Please use this identifier to cite or link to this item: https://scholarbank.nus.edu.sg/handle/10635/104621
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dc.titleRestoring chopped and nodded images by tight frames
dc.contributor.authorChan, R.
dc.contributor.authorShen, L.
dc.contributor.authorShen, Z.
dc.date.accessioned2014-10-28T02:51:40Z
dc.date.available2014-10-28T02:51:40Z
dc.date.issued2003
dc.identifier.citationChan, R.,Shen, L.,Shen, Z. (2003). Restoring chopped and nodded images by tight frames. Proceedings of SPIE - The International Society for Optical Engineering 5205 : 310-319. ScholarBank@NUS Repository.
dc.identifier.issn0277786X
dc.identifier.urihttp://scholarbank.nus.edu.sg/handle/10635/104621
dc.description.abstractIn infrared astronomy, the observed chopped and nodded image g can be viewed as the image obtained by passing the true image f through a highpass filter. Here we propose an iterative restoration algorithm by building up a tight frame wavelet system from a multiresolution analysis that has the highpass filter as one of the wavelet filters. To recover f, the low frequency information of f hidden in g is unfolded by a wavelet decomposition and reconstruction algorithm and combined with the given high frequency information in g. The main advantage of using our method to restore chopped and nodded images is that there are fewer artifacts as compared to the well-known projected Landweber method. Also the noise in the restored image is significantly reduced. Simulated and real images are tested to illustrate the efficiency of our method. Here, we briefly describe the main ideas of our recent paper1 and the details can be found there.
dc.sourceScopus
dc.subjectChopped and nodded image
dc.subjectTight frame
dc.typeConference Paper
dc.contributor.departmentMATHEMATICS
dc.description.sourcetitleProceedings of SPIE - The International Society for Optical Engineering
dc.description.volume5205
dc.description.page310-319
dc.description.codenPSISD
dc.identifier.isiutNOT_IN_WOS
Appears in Collections:Staff Publications

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