论文标题

pulsar_spectra:脉冲星密度目录和频谱拟合存储库

pulsar_spectra: A pulsar flux density catalogue and spectrum fitting repository

论文作者

Swainston, N. A., Lee, C. P., McSweeney, S. J., Bhat, N. D. R.

论文摘要

我们介绍了Pulsar_spectra软件存储库,这是一个开源的PULSAR通量密度目录和自动光谱拟合软件,可找到最佳的频谱模型并生成出版物质量的图。基于Python的软件包括使天文学社区的用户在可用时在目录中添加新发布的光谱测量值的功能。光谱拟合软件是Jankowski等人中描述的方法的实现。 (2018)使用强大的统计方法来决定单个脉冲光谱的最合适模型。 Pulsar_spectra的动机是需要用于脉冲星密度测量值的集中式存储库,以使已发表的测量更容易被天文学群落访问,并提供了一套用于测量光谱的工具。

We present the pulsar_spectra software repository, an open-source pulsar flux density catalogue and automated spectral fitting software that finds the best spectral model and produces publication-quality plots. The Python-based software includes features that enable users in the astronomical community to add newly published spectral measurements to the catalogue as they become available. The spectral fitting software is an implementation of the method described in Jankowski et al. (2018) which uses robust statistical methods to decide on the best-fitting model for individual pulsar spectra. pulsar_spectra is motivated by the need for a centralised repository for pulsar flux density measurements to make published measurements more accessible to the astronomical community and provide a suite of tools for measuring spectra.

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