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Table 2

Continuum fluxes, major axis, axis ratio and position angle derived from fitting a disk (D, for the ALMA data) or a Gaussian or point source (G or P, for the ATCA data) to the visibilities.

ID Wavelength Flux Error uv model Major axis Inclination PA
mm mJy mJy arcsec degrees degrees

ALMA band 7 0.853 2253.16 0.96 D 2.25 (0.01) 41.4±0.9 4.5 (0.1)
ALMA band 3 2.939 92.0 2.5 D 2.27 (0.02) 40.5±0.9 2.3 (1.7)

ATCA 97 GHz 3.091 76.3 5.7 G
ATCA 95 GHz 3.156 62.3 4.7 G
ATCA 93 GHz 3.224 63.0 3.5 G
ATCA 91 GHz 3.294 62.9 3.0 G
ATCA 45 GHz 6.662 5.2 0.7 G
ATCA 43 GHz 6.972 5.1 0.5 G
ATCA 40 GHz 7.459 2.67 0.21 G
ATCA 38 GHz 7.889 2.36 0.23 G
ATCA 35 GHz 8.565 2.51 0.18 G 1.7 49.5 16
ATCA 33 GHz 9.085 2.07 0.25 G 1.6 55.9 16
ATCA 24 GHz 12.491 1.16 0.34 P
ATCA 19 GHz 15.779 0.80 0.09 P
ATCA 18 GHz 16.655 0.72 0.16 P
ATCA 17 GHz 17.635 0.70 0.06 P
ATCA 9 GHz 33.310 0.3 +0.3 -0.15 P
ATCA 5.5 GHz 54.508 0.3 +0.3 -0.15 P

Notes. The flux error values do not include errors on flux calibration, which we estimate to be 10% for the ALMA observations and 20% for the ATCA observations. The 5.5, 9, 17, and 19 GHz ATCA fluxes were earlier published in Ubach (2014). We re-extract the fluxes from the observations following the same method as used for the other ATCA fluxes for consistency.

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