A fast directional continuous spherical wavelet transform
| dc.creator | McEwen, J. D. | |
| dc.creator | Hobson, M. P. | |
| dc.creator | Lasenby, A. N. | |
| dc.creator | Mortlock, D. J. | |
| dc.date | 2004-09-13 | |
| dc.date.accessioned | 2026-07-07T02:14:35Z | |
| dc.date.available | 2026-07-07T02:14:35Z | |
| dc.description | A fast algorithm for Antoine and Vandergheynst's (1998) directional continuous spherical wavelet transform (CSWT) is presented. Computational requirements are reduced by a factor of O(\sqrt{N}), when N is the number of pixels on the sphere. The spherical Mexican hat wavelet Gaussianity analysis of the WMAP 1-year data performed by Vielva et al. (2003) is reproduced and confirmed using the fast CSWT. The proposed extension to directional analysis is inherently afforded by the fast CSWT algorithm. | |
| dc.description | 4 pages, 2 figures, XXXIXth Recontres de Moriond | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0409288 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0409288 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8167 | |
| dc.subject | Astrophysics | |
| dc.title | A fast directional continuous spherical wavelet transform | |
| dc.type | text |