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, Direct 233 GHz measurements from ALMA indicate a mean flux of 3.47 ± 0.024 ± 0.24 Jy, where the first error bar is the formal uncertainty calculated from the individual errors, and the second one is the standard deviation between the individual measurements. Spectral index (spix) fitting of the mean 91.5, 103 and 343 GHz fluxes gives spix = -0.56 and a 233 GHz flux of 3.55 Jy, fully consistent with above. Because we do not have any other quasars available to calibrate the Chariklo data, days before 2002 GZ 32 ) to be 1.35 ± 0.09 Jy. Specifying a 1.87 Jy for the prime calibrator J1733-1304 leads to 1.28 Jy for J1751+0939 in our data. A better overall compromise is achieved by specifying 1.93 Jy for J1733-1304 (+3.2% higher than the initial estimate, 2002.

. Müller, On another hand, the spectral index, derived from 10 sets of ALMA 91.5, 103.5 and 343 GHz dat, is spix = -0.50 ± 0.05. Applying this to the 343 GHz flux measured on the same date (2.5 ± 0.34 Jy) would provide 3.03 ± 0.41 Jy, only 1.2? consistent with the above. The weighted-mean average of the two values is 3.61 ± 0.17 Jy. We still adopt the directly measured value of 3.74 Jy, but inflate somewhat the uncertainty to 0.25 Jy (6.7%). With this, we derive a Pallas flux of 159 ± 11 mJy for, -J0006-0623 and Pallas (Chiron). Asteroid (4) Pallas was observed as the prime calibrator for the Chiron observations. Detailed shape and thermophysical models, vol.27, 2014.