J013333.22+303343.4, J013350.12+304126.6

Both objects display all classification characteristics of B[e]SGs. Their locations in the WISE diagram coincide with the B[e]SG domain. In the near-IR diagram they appear slightly off the B[e]SG region, shifted towards the HAeBe domain, but their high-luminosities clearly classify them as supergiants. The CO band absorption detected from J013333.22+303343.4 cannot be explained with a cool companion, but might originate from a pole-on seen jet [138]. Whether also CO band emission is present in this object, but veiled by the intense absorption component, is currently unknown.
