Sengi: A small, fast, interactive viewer for spectral outputs from stellar population synthesis models

C. Lovell
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引用次数: 1

Abstract

We present Sengi ( this http URL, this https URL ), an online tool for viewing the spectral outputs of stellar population synthesis (SPS) codes. Typical SPS codes require significant disk space or computing resources to produce spectra for simple stellar populations with arbitrary parameters. This makes it difficult to present their results in an interactive, web-friendly format. Sengi uses Non-negative Matrix Factorisation (NMF) and bilinear interpolation to estimate output spectra for arbitrary values of stellar age and metallicity. The reduced disk requirements and computational expense allows the result to be served as a client-based Javascript application. In this paper we present the method for generating grids of spectra, fitting those grids with NMF, bilinear interpolation across the fitted coefficients, and finally provide estimates of the prediction and interpolation errors.
Sengi:一个小型、快速、交互式的查看器,用于从恒星族合成模型中输出光谱
我们提出了Sengi(这个http URL,这个https URL),一个在线工具,用于查看恒星族合成(SPS)代码的光谱输出。典型的SPS编码需要大量的磁盘空间或计算资源来生成具有任意参数的简单恒星群的光谱。这使得以交互式、网络友好的格式呈现结果变得困难。Sengi使用非负矩阵分解(NMF)和双线性插值来估计任意恒星年龄和金属丰度值的输出光谱。减少的磁盘需求和计算开销允许将结果作为基于客户机的Javascript应用程序提供。本文提出了生成光谱网格的方法,用NMF拟合这些网格,在拟合系数上进行双线性插值,最后给出了预测和插值误差的估计。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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