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The Mexican Hat Wavelet Family. Application to the study of non-Gaussianity in cosmic microwave background maps.

, , , , and . EUSIPCO, page 1-5. IEEE, (2006)

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Matrix Filters for the Detection of Extragalactic Point Sources in Cosmic Microwave Background Images., and . J. Sel. Topics Signal Processing, 2 (5): 727-734 (2008)Filter design for the detection/estimation of the modulus of a vector: Application to polarization data., , and . Signal Process., 91 (7): 1527-1534 (2011)The Mexican Hat Wavelet Family. Application to point source detection in cosmic microwave background maps., , , , , , and . EUSIPCO, page 1-4. IEEE, (2005)Adaptive Langevin Sampler for Separation of t-Distribution Modelled Astrophysical Maps., , , , , and . IEEE Trans. Image Processing, 19 (9): 2357-2368 (2010)Astrophysical image denoising using bivariate isotropic cauchy distributions in the undecimated wavelet domain., , and . ICIP, page 1225-1228. IEEE, (2004)A Bayesian approach to filter design: detection of compact sources., , , and . Computational Imaging, volume 5299 of SPIE Proceedings, page 145-154. SPIE, (2004)Astrophysical image separation by blind time-frequency source separation methods., , and . Digit. Signal Process., 19 (2): 360-369 (2009)Blind source separation from multi-channel observations with channel-variant spatial resolutions., , , , and . EUSIPCO, page 1077-1081. IEEE, (2010)Filtering in the Time-Frequency domain for the detection of compact objects., , and . EUSIPCO, page 2067-2071. IEEE, (2009)A sparse approach to astronomical point source detection., , , and . EUSIPCO, page 139-143. IEEE, (2010)