  The Simons Observatory (SO) is a Cosmic Microwave Background experiment
located in the Atacama Desert in Chile. SO consists of three small aperture
telescopes (SATs) and one large aperture telescope (LAT) with a total of 60,000
detectors in six frequency bands. As an observatory, SO encompasses hundreds of
hardware components simultaneously running at different readout rates, all
separate from its 60,000 detectors on-sky and their metadata. We provide an
overview of commissioning SO's data acquisition software system for SAT-MF1,
the first SAT deployed to the Atacama site. Additionally, we share insights
from deploying data access software for all four telescopes, detailing how
performance limitations affected data loading and quality investigations, which
led to site-compatible software improvements.
