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The Simons Observatory (SO) is a suite of telescopes located in the AtacamaDesert in Chile that will make sensitive measurements of the cosmic microwavebackground. There are a host of cosmological and astrophysical questions thatSO is forecasted to address. The universal focal-plane modules (UFMs) populatethe four SO telescope receiver focal planes. There are three varieties of UFMs,each of which contains transition-edge-sensor bolometers observing in twospectral bands between 30 and 290~GHz. We describe the novel mid-frequencyUFMs, which target two of the six spectral bands at 90 and 150~GHz and arecentral to the cosmological goals of SO.

The 90 and 150 GHz universal focal-plane modules for the Simons Observatory