Separation of instrumental and astrophysical foregrounds for mapping cosmic microwave background anisotropies
Open Access
- 1 March 2002
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 330 (4) , 807-816
- https://doi.org/10.1046/j.1365-8711.2002.05200.x
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This publication has 18 references indexed in Scilit:
- Planetary Companions to the Metal‐rich Stars BD −10o3166 and HD 52265The Astrophysical Journal, 2000
- Neural networks and the separation of cosmic microwave background and astrophysical signals in sky mapsMonthly Notices of the Royal Astronomical Society, 2000
- Simultaneous estimation of noise and signal in cosmic microwave background experimentsMonthly Notices of the Royal Astronomical Society, 2000
- Foregrounds and CMB experimentsNew Astronomy, 1999
- Mapping the CMB sky: THE BOOMERanG experimentNew Astronomy Reviews, 1999
- Multifrequency Wiener filtering of cosmic microwave background data with polarizationMonthly Notices of the Royal Astronomical Society, 1999
- Foreground separation methods for satellite observations of the cosmic microwave backgroundMonthly Notices of the Royal Astronomical Society, 1998
- Analysis of the accuracy of a destriping method for future cosmic microwave background mapping with the PLANCK SURVEYOR satelliteAstronomy and Astrophysics Supplement Series, 1998
- Diffuse Galactic Emission from Spinning Dust GrainsThe Astrophysical Journal, 1998
- Small‐Scale Cosmological Perturbations: An Analytic ApproachThe Astrophysical Journal, 1996