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Cited article:

Instrument, method, brightness, and polarization maps from the 2003 flight of BOOMERanG

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Astronomy & Astrophysics 458 (3) 687 (2006)
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XSPECT, estimation of the angular power spectrum by computing cross-power spectra with analytical error bars

M. Tristram, J. F. Macias-Perez, C. Renault and D. Santos
Monthly Notices of the Royal Astronomical Society 358 (3) 833 (2005)
https://doi.org/10.1111/j.1365-2966.2005.08760.x

Effects of Foreground Contamination on the Cosmic Microwave Background Anisotropy Measured byMAP

Chan‐Gyung Park, Changbom Park and Bharat Ratra
The Astrophysical Journal 568 (1) 9 (2002)
https://doi.org/10.1086/338840

Cosmological Parameter Determination from Counts of Galaxies

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The Astrophysical Journal 563 (1) 28 (2001)
https://doi.org/10.1086/323698

Cosmology from cosmic microwave background and galaxy clusters

M. Douspis, A. Blanchard, R. Sadat, J. G. Bartlett and M. Le Dour
Astronomy & Astrophysics 379 (1) 1 (2001)
https://doi.org/10.1051/0004-6361:20011283

Cosmic microwave background anisotropy power spectrum statistics for high precision cosmology

Benjamin D. Wandelt, Eric Hivon and Krzysztof M. Górski
Physical Review D 64 (8) (2001)
https://doi.org/10.1103/PhysRevD.64.083003

Window Function for Noncircular Beam Cosmic Microwave Background Anisotropy Experiment

Tarun Souradeep and Bharat Ratra
The Astrophysical Journal 560 (1) 28 (2001)
https://doi.org/10.1086/322425