  An asteroid pair can be described as two asteroids with highly similar
heliocentric orbits that are genetically related but not gravitationally bound.
They can be produced by asteroid collisions or rotational fission. Although
over 200 asteroid pairs are known, many more are remaining to be identified,
especially among the newly discovered asteroids. The purpose of our work is to
find new asteroid pairs in the inner part of the main belt with a new pipeline
for asteroid pair search, as well as to validate the pipeline on a sample of
known asteroid pairs. Initially, we select pair candidates in the
five-dimensional space of osculating orbital elements. Then the candidates are
confirmed using numerical modeling with the backtrack integration of their
orbits including the perturbations from the largest main-belt asteroids, as
well as the influence of the non-gravitational Yarkovsky effect. We performed a
survey of the inner part of the main belt and found 10 new probable asteroid
pairs. Their estimated formation ages lie between 30 and 400 kyr. In addition,
our pipeline was tested on a sample of 17 known pairs, and our age estimates
agreed with the ones indicated in literature in most of the cases.
