Dipole of the luminosity distance as a test for dark energy models
  The dependence of Hubble parameter on redshift can be determined directly
from the dipole of luminosity distance to Supernovae Ia. We investigate the
possibility of using the data on dipole of the luminosity distance obtained
from the Supernovae Ia compilations SDSS, Union2.1, JLA and Pantheon to
distinguish the dark energy models.
