Table A.3
Sub-mm and mm photometry for a sub-sample of stars.
| Star | F(1.3 mm) | F(λ) | Ref. |
| (mJy) | (mJy)((mm)) | ||
|
|
|||
| HD 31648 | 360 ± 24 | 3300(0.45); 780(0.85); 235(1.4); 39.9(2.7); 35.2(2.8) | (1, 2, 3) |
| HD 34282 | 110 ± 10 | 2700(0.45); 409(0.80); 360(0.85); 183(1.1); 24(2.6); 5.0(3.4) | (4, 5, 6) |
| HD 34700 | 11.7 ± 1.1∗ | 218(0.45); 41(0.85); 39(1.1) | (6, 7, 8) |
| HD 141569 | 9.0 ± 4.0 | 65(0.45); 11(0.85) | (5, 9) |
| HD 142666 | 127 ± 9 | 1090(0.45); 351(0.80); 180(1.1); < 63(2.0) | (6) |
| HD 144432 | 37 ± 3 | 103(0.80); 129(0.85); 69(1.1) | (5. 6. 9) |
| HD150193 | 45 ± 4.5 | 101(0.85) | (5, 10) |
| HD163296 | 780 ± 31 | 10660(0.35); 5560(0.45); 3380(0.60); 2650(0.75); 2320(0.80); 1920(0.85); 1020(1.1) | (11) |
| HD 179218 | 71 ± 7 | 7.6(2.6) | (12) |
| VX Cas | < 6 | ... | (13) |
| SV Cep | 7 ± 2 | ... | (13) |
| V1686Cyg | < 4.8∗ | ... | (14) |
| R Mon | 100 ± 10 | 1980(0.35); 1560(0.45); 217(0.80); 77(1.1); 1.17(20); 0.37(36); 0.29(60) | (11, 15, 16) |
| VY Mon | 120 ± 12 | 18000(0.37); 1.5(60) | (10, 17) |
| KK Oph | 52 ± 5.2 | 109(0.80); 36(1.1); 0.24(36) | (5, 16) |
| T Ori | 130 ± 28 | ... | (15) |
| BF Ori | 6 ± 2 | ... | (13) |
| CO Ori | < 4.0 | ... | (13) |
| HK Ori | < 100 | ... | (15) |
| UX Ori | 23 ± 2 | 3.8(2.6); 0.8(7.0) | (13, 18, 19) |
| VV Ser | < 20 | ... | (15) |
| CQ Tau | 143 ± 8.4 | 2.6(7.0) | (12, 19) |
| RR Tau | < 20 | ... | (15) |
| RY Tau | 212 ± 21∗ | 2439(0.35); 1920(0.45); 560(0.85) | (20, 21) |
| WW Vul | 10.5 ± 1.0 | ... | (13) |
| LkHa 234 | 827 ± 82.7∗ | 60000(0.45); 4200(0.80); 3400(0.85); 2.67(20); 1.82(36); 1.65(60) | (16) |
Notes. The second column shows the fluxes used to compute the disk masses in Table 1. Those tagged with ∗ were measured at 1.35 mm (HD 34700), 2.70 mm (V1686 Cyg) and 1.20 mm (RY Tau and LkHa 234). An uncertainty of 10% is assigned when that is not provided in the reference.
References. (1): Mannings & Sargent (1997), (2): Sandell & Weintraub (2002), (3): Piétu et al. (2006), (4): Piétu et al. (2003), (5): Sandell et al. (2011), (6): Sylvester et al. (1996), (7): Sylvester et al. (2001), (8): Sheret et al. (2004), (9): Walker & Butner (1995), (10): Alonso-Albi et al. (2009), (11): Mannings (1994), (12): Mannings & Sargent (2000), (13): Natta et al. (1997), (14): Natta et al. (2000), (15): Hillenbrand et al. (1992), (16): Pezzuto & Strafella (1997), (17): Casey & Harper (1990), (18): Acke & van den Ancker (2006), (19): Testi et al. (2001), (20): Robitaille et al. (2007), (21): Altenhoff et al. (1994).
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