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Table D.1

Peak flux and map rms from the science target images processed with and without WVR scaling.

UID Separation Peak flux Image rms S/N Peak flux Image rms S/N Improvement
to BP cal. standard standard scaled scaled ratio
(°) (mJy/bm) (μJy/bm) (mJy/bm) (μJy/bm)

Juno Band 6

Xbc7 a 8.6 7.045 84.92 83.0 7.049 84.64 83.3 1.004
Xbc7 b 8.6 6.945 81.60 85.1 6.962 81.54 85.4 1.003
Xdae a 8.6 6.512 87.96 74.0 6.516 87.99 74.0 1.000
Xdae b 8.6 6.865 88.95 77.2 6.852 88.90 77.1 0.998
X1363 a 8.6 3.434 182.18 18.8 3.470 182.24 19.0 1.010
X1363 b 8.6 3.251 156.62 20.8 3.189 157.71 20.2 0.974

Mira Band 6

X423 7.6 44.30 395.5 112.0 48.94 290.1 168.7 1.506

X137 20.2 65.13 163.1 399.2 65.23 143.9 453.1 1.135

HL Tau Band 3

Xc7f 9.1 2.887 26.72 108.0 2.843 26.76 106.2 0.983

HL Tau Band 6

Xb2 9.1 7.485 51.05 146.6 7.693 49.73 154.7 1.055

Xc8c 9.1 5.171 46.39 111.4 5.307 46.28 114.6 1.028

Xdc 19.7 8.250 61.60 133.9 8.259 62.78 131.5 0.982

X760 27.0 5.519 38.16 144.6 5.877 38.07 154.3 1.067
X9dd 19.7 5.661 37.11 152.5 5.933 36.16 164.0 1.076
Xc3c 9.1 6.261 35.72 175.2 6.366 35.92 177.1 1.011

X387 9.1 6.738 38.34 175.7 6.789 38.32 177.1 1.008

HL Tau Band 7

X20a 19.7 8.203 80.65 101.7 8.399 81.00 103.7 1.018
X6d8 19.7 8.057 83.93 96.0 8.250 83.85 98.4 1.024
Xa16 9.1 8.469 82.30 102.9 8.682 83.23 104.3 1.013

X585 19.7 8.369 82.44 101.5 8.516 82.42 103.3 1.017
X826 9.1 8.083 80.82 100.0 8.245 80.65 102.2 1.022

X5ab 19.7 7.062 91.87 76.9 7.294 91.83 79.4 1.033

X446 9.1 8.548 91.83 93.1 8.622 92.08 93.6 1.005

SDP.81 Band 6

X1716 9.7 0.199 28.52 7.0 0.210 28.58 7.3 1.050

X65f 9.7 0.295 31.07 9.5 0.293 31.09 9.4 0.998

X1f23 1.7 0.386 60.54 6.4 0.389 60.41 6.5 1.009

SDP.81 Band 7

Xb6 9.7 0.261 35.81 7.3 0.262 35.83 7.3 1.005
X517 1.7 0.293 45.85 6.4 0.321 45.47 7.1 1.104

X5e6 9.7 0.248 32.23 7.7 0.244 32.21 7.6 0.984

X1059 9.7 0.271 37.37 7.3 0.271 37.38 7.3 1.000
X1336 9.7 0.271 38.04 7.1 0.275 38.05 7.2 1.011
X1562 9.7 0.323 37.97 8.5 0.324 37.92 8.6 1.003

Xa99 16.1 0.270 48.23 5.6 0.275 48.21 5.7 1.016
Xcc5 16.1 0.281 46.06 6.1 0.274 46.01 6.0 0.983

Notes. Separation column indicates the angular separation between the bandpass target and the source using the casa analysis utilities “aU.angularSeparationOfFields”. The improvement ratio is with respect to the change in S/N. For Juno there are two science target images made, (a) and (b), per EB to account for the rotation of the asteroid. Although both (a) and (b) images are presented separately the average from each EB is used in the main analysis. The () indicates that this Juno EB the calibration is worse with or without WVR scaling. The EBs suffix X12c and Xa47 (SDP.81 B4) have very weak emission such that blends with the noise and image parameters cannot be reported. The noise is measured within the same area for both images with and without WVR scaling applied. The horizontal lines separate the different SBs as noted in Table A.1.

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