ViSL3D

Ixaka Labadie García
07/08/2024

ViSL3D is a Python package that creates X3D and HTML files to visualize datacubes from astrophysics in 3D in an interactive way. We use X3D and x3dom to represent figures in 3D and to integrate them into an HTML. The models have been made taking the x3d-pathway (Vogt et al. 2016) as a starting point. The current code was made for radio data, although it can be used with other types of 3D data.

Installation

pip install visl3d

How to use

Examples of how to use the package are provided in the Jupyter notebook jupyter_example.ipynb.

The produced HTML file can be visualised in any standard browser.

Prerequisites to visualise external X3D file (createX3D/createHTML)

1. Install a local HTTP Server. Visualisations produced by ViSL3D must be opened through a local server in order to be displayed. There are a few options:

   • Apache is a popular HTTP server that can be installed in most operating systems.
   • Python has a built-in HTTP server that can be used by running python -m http.server in the directory where the HTML and X3D files are located.
   • VS Code has a built-in HTTP server that can be used by installing the Live Preview extension.

2. Copy the x3dom folder into the server root directory. This should be the directory where the HTML and X3D files are located. By default, in Apache, it is /var/www/html in Linux, C:\Apache24\htdocs in Windows and /usr/local/var/www (or similar) in Mac. The DocumentRoot can be found and modified in the httpd.config file.

3. Move the created X3D and HTML files into the Apache DocumentRoot directory and open the visualisation in a browser (most common browsers are supported) by typing the URL localhost\example_file.html.

Features

• Plot any number of contour surfaces.
• Plot galaxies with labels.
• Add a 2D image in any wavelength in background.
• Change the scale of the velocity axis.
• Shift 2D image along velocity axis and display the value.
• Rotate, zoom and pan complete figure.
• Hide/Show different components of the figure.
• Change ax labels.
• Change viewpoints.
• Change the colormap
• Add markers

References

Vogt, Owen, Verdes-Montenegro & Borthakur, Advanced Data Visualization in Astrophysics: the X3D Pathway, ApJ 818, 115 (2016) (arxiv; ADS)