The Mexican hat wavelet family: application to point-source detection in cosmic microwave background maps
- 7 June 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 369 (4) , 1603-1610
- https://doi.org/10.1111/j.1365-2966.2006.10442.x
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This publication has 27 references indexed in Scilit:
- SURVEYS OF EXTRAGALACTIC SOURCES WITH PLANCKPublished by Springer Nature ,2006
- Source subtraction for the extended Very Small Array and 33-GHz source count estimatesMonthly Notices of the Royal Astronomical Society, 2005
- Predictions for high-frequency radio surveys of extragalactic sourcesAstronomy & Astrophysics, 2005
- First‐YearWilkinson Microwave Anisotropy Probe(WMAP) Observations: Foreground EmissionThe Astrophysical Journal Supplement Series, 2003
- Predictions for Cosmological Infrared Surveys from Space with the Multiband Imaging Photometer forSIRTFThe Astrophysical Journal, 2003
- TheMicrowave Anisotropy ProbeMissionThe Astrophysical Journal, 2003
- Spherical Mexican hat wavelet: an application to detect non-Gaussianity in theCOBE-DMR mapsMonthly Notices of the Royal Astronomical Society, 2001
- Constraining our Universe with X-ray and optical cluster dataMonthly Notices of the Royal Astronomical Society, 2001
- Isotropic wavelets: a powerful tool to extract point sources from cosmic microwave background mapsMonthly Notices of the Royal Astronomical Society, 2000
- A Method Based on Wavelet Transforms for Source Detection in Photon‐counting Detector Images. II. Application toROSATPSPC ImagesThe Astrophysical Journal, 1997