The CMB temperature power spectrum from an improved analysis of the Archeops dataTRISTRAM, M; PATANCHON, G; BOCK, J. J et al.Astronomy and astrophysics (Berlin. Print). 2005, Vol 436, Num 3, pp 785-797, issn 0004-6361, 13 p.Article

The selection function of SZ cluster surveysMELIN, J.-B; BARTLETT, J. G; DELABROUILLE, J et al.Astronomy and astrophysics (Berlin. Print). 2005, Vol 429, Num 2, pp 417-426, issn 0004-6361, 10 p.Article

The galaxy cluster Y_SZ―L_X and Y_SZ―M relations from the WMAP 5-yr dataMELIN, J.-B; BARTLETT, J. G; DELABROUILLE, J et al.Astronomy and astrophysics (Berlin. Print). 2011, Vol 525, issn 0004-6361, A139.1-A139.11, 2Article

Blind component separation in wavelet space : Application to CMB analysisMOUDDEN, Y; CARDOSO, J.-F; STARCK, J.-L et al.EURASIP journal on applied signal processing. 2005, Vol 2005, Num 15, pp 2437-2454, issn 1110-8657, 18 p.Article

First detection of polarization of the submillimetre diffuse galactic dust emission by ArcheopsBENOIT, A; ADE, P; BOCK, J. J et al.Astronomy and astrophysics (Berlin. Print). 2004, Vol 424, Num 2, pp 571-582, issn 0004-6361, 12 p.Article

Catalog extraction in SZ cluster surveys : a matched filter approachMELIN, J.-B; BARTLETT, J. G; DELABROUILLE, J et al.Astronomy and astrophysics (Berlin. Print). 2006, Vol 459, Num 2, pp 341-352, issn 0004-6361, 12 p.Article

Planck intermediate results I. Further validation of new Planck clusters with XMM-NewtonAGHANIM, N; ARNAUD, M; BATTANER, E et al.Astronomy and astrophysics (Berlin. Print). 2012, Vol 543, issn 0004-6361, A102.1-A102.14, 2Article

Limits on the detectability of the CMB B-mode polarization imposed by foregroundsTUCCI, M; MARTINEZ-GONZALEZ, E; VIELVA, P et al.Monthly Notices of the Royal Astronomical Society. 2005, Vol 360, Num 3, pp 935-949, issn 0035-8711, 15 p.Article

Cosmic microwave background and foregrounds in Wilkinson Microwave Anisotropy Probe first-year dataPATANCHON, G; CARDOSO, J.-F; DELABROUILLE, J et al.Monthly Notices of the Royal Astronomical Society. 2005, Vol 364, Num 4, pp 1185-1194, issn 0035-8711, 10 p.Article

Scale-dependent non-Gaussianities in the WMAP data as identified by using surrogates and scaling indicesRÄTH, C; BANDAY, A. J; ROSSMANITH, G et al.Monthly notices of the Royal Astronomical Society (Print). 2011, Vol 415, Num 3, pp 2205-2214, issn 0035-8711, 10 p.Article

Planck pre-launch status: The HFI instrument, from specification to actual performance : PRE-LAUNCH STATUS OF THE PLANCK MISSIONLAMARRE, J.-M; PUGET, J.-L; BENOIT, A et al.Astronomy and astrophysics (Berlin. Print). 2010, Vol 520, issn 0004-6361, p. A9.1Article

A full sky, low foreground, high resolution CMB map from WMAPDELABROUILLE, J; CARDOSO, J.-F; LE JEUNE, M et al.Astronomy and astrophysics (Berlin. Print). 2009, Vol 493, Num 3, pp 835-857, issn 0004-6361, 23 p.Article

Measuring the tensor to scalar ratio from CMB B-modes in the presence of foregroundsBETOULE, M; PIERPAOLI, E; DELABROUILLE, J et al.Astronomy and astrophysics (Berlin. Print). 2009, Vol 503, Num 3, pp 691-706, issn 0004-6361, 16 p.Article

Temperature and polarization angular power spectra of Galactic dust radiation at 353 GHz as measured by ArcheopsPONTHIEU, N; MACIAS-PEREZ, J. F; BLANCHARD, A et al.Astronomy and astrophysics (Berlin. Print). 2005, Vol 444, Num 1, pp 327-336, issn 0004-6361, 10 p.Article

Séparation de composantes pour la mesure des anisotropies du fond diffus cosmologique. Une approche en aveugle basée sur la diversité spectrale : Modélisation : de la physique au traitement du signal = Component separation for measuring anisotropies in diffuse cosmological background. Blind approach based on spectral diversityPATANCHON, G; SNOUSSI, H; CARDOSO, J.-F et al.REE. Revue de l'électricité et de l'électronique. 2003, Num 6-7, pp 91-97, issn 1265-6534, 7 p.Article