  We report photometric analysis of two main-belt asteroids observed at the
Observatorio Astronomico Nacional in the Sierra San Pedro Martir, Baja
California, M\'exico. For 18301 Konyukhov our derived intrinsic rotation period
is 2.6667 $\pm$ 0.0003 h with an amplitude of 0.16 magnitudes. To the best of
our knowledge, this is the first lightcurve reported for this asteroid. In the
case of 2022 West our derived intrinsic rotation period is 14.1385 $\pm$ 0.0031
h with an amplitude of 0.54 magnitudes.
