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[ascl:1805.026] PySE: Python Source Extractor for radio astronomical images

PySE finds and measures sources in radio telescope images. It is run with several options, such as the detection threshold (a multiple of the local noise), grid size, and the forced clean beam fit, followed by a list of input image files in standard FITS or CASA format. From these, PySe provides a list of found sources; information such as the calculated background image, source list in different formats (e.g. text, region files importable in DS9), and other data may be saved. PySe can be integrated into a pipeline; it was originally written as part of the LOFAR Transient Detection Pipeline (TraP, ascl:1412.011).

Code site:
https://github.com/transientskp/pyse
Appears in:
https://ui.adsabs.harvard.edu/#abs/2018A%26C....23...92C https://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.4011B
Bibcode:
2018ascl.soft05026S

Views: 585

ascl:1805.026
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