场光谱数据的恒星星族和电离气体的性质。创建Pipe 3D是为了提供连贯、易于分发和可比的数据产品，而与数据来源无关，侧重于最新IFU调查的数据（例如，CALIFA、MaNGA和SAMI）和上一代IFS仪器（例如，MUSE）。沿着这篇文章，我们描述了数据分析中涉及的不同步骤，通过显示由CALIFA和P-MaNGA观测到的NGC 2916的数据产品来说明它们。作为管道的实际使用，我们提出了一套完整的dataproducts派生的200 datacubes，包括V500设置的CALIFA数据发布2（DR 2），使他们免费提供通过网络（ftp：//ftp.caha.es/CALIFA/dataproducts/DR2/Pipe3D）。最后，我们探讨了星系有效半径处的恒星星族和电离气体的性质代表星系总体平均性质的假设，发现情况确实如此。
英文摘要：
We present Pipe3D, an analysis pipeline based on the FIT3D fitting tool, devel- oped to explore the properties of the stellar populations and ionized gas of Integral Field Spectroscopy data. Pipe3D was created to provide with coherent, simple to distribute, and comparable dataproducts, independently of the origin of the data, focused on the data of the most recent IFU surveys (e.g., CALIFA, MaNGA, and SAMI), and the last generation IFS instruments (e.g., MUSE). Along this article we describe the different steps involved in the analysis of the data, illustrating them by showing the dataproducts derived for NGC 2916, observed by CALIFA and P-MaNGA. As a practical use of the pipeline we present the complete set of dataproducts derived for the 200 datacubes that comprises the V500 setup of the CALIFA Data Release 2 (DR2), making them freely available through the network (ftp://ftp.caha.es/CALIFA/dataproducts/DR2/Pipe3D). Finally, we explore the hypothesis that the properties of the stellar populations and ionized gas of galaxies at the effective radius are representative of the overall average ones, finding that this is indeed the case.
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。
