fourier_corr

jwst.ami.bp_fix.fourier_corr(data, pxdq, fmas)

Compute and apply the bad pixel corrections based on Section 2.5 of Ireland 2013.

Parameters:

datanumpy array

Science data

pxdqnumpy array

Bad pixel mask

fmasnumpy array

FT of science data

Returns:

data_outnumpy array

Corrected science data

References

M. J. Ireland, Phase errors in diffraction-limited imaging: contrast limits for sparse aperture masking, Monthly Notices of the Royal Astronomical Society, Volume 433, Issue 2, 01 August 2013, Pages 1718–1728, https://doi.org/10.1093/mnras/stt859