FTbg: Background removal using Fourier Transform

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Ada Coda
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FTbg: Background removal using Fourier Transform

Post by Ada Coda » Wed Nov 29, 2017 6:33 pm

FTbg: Background removal using Fourier Transform

Abstract: FTbg performs Fourier transforms on FITS images and separates low- and high-spatial frequency components by a user-specified cut. Both components are then inverse Fourier transformed back to image domain. FTbg can remove large-scale background/foreground emission in many astrophysical applications. FTbg has been designed to identify and remove Galactic background emission in Herschel/Hi-GAL continuum images, but it is applicable to any other (e.g., Planck) images when background/foreground emission is a concern.

Credit: Wang, Ke

Site: https://github.com/esoPanda/FTbg

Bibcode: 2017ascl.soft11003W

Preferred citation method: https://ui.adsabs.harvard.edu/abs/2015MNRAS.450.4043W

ID: ascl:1711.003
Last edited by Ada Coda on Sun Sep 05, 2021 1:28 am, edited 1 time in total.
Reason: Updated code entry.

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