$f(T,B)$ cosmography for high redshifts
  In light of the statistical performance of cosmological observations, in this
work we present the cosmography in $f(T,B)$ gravity. In this scenario we found
a cosmological viable standard case that allows to reduce the degeneracy
between several $f(T,B)$ models already proposed in the literature.
Furthermore, we constrain this model using Pantheon SNeIa compilation, Cosmic
Chronometers and a newly GRB calibrated data sample. We found that with an
appropriate strategy for including the cosmographic parameter, we do produce a
viable cosmology with our model within $f(T,B)$ gravity.
