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Table 2. Praesepe member candidates based on our astrometric and photometric selection. Here we present the photometry and the astrometry of the candidates.

Table 3. Praesepe member candidates based on our astrometric and photometric selection. Here we present the physical parameters of the candidates, i.e. mass and effective temperature.

Table 6. Praesepe member candidates identified to have membership probabilities calculated from proper motions greater than 0.5.

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