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We extend the results of a previous analysis of ours showing that, when bothheavy and light flavour effects are taken into account, successful minimal(type I + thermal) leptogenesis with SO(10)-inspired relations is possible.Barring fine tuned choices of the parameters, these relations enforce ahierarchical RH neutrino mass spectrum that results into a final asymmetrydominantly produced by the next-to-lightest RH neutrino decays (N_2 dominatedleptogenesis). We present the constraints on the whole set of low energyneutrino parameters. Allowing a small misalignment between the Dirac basis andthe charged lepton basis as in the quark sector, the allowed regions enlargeand the lower bound on the reheating temperature gets relaxed to values as lowas ~ 10^10 GeV. It is confirmed that for normal ordering (NO) there are twoallowed ranges of values for the lightest neutrino mass: m_1 \simeq (1-5)\times10^-3 eV and m_1\simeq (0.03-0.1) eV. For m_1\lesssim 0.01 eV the allowedregion in the plane theta_13-theta_23 is approximately bounded by 44 +3(theta_13-9) \lesssim theta_23 \lesssim 48 + 0.4 (theta_13-5), while theneutrinoless double beta decay effective neutrino mass falls in the rangem_ee=(1-3)10^-3 eV for theta_13=(6 -11.5). For m_1 \gtrsim 0.01 eV, one hasquite sharply m_ee\simeq m_1 and an upper bound theta_23 \lesssim 46 . Theseconstraints will be tested by low energy neutrino experiments during nextyears. We also find that inverted ordering (IO), though quite stronglyconstrained, is not completely ruled out. In particular, we find approximatelytheta_23 \simeq 43 +12 log(0.2 eV/m_1), that will be fully tested by futureexperiments.

Testing SO(10)-inspired leptogenesis with low energy neutrino experiments