Motivated by the data analysis needs emerging from the ESA's cosmological mission Euclid, a linear noiseless model is introduced for a grism-generated slitless spectrographic image. A first-attempt strategy to spectrum deconvolution and decontamination is then suggested, neglecting the typical errors affecting this type of data, while trying to control the severe ill-posedness of the original problem. Three standard approaches are applied on a toy photometry, in order to have an idea on the solutions to be expected: the Moore-Penrose pseudoinversion, the standard Tikhonov regularization, and the preconditioned-projected Landweber iterative method.
Spectrum extraction from slitless spectrographic images
Salerno E;
2014
Abstract
Motivated by the data analysis needs emerging from the ESA's cosmological mission Euclid, a linear noiseless model is introduced for a grism-generated slitless spectrographic image. A first-attempt strategy to spectrum deconvolution and decontamination is then suggested, neglecting the typical errors affecting this type of data, while trying to control the severe ill-posedness of the original problem. Three standard approaches are applied on a toy photometry, in order to have an idea on the solutions to be expected: the Moore-Penrose pseudoinversion, the standard Tikhonov regularization, and the preconditioned-projected Landweber iterative method.File | Dimensione | Formato | |
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Descrizione: Spectrum extraction from slitless spectrographic images
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