ASCL Code Record
[ascl:1502.007]
PyBDSF: Python Blob Detection and Source Finder
PyBDSF (Python Blob Detector and Source Finder, formerly PyBDSM) decomposes radio interferometry images into sources and makes their properties available for further use. PyBDSF can decompose an image into a set of Gaussians, shapelets, or wavelets as well as calculate spectral indices and polarization properties of sources and measure the psf variation across an image. PyBDSF uses an interactive environment based on CASA (ascl:1107.013); PyBDSF may also be used in Python scripts.
- Code site:
- https://github.com/lofar-astron/PyBDSF
- Used in:
- https://ui.adsabs.harvard.edu/abs/2012A%26A...543A..43V https://ui.adsabs.harvard.edu/abs/2013A%26A...549A..55W https://ui.adsabs.harvard.edu/abs/2013A%26A...558A..72I https://ui.adsabs.harvard.edu/abs/2014MNRAS.442.2867W https://ui.adsabs.harvard.edu/abs/2014ApJ...793...82V
- Bibcode:
- 2015ascl.soft02007M
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