

Publisher: Edp Sciences
E-ISSN: 1432-0746|492|2|L33-L34
ISSN: 0004-6361
Source: Astronomy & Astrophysics, Vol.492, Iss.2, 2008-12, pp. : L33-L34
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Related content


Kolmogorov cosmic microwave background sky
Astronomy & Astrophysics, Vol. 497, Iss. 2, 2009-04 ,pp. :


Kolmogorov complexity as a descriptorof cosmic microwave background maps
EPL (EUROPHYSICS LETTERS), Vol. 46, Iss. 1, 2010-03 ,pp. :




Concerning parameter estimation using the cosmic microwave background
Astronomy & Astrophysics, Vol. 368, Iss. 1, 2001-03 ,pp. :


On using the cosmic microwave background shift parameter in tests of models of dark energy
Astronomy & Astrophysics, Vol. 471, Iss. 1, 2007-08 ,pp. :