We have developed a new method that uses wavelet analysis to remove
interference fringe patterns from images. This method is particularly useful
for flat fields in the common case where fringes vary between the calibration
and object data. We analyze the efficacy of this method by creating fake flats
with fictitious fringes and removing the fringes. We find that the method
removes 90% of the fringe pattern if its amplitude is equal to the random noise
level and 60% if the fringe amplitude is ≈1/10 of the noise level. We
also present examples using real flat field frames. A routine written in the
Interactive Data Language (IDL) that implements this algorithm is available
from the authors and as an attachment to this paper.Comment: 7 pages, 14 figures. Accepted to the Astrophysical Journal. (The
quality of the figures in this preprint has been downgraded in order to
fulfill arXiv requirements. Check journal for the high-quality figures