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In-beam $ \gamma $-ray spectroscopy of $^{131}$Xe has been carried out tostudy the structure of the intruder $ \nu h_{11/2} $ band. Excited states werepopulated via an $ \alpha $-induced fusion-evaporation reaction at E$ _{\alpha}= 38 $ MeV. Inspection of $ \gamma \gamma $-coincidence data resulted in theidentification of a new rotational sequence. Based on the systematics ofexcitation energy, assigned spin-parity, decay pattern, and the electromagneticcharacter of the inter-band $ \Delta I = 1 $ $ \gamma $-transitions, thissequence is proposed as the unfavoured signature partner of the $ \nu h_{11/2}$ band. The structure of this band is further illuminated in the light of thetriaxial particle rotor model (TPRM). The possibility of wobbling excitation in$ N = 77 $ Xe-Ba-Ce isotones has been explored in a systematic manner.

Search for the origin of wobbling motion in the $ A \approx 130 $ region: The case of $^{131}$Xe