in 2 hour scheduling blocks on 4 dates in early 2017: Feb 16, Mar 04, 11, and 13. The baselines ranged from 0.04 to 1.03 km. The weather conditions were very good, with phase noise measurements from the Atmospheric Phase Interferometer (on a 300 m baseline at 11.7 GHz) ranging from 3.3 to 7.4$\degr$. The phase center was set to the same position as for the SMA observations. The correlator was used to obtain the maximum continuum bandwidth of 8 GHz, comprised of 4 bands centered at 30, 32, 34, and 36 GHz, for two polarizations. The primary beam FWHM size of the 25-meter diameter array antennas is approximately $85\arcsec (\nu/ 30~\rm GHz)$. The observing sequence interleaved 1 minute observations of the complex gain calibrator 3C454.3 with 5 minute observations on HR 8799. Passband calibration was obtained with observations of 3C454.3. The absolute flux scale was set with observations of the standard calibrator 3C48 in each execution, with an estimated accuracy of 10%. The basic calibration was done using VLA pipeline processing in the [CASA]{} package (version 4.7.2) followed by imaging with [clean]{} task.

Results and Analysis {#sec:results}
====================

![image](fig1.eps)

\[fig:cont\]

![image](fig2.eps)

\[fig:vis\]

Continuum Emission {#subsec:continuum}
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Figure \[fig:cont\] shows 