Supported by the National Natural Science Foundation of China under Grant Nos.11690021,11575271,and 11747601;the Strategic Priority Research Program of Chinese Academy of Sciences under Grant Nos.XDB23000000 and XDA15020701;Top-Notch Young Talents Program of China
We report the constraints of H0 obtained from Wilkinson Microwave Anisotropy Probe(WMAP)9-year data combined with the latest baryonic acoustic oscillations(BAO)measurements.We use the BAO measurements from 6dF Galaxy ...
supported by the National Natural Science Foundation of China (Grant Nos. 10821504, 11322545, 11335012, 11173021 and 11322324);the Project of KIP of the Chinese Academy of Sciences and the National Basic Research Program of China (Grant No. 2012CB821804)
Recently Background Imaging of Cosmic Extragalactic Polarization (B2) discovered the relic gravitational waves at 7.00- confi- dence level. However, the other cosmic microwave background (CMB) data, for example Pl...
supported by the National Basic Research Program of China(2009CB824800);the National Natural Science Foundation of China(11033003);the National Natural Science Foundation for Young Scientistsof China (11203024);the Youth Innovation Promotion Association,CAS
In cosmic microwave background (CMB) experiments, foreground-cleaned temperature maps are still contaminated by the residual dipole due to uncertainties of the Doppler dipole direction and microwave radiometer sidelob...
Previous work by Sigalotti in 2006 and recently by Hendi and Sharifzadeh in 2012 showed that all the fundamental equations of special relativity may be derived from a golden mean proportioned classical-Euclidean trian...
supported by the National Natural Science Foundation of China (11033003);National Basic Research Program of China (2009CB824800);the CAS project (KJCX2-YW-T03)
We have discovered in our previous work that different observational systematics,e.g.errors from antenna pointing directions or an asynchronism between the attitude and science data may generate a pseudo-dipole signal...