High-spin states in 123 I were populated in the reaction 80 Se( 48 Ca,p4n) 123 I at a beam energy of 207 MeV and γ -ray coincidence events were measured using the Gammasphere spectrometer. Three weakly populated, high-spin rotational bands have been discovered with characteristics similar to those of the long collective bands recently observed in other nuclei of this mass region. Configuration assignments are proposed based on calculations within the framework of the cranked Nilsson-Strutinsky approach.The nuclei in the A = 125 mass region, with a limited number of valence nucleons outside the 114 Sn core, undergo a transition from weakly prolate deformation at low spin to an oblate shape at medium spin. The shape change is induced by the successive alignment of nucleons along the rotation axis and, finally, the level sequences terminate in maximally aligned oblate states [1][2][3][4][5][6]. In addition, several high-spin rotational bands have recently been observed in 120 Te [7], 124 Ba [6], 125 I [8], 125 Xe [9], and 126 Xe [10], which extend far beyond the noncollective oblate states. Only some of these sequences are firmly connected to lower-lying levels; they feed normal-deformed states in the spin range of I 25 at excitation energies around 10 MeV.In the present work, the results of a further analysis of the data from the experiment to investigate the high-spin structure of 123 I [2] are reported. This investigation revealed three highly deformed bands in this nucleus. Their properties are similar to those of the long bands observed in neighboring nuclei. Cranked Nilsson-Strutinsky (CNS) calculations have been employed to propose configurations for the new bands.High-spin states in 123 I were populated using the reaction 80 Se( 48 Ca,p4n) 123 I. The beam with an energy of 207 MeV was provided by the ATLAS accelerator at ANL. The target consisted of a 80 Se layer with a thickness of 0.6 mg/cm 2 . Gamma-ray coincidence events were recorded with the Gammasphere spectrometer [11]. Further details on the experiment and the data analysis are given in previous publications by the present collaboration [2,7].The three rotational sequences with large moments of inertia discovered in 123 I are displayed in Fig. 1. Their intensities are <1% of the channel strength. Bands a and b are about equal in intensity, while band c is weaker. Such small intensities preclude a measurement of directional correlations. However, the regularity of the bands and their similarity with high-spin bands in neighboring nuclei suggests that the in-band transitions are of E2 multipolarity. It was not possible to establish linking transitions into known 123 I levels. Excitation energies and spins of the new bands were estimated on the basis of the observed coincidences. These values were varied within reasonable limits to give agreement with theoretical predictions for the suggested configurations. The adopted values are similar to those of the connected bands in the neighboring nuclei 125 I [8], 125 Xe [9], and 126 Xe [10].Triple-gated γ -ra...