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[ascl:1401.006] convolve_image.pro: Common-Resolution Convolution Kernels for Space- and Ground-Based Telescopes

The IDL package convolve_image.pro transforms images between different instrumental point spread functions (PSFs). It can load an image file and corresponding kernel and return the convolved image, thus preserving the colors of the astronomical sources. Convolution kernels are available for images from Spitzer (IRAC MIPS), Herschel (PACS SPIRE), GALEX (FUV NUV), WISE (W1 - W4), Optical PSFs (multi- Gaussian and Moffat functions), and Gaussian PSFs; they allow the study of the Spectral Energy Distribution (SED) of extended objects and preserve the characteristic SED in each pixel.

Code site:
https://www.astro.princeton.edu/~ganiano/Kernels.html
Described in:
http://adsabs.harvard.edu/abs/2011PASP..123.1218A
Bibcode:
2014ascl.soft01006A

Views: 1612

ascl:1401.006
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