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Table A.2

Masses of the embedded disks in Perseus.

Source name Class Mdust at 9 mm Mdust at 1 mm α α Robust Dataset
M M VLA/ALMA VLA
Per-emb-1 0 279.6 ± 50.0 82.5 ± 1.2 2.4 1.9 n Segura-Cox
Per-emb-2 0 927.4 ± 175.6 573.6 ± 18.2 2.8 2.9 y Hsieh
Per-emb-3 0 157.8 ± 32.7 51.2 ± 0.4 2.4 1.5 n Hsieh
Per-emb-4 0 <11.3 ± 7.2 0.5 ± 0.1 1.5 n Hsieh
Per-emb-5 0 502.3 ± 86.3 267.6 ± 2.1 2.7 2.7 y Hsieh
Per-emb-6 0 78.5 ± 21.5 11.0 ± 0.2 2.0 1.7 y Hsieh
Per-emb-7 0 <11.8 ± 7.2 2.4 ± 0.4 2.2 n Hsieh
Per-emb-8 0 237.9 ± 47.5 147.6 ± 5.5 2.7 3.0 y Tobin
Per-emb-9 0 23.1 ± 14.4 9.7 ± 0.4 2.6 3.3 n Hsieh
Per-emb-10 0 143.4 ± 30.7 21.7 ± 0.3 2.1 1.5 n Hsieh
Per-emb-11-A 0 413.5 ± 73.1 230.2 ± 1.6 2.7 2.4 y Segura-Cox
Per-emb-11-B 0 21.7 ± 14.9 7.4 ± 1.1 2.4 1.7 n Segura-Cox
Per-emb-11-C 0 30.5 ± 15.4 5.1 ± 0.4 2.1 3.2 n Segura-Cox
Per-emb-12-A 0 2853.9 ± 437.0 2159.5 ± 59.3 2.8 3.0 y Tobin
Per-emb-12-B 0 158.1 ± 38.4 623.6 ± 16.0 3.7 3.2 n Tobin
Per-emb-13 0 1271.3 ± 207.6 2.7 n
Per-emb-14 0 311.2 ± 58.6 95.5 ± 0.9 2.4 2.4 y Hsieh
Per-emb-15 0 <9.3 ± 6.6 6.3 ± 0.4 2.8 n Hsieh
Per-emb-16 0 <34.9 ± 18.1 n
Per-emb-17-A 0 160.1 ± 32.4 37.5 ± 1.0 2.2 1.9 y Tobin
Per-emb-17-B 0 39.3 ± 10.4 29.3 ± 1.0 2.8 2.6 y Tobin
Per-emb-18 0 224.8 ± 47.1 208.5 ± 2.8 2.9 1.5 n Tobin
Per-emb-19 0 112.3 ± 27.7 17.1 ± 0.2 2.1 1.1 n Hsieh
Per-emb-20 0 <31.1 ± 15.5 7.8 ± 0.4 2.3 n Hsieh
Per-emb-21 0 211.9 ± 41.1 70.8 ± 1.0 2.4 2.5 y Tobin
Per-emb-22-A 0 96.4 ± 24.1 47.3 ± 1.5 2.6 1.0 n Hsieh
Per-emb-22-B 0 23.1 ± 13.0 23.9 ± 1.5 3.0 3.4 n Hsieh
Per-emb-23 0 37.2 ± 15.0 3.8 n
Per-emb-24 0 21.5 ± 7.9 3.8 ± 0.3 2.2 3.0 n Hsieh
Per-emb-25 0 172.6 ± 65.4 122.4 ± 1.1 2.8 1.7 n Hsieh
Per-emb-26 0 636.1 ± 102.5 2.2 n
Per-emb-27-A 0 570.1 ± 90.4 215.0 ± 5.1 2.5 1.9 n Hsieh
Per-emb-27-B 0 113.6 ± 24.4 22.5 ± 4.8 2.2 1.9 y Hsieh
Per-emb-28 0/I 23.5 ± 16.6 4.4 n
Per-emb-29 0/I 233.5 ± 43.5 123.3 ± 2.4 2.7 1.8 n Hsieh
Per-emb-30 0/I 263.5 ± 47.7 46.8 ± 0.4 2.2 2.1 y Hsieh
Per-emb-31 0/I <26.5 ± 14.9 1.1 ± 0.2 1.5 n Hsieh
Per-emb-32-A 0/I 18.2 ± 8.1 0.9 n
Per-emb-32-B 0/I 30.0 ± 10.5 3.6 n
Per-emb-33-A 0 294.0 ± 57.6 9.3 ± 1.6 1.2 2.3 n Tobin
Per-emb-33-B 0 170.6 ± 39.4 45.8 ± 2.8 2.3 1.2 n Tobin
Per-emb-33-C 0 55.8 ± 19.0 234.1 ± 3.7 3.7 2.0 n Tobin
Per-emb-34 I 85.6 ± 22.5 12.0 ± 0.3 2.0 1.2 n Hsieh
Per-emb-35-B I 86.8 ± 20.6 19.3 ± 0.4 2.3 1.3 n Hsieh
Per-emb-35-A I 47.0 ± 15.7 26.8 ± 0.4 2.7 3.2 n Hsieh
Per-emb-36-A I 555.9 ± 90.4 185.5 ± 1.8 2.4 2.5 y Tobin
Per-emb-36-B I 110.6 ± 23.3 17.7 ± 1.4 2.0 2.2 y Tobin
Per-emb-37 0 95.4 ± 23.9 1.7 n
Per-emb-38 I 78.7 ± 23.6 26.7 ± 0.3 2.5 1.9 n Hsieh
Per-emb-39 I <12.3 ± 7.3 0.8 ± 0.2 1.7 n Hsieh
Per-emb-40-A I 72.9 ± 18.0 22.8 ± 0.6 2.4 2.3 y Tobin
