Intermediate evolution using SNIa, and BAO
  We study the intermediate evolution model and show that, compared with the
recent study of a power-law evolution, the intermediate evolution is a better
description of the low-redshift regime supported by observations from type Ia
supernovae and BAO. We found also that recent data suggest that the
intermediate evolution is as good a fit to this redshift range as the
$\Lambda$CDM model.
