  We present a reconstruction algorithm for cosmological models based on
$f(\mathcal{Q})$ gravity. We specifically focus on obtaining exact Bianchi
Type-I and Friedmann-Lema\^{\i}tre-Robertson-Walker solutions, finding
solutions that might have application in a variety of scenarios such as
spontaneous isotropization of Bianchi Type-I models, dark energy, inflation as
well as pre-Big Bang cosmologies.
