Abstract
Upcoming H I surveys will deliver large datasets, and automated
processing using the full 3-D information (two positional dimensions and
one spectral dimension) to find and characterize H I objects is
imperative. In this context, visualization is an essential tool for
enabling qualitative and quantitative human control on an automated
source finding and analysis pipeline. We discuss how Visual Analytics,
the combination of automated data processing and human reasoning,
creativity and intuition, supported by interactive visualization,
enables flexible and fast interaction with the 3-D data, helping the
astronomer to deal with the analysis of complex sources. 3-D
visualization, coupled to modeling, provides additional capabilities
helping the discovery and analysis of subtle structures in the 3-D
domain. The requirements for a fully interactive visualization tool are:
coupled 1-D/2-D/3-D visualization, quantitative and comparative
capabilities, combined with supervised semi-automated analysis.
Moreover, the source code must have the following characteristics for
enabling collaborative work: open, modular, well documented, and well
maintained. We review four state of-the-art, 3-D visualization packages
assessing their capabilities and feasibility for use in the case of 3-D
astronomical data.
Original language | English |
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Article number | 1505.06976 |
Pages (from-to) | 86-99 |
Number of pages | 15 |
Journal | Astronomy and Computing |
Volume | 12 |
DOIs | |
Publication status | Published - Sept-2015 |
Keywords
- Radio lines: galaxies
- Galaxies: kinematics and dynamics
- Surveys
- Scientific visualization
- Visual analytics
- DIMENSIONAL DATA VISUALIZATION
- HIGH-VELOCITY CLOUDS
- SPECTRAL-LINE DATA
- ASTRONOMICAL DATA
- SOURCE-FINDER
- SCIENTIFIC VISUALIZATION
- NEUTRAL HYDROGEN
- DISK GALAXIES
- ASKAP
- ARRAY