The shell model (SM) is used to calculate the energy levels and transition probabilities ( 2) for 18,19,20 O isotopes. Two interactions (USDA and USDB) are used in the SDPN model space. We assume that all possible many-nucleon configurations are defined by the 0 5/2 , 1 1/2 , and 3/2 states that are higher than in
16O doubly magic nucleus. The available empirical data are in a good agreement with theoretical energy levels predictions. Spins and parities were affirmed for new levels, and the transition probabilities ( 2; ↓) are predicted.K e y w o r d s: shell model, OXBASH code, energy levels, model space, ( 2; ↓).