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

Reconstructing isotropic and anisotropic $f(\mathcal{Q})$ cosmologies