Required integration time to achieve SNR=20 assuming rms sensitivity of mJy.. cm Table 1. A list of 22 bright main sequence stars visible from Chajnantor that are non-variable and non-binary with expected GHz flux mJy, compiled by Richard Simon. They are unresolved by the 3 km baseline of the MMA, and the thermal blackbody emission from the 5 brightest stars can be detectable with.
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