The Source Finding Application, SoFiA, is a new, fully automated source finding and parameterisation pipeline for 3-D extragalactic HI data cubes developed as part of the activities of WALLABY’s technical working group 4 (“Source finding and cataloguing”) led by Tobias Westmeier. SoFiA combines a large number of sophisticated algorithms, allowing users to choose an optimal set of parameters for their specific data cube. In addition to the command-line tool, SoFiA also comes with a modern graphical user interface (GUI) that allows users to interactively change the pipeline settings, run the pipeline from within the GUI, and inspect the resulting output catalogues and images. SoFiA will continue to be developed and improved by our team and has been made available to the community via GitHub.
- SoFiA and SoFiA 2 on GitHub
- SoFiA wiki and SoFiA 2 wiki with tutorials and documentation
- SoFiA overview paper: Serra, P., Westmeier, T., Giese, N., et al., 2015, MNRAS, 448, 1922 (ADS | arXiv)
The 2-D Bayesian Automated Tilted-ring fitter, 2DBAT, has been developed by Se-Heon Oh and the WALLABY Kinematics working group for the purpose of fitting tilted rings to the 2-D velocity field of spatially resolved galaxies detected by the WALLABY survey and extract their rotation curves. By using a new Bayesian-based algorithm instead of the standard χ2 minimisation, the fitting procedure is more robust and can be fully automated, which is crucial for fitting the large number of extended galaxies expected to be detected by WALLABY. 2DBAT works best for well-resolved galaxies with intermediate inclinations in the range of 20° < i < 70°, complementing 3-D techniques better suited to modelling highly inclined galaxies. 2DBAT has been made available to the community via GitHub.
- 2DBAT on GitHub
- 2DBAT overview paper: Oh, S.-H., Staveley-Smith, L., Spekkens, K., et al., 2018, MNRAS, 473, 3256 (ADS | arXiv)
Fully Automated TiRiFiC, FAT, is a wrapper around the Tilted Ring Fitting Code (TiRiFiC) which aims to fully automate the process of fitting simple tilted ring models to spectral line emission cubes of resolved galaxies. Developed by Peter Kamphuis and the WALLABY Kinematics working group, FAT fits simple rotationally symmetric discs with asymmetric warps and surface brightness distributions in order to extract the rotation curve of the galaxy. FAT accurately models the kinematics and morphology of galaxies with an size of eight beams across the major axis and in the inclination range of 20° < i < 90° without the need for priors. This will allow the large number of well-resolved galaxies that WALLABY will detect to be fitted in an automated fashion. FAT has been made available to the community via GitHub.
- FAT on GitHub
- FAT overview paper: Kamphuis, P., Józsa, G. I. G., Oh, S.-H., et al., 2015, MNRAS, 452, 3139 (ADS | arXiv)
In addition to the software tools developed by the WALLABY team, the following external software packages and computing projects are of relevance to WALLABY.