  In this work we use the latest observations on SNIa, $H(z)$, BAO, $f_{gas}$
in clusters and CMBR, to constrain three models showing an explicit interaction
between dark matter and dark energy. In particular, we use the BOSS BAO
measurements at $z \simeq 0.32$, $0.57$ and $2.34$, using the full
2-dimensional constraints on the angular and line of sight BAO scale. We find
that using all five observational probes together, two of the interaction
models show positive evidence at more than 3 $ \sigma $. Although significant,
further study is needed to establish this statement firmly.
