ViaLactea Visual Analytics @ NEANIAS

The ViaLactea Service is aimed at exploiting astrophysical surveys of the Galactic Plane to study the star formation process of the Milky Way. The ViaLactea Visual Analytic (VLVA) tool combines different types of visualization to perform the analysis exploring the correlation between different data, for example 2D intensity images with 3D molecular spectral cubes. All underlying data are managed in the ViaLactea Knowledge Base (VLKB). The VLKB includes 2D and 3D (velocity cubes) surveys, numerical model outputs, point-like and diffuse object catalogues and allows for retrival of all the avaiable datasets as well as cutouts on the positional and/or velocity axis and some merging capabilities on adjacent datasets. The project aims at extending the VLVA tool to access cloud services of NEANIAS to access the data services of the ViaLactea Knowledge Base.

Employed Technologies: QT (https://www.qt.io/), C++, Visualization ToolKit (https://vtk.org/)

 

Contacts: Eva Sciacca (eva.sciacca@inaf.it) and Fabio Vitello (fabio.vitello@inaf.it)

 

DURATION: 2 – 4 months

More information

F. Vitello et al., ViaLactea Visual Analytics Tool for Star Formation Studies of the Galactic Plane, Publications of the Astronomical Society of the Pacific 130.990 (2018): 084503. Available on: https://arxiv.org/pdf/1807.07723; Video tutorial on VLVA available on YouTube: https://youtu.be/gsrpejLF3g8.

About NEANIAS