Note. DPFU values are quoted for both lower (LSB) and upper (USB) sidebands, and both polarizations (RCP and LCP). For phased arrays (ALMA and SMA), the DPFUs represent the combined sensitivity of all phased dishes. The gain curve parameters B and E₀ as a function of elevation E are given based on a g_E = 1 − B(E − E₀)² parameterization (see Janssen et al. 2019b; Koay et al. 2023a, for further details). ^aThe ALMA DPFU uncertainty is based on the overall 10% systematic uncertainties associated with the QA2 flux calibration tables. ^bAPEX measures DPFUs for each of the four bands separately. LSB and USB DPFUs shown here are the mean of the bands 1 and 2 DPFUs, and bands 3 and 4 DPFUs, respectively. ^cGLT DPFU uncertainties are based on the scatter of three measurements, inclusive of flux density model errors, but may be larger due to significant antenna astigmatism. There is also a ∼15% uncertainty contributing to the total SEFD uncertainty. ^dFor the JCMT DPFU, the nighttime value is shown. ^eThe SMA DPFU uncertainty is based on the dominant 5−15% uncertainty on the phasing efficiency.