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Suzuki, N., et al. (2011) The Hubble Space Telescope Cluster Supernovae Survey: V. Improving the Dark Energy Constraints Above Z > 1 and Building an Early-Type-Hosted Supernova Sample.

has been cited by the following article:

• TITLE: How a Realistic Linear Rh = ct Model of Cosmology Could Present the Illusion of Late Cosmic Acceleration

  AUTHORS: Eugene Terry Tatum, U. V. S. Seshavatharam

  KEYWORDS: Dark Energy Survey, Cosmology Theory, Cosmic Coasting, Cosmic Flatness, Type Ia Supernovae, CMBR, Flat Space Cosmology, Milne Universe Theories

  JOURNAL NAME: Journal of Modern Physics, Vol.9 No.7, June 8, 2018

  ABSTRACT: Realistic FLRW cosmic coasting models which contain matter now appear to be a reasonable alternative in explaining the accumulated Supernova Cosmology Project data since 1998. In sharp contrast to the unrealistic original classic Milne universe, which was entirely devoid of matter, these modified Milne-type models containing matter, often referred to as realistic linear Rh = ct models, have rapidly become the primary competition with standard cosmology. This paper compares the expected relative luminosity distances and relative angular diameter distances for given magnitudes of redshift within these two competing models. A simple ratio formula is derived, which explains how expected luminosity distances and angular diameter distances for given magnitudes of redshift within a realistic Milne-type cosmic expansion could create the illusion (for standard model proponents) of cosmic acceleration where none exists.