  The paper deals with cosmology in modified f(T) gravity theory. With some
phenomenological choices for the function f(T) it is possible to have
cosmological solutions describing different phases of the evolution of the
Universe for the homogeneous and isotropic FLRW model. By proper choice of the
parameters involved in the function $f(T)$ and also in the cosmological
solutions it is shown that a continuous cosmic evolution starting from the
emergent scenario to the present late time acceleration is possible. Finally
thermodynamical analysis of f(T) gravity is presented.
