CORC  > 清华大学
Observation number correlation in WMAP data
Li, Ti-Pei ; Liu, Hao ; Song, Li-Ming ; Xiong, Shao-Lin ; Nie, Jian-Yin
2010-10-12 ; 2010-10-12
关键词methods: data analysis cosmic microwave background cosmology: observations SYSTEMATIC-ERROR LIMITS ANISOTROPY-PROBE DATA RADIOMETER CHARACTERIZATION MICROWAVE ANOMALIES ISOTROPY MAPS ALIGNMENT FIELD SKY Astronomy & Astrophysics
中文摘要A remarkable similarity between the large-scale non-Gaussian pattern of cosmic microwave background (CMB) temperatures obtained by the Wilkinson Microwave Anisotropy Probe (WMAP) mission and the distribution features of observation numbers is noted. Motivated by such a similarity, in this work we check the WMAP data for the correlation between pixel temperature t and observation number N. Systematic effects of imbalance in the differential observations and significant t-N correlations in magnitude, distribution of non-Gaussianity and north-south asymmetry are found. Our results indicate that, for precision cosmology studies based on WMAP observations, the observation effect on released WMAP temperature maps requires further careful study.
语种英语 ; 英语
出版者WILEY-BLACKWELL PUBLISHING, INC ; MALDEN ; COMMERCE PLACE, 350 MAIN ST, MALDEN 02148, MA USA
内容类型期刊论文
源URL[http://hdl.handle.net/123456789/81643]  
专题清华大学
推荐引用方式
GB/T 7714
Li, Ti-Pei,Liu, Hao,Song, Li-Ming,et al. Observation number correlation in WMAP data[J],2010, 2010.
APA Li, Ti-Pei,Liu, Hao,Song, Li-Ming,Xiong, Shao-Lin,&Nie, Jian-Yin.(2010).Observation number correlation in WMAP data..
MLA Li, Ti-Pei,et al."Observation number correlation in WMAP data".(2010).
个性服务
查看访问统计
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。


©版权所有 ©2017 CSpace - Powered by CSpace