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ASCL Code Record

[ascl:2103.003] spalipy: Detection-based astronomical image registration

spalipy performs detection-based astronomical image registration in Python. A source image is transformed to the pixel-coordinate system of a template image using their respective detections as tie-points by finding matching quads of detections. spalipy also includes an optional additional warping of the initial affine transformation via splines to achieve accurate registration in the case of non-homogeneous coordinate transforms. This is particularly useful in the case of optically distorted or wide field-of-view images.

Code site:
https://github.com/Lyalpha/spalipy
Used in:
https://ui.adsabs.harvard.edu/abs/2020MNRAS.495..992L
Bibcode:
2021ascl.soft03003L

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ascl:2103.003
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