LSSGalPy: Interactive Visualization of the Large-scale Environment Around Galaxies

被引:6
|
作者
Argudo-Fernandez, M. [1 ]
Duarte Puertas, S. [2 ]
Ruiz, J. E. [2 ]
Sabater, J. [3 ]
Verley, S. [4 ,5 ]
Bergond, G. [6 ]
机构
[1] Univ Antofagasta, Unidad Astron, Fac Cs Basicas, Av U Antofagasta, Antofagasta 02800, Chile
[2] CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, E-18008 Granada, Spain
[3] Univ Edinburgh, Inst Astron, Edinburgh EH9 3HJ, Midlothian, Scotland
[4] Univ Granada, Dept Fis Teor & Cosmos, E-18071 Granada, Spain
[5] Univ Granada, Inst Univ Carlos I Fis Teor & Computac, E-18071 Granada, Spain
[6] Ctr Astron Hispano Aleman, Compl Observ Calar Alto S-N, Sierra De Los Filabres 04550, Gergal, Spain
关键词
methods: data analysis; methods: miscellaneous; methods: observational; methods: statistical surveys; galaxies: general; galaxies: statistics;
D O I
10.1088/1538-3873/aa5785
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
New tools are needed to handle the growth of data in astrophysics delivered by recent and upcoming surveys. We aim to build open-source, light, flexible, and interactive software designed to visualize extensive three-dimensional (3D) tabular data. Entirely written in the Python language, we have developed interactive tools to browse and visualize the positions of galaxies in the universe and their positions with respect to its large-scale structures (LSS). Motivated by a previous study, we created two codes using Mollweide projection and wedge diagram visualizations, where survey galaxies can be overplotted on the LSS of the universe. These are interactive representations where the visualizations can be controlled by widgets. We have released these open-source codes that have been designed to be easily re-used and customized by the scientific community to fulfill their needs. The codes are adaptable to other kinds of 3D tabular data and are robust enough to handle several millions of objects.
引用
收藏
页数:5
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