Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/4859
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dc.contributor.authorHallur, Pravita-
dc.contributor.authorMedeiros, Lia-
dc.contributor.authorLauer, Tod R.-
dc.date.accessioned2023-08-18T18:36:02Z-
dc.date.available2023-08-18T18:36:02Z-
dc.date.issued2022-
dc.identifier.citationAstrophysical Journal, 927(1), 45170.en_US
dc.identifier.urihttp://doi.org/10.3847/1538-4357/ac502a-
dc.identifier.urihttp://hdl.handle.net/123456789/4859-
dc.descriptionOnly IISER Mohali authors are available in the record.en_US
dc.description.abstractWe demonstrate the use of an eigenbasis that is derived from principal component analysis (PCA) applied on an ensemble of random-noise images that have a "red" power spectrum; i.e., a spectrum that decreases smoothly from large to small spatial scales. The pattern of the resulting eigenbasis allows for the reconstruction of images with a broad range of image morphologies. In particular, we show that this general eigenbasis can be used to efficiently reconstruct images that resemble possible astronomical sources for interferometric observations, even though the images in the original ensemble used to generate the PCA basis are significantly different from the astronomical images. We further show that the efficiency and fidelity of the image reconstructions depends only weakly on the particular parameters of the red-noise power spectrum used to generate the ensemble of images.en_US
dc.language.isoen_USen_US
dc.publisherIOP Publishingen_US
dc.subjectRed-noiseen_US
dc.subjectEigenbasisen_US
dc.subjectReconstructionen_US
dc.subjectBlobby Imagesen_US
dc.titleA Red-noise Eigenbasis for the Reconstruction of Blobby Imagesen_US
dc.typeArticleen_US
Appears in Collections:Research Articles

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