Isern, J. (2010) Type Ia Supernova: Observations and Theory. Proceedings of the 11th Symposium on Nuclei in the Cosmos, Heidelberg, 19-23 July 2010, 66.
http://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=100

has been cited by the following article:

• TITLE: A New Insight into the Observations and Analysis of Type Ia Supernovae

  AUTHORS: Qiuhe Peng, Jingjing Liu

  KEYWORDS: Supernovae, Cosmology, Cosmic Microwave Background

  JOURNAL NAME: Journal of Applied Mathematics and Physics, Vol.9 No.7, July 30, 2021

  ABSTRACT: In this paper, we have given some analysis from observations of type Ia supernovae (SNIa). We find that the average total observational error of SNIa is obviously greater than 0.55m. On the other hand, a popular view of circumstantial evidence for the accelerating universe comes from the comparison of theoretical models simulating the accelerating expansion of the universe with observations from the Wilkinson Microwave Anisotropy Probe (WMAP) satellite deviating from the observed isotropic temperature of the Cosmic Microwave Background (CMB). Due to the fact that the velocity space is not isotropic, then the theoretical simulations are incredibly consistent with observations from the WMAP and Planck satellites. We conclude that the anisotropy of the velocity space will inevitably lead to an anisotropic distribution of the CMB temperature, and the above indirect evidence of the cosmic acceleration is inadequate and inappropriate.