Per-emb-40-B I <17.6 ± 8.7 1.3 ± 0.2 1.7 n Tobin
Per-emb-41 I 44.2 ± 18.8 11.0 ± 0.3 2.3 0.9 n Hsieh
Per-emb-42 I 116.5 ± 29.0 1.7 n
Per-emb-43 I <11.8 ± 7.2 n
Per-emb-44-A 0/I 497.7 ± 80.8 142.2 ± 2.2 2.3 2.3 y Tobin
Per-emb-44-B 0/I 176.7 ± 41.7 227.1 ± 3.7 3.1 1.7 n Tobin
Per-emb-45 I <11.8 ± 7.2 1.0 ± 0.2 1.8 n Hsieh
Per-emb-46 I 55.5 ± 26.6 5.8 ± 0.3 1.9 0.8 n Hsieh
Per-emb-47 I 106.5 ± 28.3 2.2 n
Per-emb-48-A I 37.9 ± 16.5 5.7 ± 0.8 2.0 0.7 n Tobin
Per-emb-48-B I <14.9 ± 10.5 <0.6 ± 0.8 1.3 n Tobin
Per-emb-49-A I 145.2 ± 31.0 21.4 ± 0.3 2.1 0.6 n Hsieh
Per-emb-49-B I <53.0 ± 16.5 4.5 ± 0.3 1.8 n Hsieh
Per-emb-50 I 535.2 ± 91.0 124.1 ± 0.4 2.2 2.1 y Segura-Cox
Per-emb-51 I <12.8 ± 8.1 1.6 ± 0.8 2.0 n Hsieh
Per-emb-52 I 35.4 ± 19.6 5.0 ± 0.3 2.0 1.0 n Hsieh
Per-emb-53 I 56.6 ± 22.6 42.3 ± 0.8 2.8 1.1 n Segura-Cox
Per-emb-54 I 115.5 ± 28.2 3.0 ± 0.9 1.2 1.0 y Hsieh
Per-emb-55-A I 48.7 ± 11.8 4.7 ± 1.0 1.8 3.6 n Tobin
Per-emb-55-B I 7.4 ± 5.2 0.7 ± 0.6 1.8 4.4 n Tobin
Per-emb-56 I 45.7 ± 16.9 3.7 n
Per-emb-57 I 67.9 ± 22.8 0.6 n
Per-emb-58 I <37.9 ± 17.9 4.4 ± 0.2 2.0 n Hsieh
Per-emb-59 I <13.8 ± 8.2 1.5 ± 0.2 1.9 n Hsieh
Per-emb-60 I <13.3 ± 8.1 n
Per-emb-61 I 52.1 ± 23.4 2.6 n
Per-emb-62 I 200.8 ± 41.6 110.5 ± 0.2 2.7 2.2 n Segura-Cox
Per-emb-63-B I <11.8 ± 8.3 3.6 ± 0.3 2.4 n Hsieh
Per-emb-63-C I <11.8 ± 8.3 2.1 ± 0.2 2.2 n Hsieh
Per-emb-63-A I 109.7 ± 27.3 24.9 ± 0.3 2.3 2.0 y Hsieh
Per-emb-64 I 240.9 ± 48.0 40.9 ± 0.4 2.1 1.8 y Hsieh
Per-emb-65 I 58.5 ± 25.0 35.9 ± 0.3 2.8 1.1 n Hsieh
Per-emb-66 I <13.3 ± 8.1 n
Per-bolo-58 0 <12.8 ± 8.1 n
Per-bolo-45 0 <12.3 ± 7.3 n
L1451-MMS 0 97.3 ± 22.8 2.2 n
L1448IRS2E 0 <14.7 ± 9.0 n
B1-bN 0 483.8 ± 85.1 2.5 n
B1-bS 0 354.0 ± 76.5 319.4 ± 3.5 2.9 2.1 n Hsieh
L1448IRS1-A I 292.7 ± 53.2 105.4 ± 1.8 2.5 2.2 y Tobin
L1448IRS1-B I 36.4 ± 15.6 7.9 ± 1.4 2.2 3.7 n Tobin
L1448NW-A 0 194.5 ± 38.6 71.5 ± 1.0 2.5 1.7 n Tobin
L1448NW-B 0 187.9 ± 39.1 21.3 ± 0.4 1.9 1.7 y Tobin
L1448IRS3A I 235.1 ± 47.8 145.0 ± 5.1 2.7 0.7 n Tobin
SVS13C 0 223.9 ± 48.4 89.3 ± 1.9 2.5 1.4 n Segura-Cox
SVS13B 0 581.1 ± 98.2 200.3 ± 8.1 2.5 2.3 y Hsieh
IRAS03363+3207 I? 326.3 ± 58.0 2.4 n
IRAS4B’ 0 603.2 ± 115.2 2.6 n
SVS13A2 0? 102.6 ± 27.7 18.2 ± 5.2 2.2 1.4 n Hsieh

Notes. Class – evolutionary class of the source. In the analysis, borderline sources (0/I) are treated as Class 0. Dataset: Tobin – (Tobin et al. 2018) (1.3 mm), Segura-Cox – 2017.1.01078.S (1.3 mm), Hsieh – (Hsieh et al. 2019b) (1.1 mm). αVLA/ALMA – spectral indices obtained between 1 and 9 mm, αVLA - Ka-band intraband indices. Robust – if “y”, sources with consistent spectral indices betweem VLA/ALMA and VLA Ka-band.

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