New evidence for lack of CMB power on large scales  

作　　者：LIU Hao1 & LI TiPei1,2,3 1 Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China 2 Department of Physics & Center for Astrophysics, Tsinghua University, Beijing 100084, China 3 Department of Engineering Physics & Center for Astrophysics, Tsinghua University, Beijing 100084, China 

出　　处：《Science China(Physics,Mechanics & Astronomy)》2010年第3期567-570,共4页中国科学：物理学、力学、天文学（英文版）

基　　金：supported by the National Natural Science Foundation of China (Grant No. 10533020);the National Basic Research Program of China (Grant No. 2009CB824800);the China Postdoctoral Science Foundation Funded Project (Grant No. H91I21734A);the CAS Project (Grant No. KJCX2-YW-T03)

摘　　要：A digitalized temperature map is recovered from the first light sky survey image published by the Planck team, from which an angular power spectrum of the cosmic microwave background (CMB) is derived. The amplitudes of the low multipoles (low-l) measured from the preliminary Planck power spectrum are significantly lower than those reported by the WMAP team. Possible systematical effects are far from enough to explain the observed low-l differences.A digitalized temperature map is recovered from the first light sky survey image published by the Planck team, from which an angular power spectrum of the cosmic microwave background (CMB) is derived. The amplitudes of the low multipoles (low-l) measured from the preliminary Planck power spectrum are significantly lower than those reported by the WMAP team. Possible systematical effects are far from enough to explain the observed low-l differences.

关 键 词：COSMOLOGY COSMIC MICROWAVE BACKGROUND DATA analysis 

分 类 号：P142[天文地球—天体物理]