  The Simons Observatory (SO) is a next-generation ground-based telescope
located in the Atacama Desert in Chile, designed to map the cosmic microwave
background (CMB) with unprecedented precision. The observatory consists of
three small aperture telescopes (SATs) and one large aperture telescope (LAT),
each optimized for distinct but complementary scientific goals. To achieve
these goals, optimized scan strategies have been defined for both the SATs and
LAT. This paper describes a software system deployed in SO that effectively
translates high-level scan strategies into realistic observing scripts
executable by the telescope, taking into account realistic observational
constraints. The data volume of SO also necessitates a scalable software
infrastructure to support its daily data processing needs. This paper also
outlines an automated workflow system for managing data packaging and daily
data reduction at the site.
