The power spectrum of the cosmic microwave background Kolmogorov maps: possible clue to correlation of voidsGURZADYAN, V. G; KASHIN, A. L; KHACHATRYAN, H. G et al.Astronomy and astrophysics (Berlin. Print). 2009, Vol 506, Num 3, issn 0004-6361, L37-L40Article

Induced two-photon decay of the 2s level and the rate of cosmological hydrogen recombinationCHLUBA, J; SUNYAEV, R. A.Astronomy and astrophysics (Berlin. Print). 2006, Vol 446, Num 1, pp 39-42, issn 0004-6361, 4 p.Article

Antenna instrumental polarization and its effects on E- and B-modes for CMBP observationsCARRETTI, E; CORTIGLIONI, S; SBARRA, C et al.Astronomy and astrophysics (Berlin. Print). 2004, Vol 420, Num 2, pp 437-445, issn 0004-6361, 9 p.Article

Kolmogorov stochasticity parameter measuring the randomness in the cosmic microwave backgroundGURZADYAN, V. G; KOCHARYAN, A. A.Astronomy and astrophysics (Berlin. Print). 2008, Vol 492, Num 2, issn 0004-6361, L33-L34Article

Kolmogorov cosmic microwave background skyGURZADYAN, V. G; ALLAHVERDYAN, A. E; GHAHRAMANYAN, T et al.Astronomy and astrophysics (Berlin. Print). 2009, Vol 497, Num 2, pp 343-346, issn 0004-6361, 4 p.Article

Some good reasons to use matched filters for the detection of point sources in CMB mapsVIO, R; ANDREANI, P; WAMSTEKER, W et al.Astronomy and astrophysics (Berlin. Print). 2004, Vol 414, Num 1, pp 17-21, issn 0004-6361, 5 p.Article

A test of the Poincaré dodecahedral space topology hypothesis with the WMAP CMB dataLEW, B; ROUKEMA, B.Astronomy and astrophysics (Berlin. Print). 2008, Vol 482, Num 3, pp 747-753, issn 0004-6361, 7 p.Article

Comparison of map-making algorithms for CMB experimentsPOUTANEN, T; DE GASPERIS, G; MAINO, D et al.Astronomy and astrophysics (Berlin. Print). 2006, Vol 449, Num 3, pp 1311-1322, issn 0004-6361, 12 p.Article

The effects of low temporal frequency modes on minimum variance maps from PLANCKSTOMPOR, R; WHITE, M.Astronomy and astrophysics (Berlin. Print). 2004, Vol 419, Num 2, pp 783-792, issn 0004-6361, 10 p.Article

The effect of signal digitisation in CMB experimentsMARIS, M; MAINO, D; BURIGANA, C et al.Astronomy and astrophysics (Berlin. Print). 2004, Vol 414, Num 2, pp 777-794, issn 0004-6361, 18 p.Article

Porosity criterion for hyperbolic voids and the cosmic microwave backgroundGURZADYAN, V. G; KOCHARYAN, A. A.Astronomy and astrophysics (Berlin. Print). 2009, Vol 493, Num 3, issn 0004-6361, L61-L63Article

Mapping the large-scale anisotropy in the WMAP dataBERNUI, A; MOTA, B; REBOUCAS, M. J et al.Astronomy and astrophysics (Berlin. Print). 2007, Vol 464, Num 2, pp 479-485, issn 0004-6361, 7 p.Article

Trade-off between angular resolution and straylight contamination in the PLANCK Low Frequency Instrument. I. Pattern simulationsSANDRI, M; VILLA, F; NESTI, R et al.Astronomy and astrophysics (Berlin. Print). 2004, Vol 428, Num 1, pp 299-310, issn 0004-6361, 12 p.Article

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

ROMA : A map-making algorithm for polarised CMB data setsDE GASPERIS, G; BALBI, A; CABELLA, P et al.Astronomy and astrophysics (Berlin. Print). 2005, Vol 436, Num 3, pp 1159-1165, issn 0004-6361, 7 p.Article

What can be learned about dark energy evolution?DOUSPIS, M; ZOLNIEROWSKI, Y; BLANCHARD, A et al.Astronomy and astrophysics (Berlin. Print). 2008, Vol 488, Num 1, pp 47-53, issn 0004-6361, 7 p.Article

Small scale contributions to the cosmic microwave background : a coherent analysisDOUSPIS, M; AGHANIM, N; LANGER, M et al.Astronomy and astrophysics (Berlin. Print). 2006, Vol 456, Num 3, pp 819-826, issn 0004-6361, 8 p.Article

Dust from reionizationELFGREN, E; DESERT, F.-X.Astronomy and astrophysics (Berlin. Print). 2004, Vol 425, Num 1, pp 9-14, issn 0004-6361, 6 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

Effects of thermal fluctuations in the SPOrt experimentCARRETTI, E; ZANNONI, M; MACCULI, C et al.Astronomy and astrophysics (Berlin. Print). 2004, Vol 428, Num 3, pp 781-791, issn 0004-6361, 11 p.Article

Is there a need and another way to measure the cosmic microwave background temperature more accurately?CHLUBA, J; SUNYAEV, R. A.Astronomy and astrophysics (Berlin. Print). 2008, Vol 478, Num 2, issn 0004-6361, L27-L30Article

Testing CPT symmetry with CMB measurementsXIA, J.-Q; LI, H; WANG, X et al.Astronomy and astrophysics (Berlin. Print). 2008, Vol 483, Num 3, pp 715-718, issn 0004-6361, 4 p.Article

Spectral indications of thermal Sunyaev-Zel'dovich effect in ARCHEOPS and WMAP dataHERNANDEZ-MONTEAGUDO, C; MACIAS-PEREZ, J. F; TRISTRAM, M et al.Astronomy and astrophysics (Berlin. Print). 2006, Vol 449, Num 1, pp 41-48, issn 0004-6361, 8 p.Article

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

A halo approach to the evaluation of the cross-correlation between the SZ sky and galaxy surveysQU, Y; WU, X.-P.Astronomy and astrophysics (Berlin. Print). 2004, Vol 423, Num 1, pp 21-26, issn 0004-6361, 6 p.Article