Using Gaia DR3 with ASteCA and SED fitting, the authors derive structural, kinematic, and orbital parameters for open clusters SAI 72 and SAI 75, but the adopted SAI 75 motion conflicts with catalog values.
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Enhancing SED-Based Astrometric, Photometric, and Kinematic Studies of SAI 72 and SAI 75 Using Gaia DR3
Using Gaia DR3 with ASteCA and SED fitting, the authors derive structural, kinematic, and orbital parameters for open clusters SAI 72 and SAI 75, but the adopted SAI 75 motion conflicts with catalog values.