Table 1
Source sample.
| Object | α | δ | Sν(3.4) | Sν(1.3) | Other | Sp Type | L∗ | Mass | Age | rms | |
| (J2000) | (J2000) | (mJy) | (mJy) | name | (L⊙) | (M⊙) | (Myr) | (mK) | |||
|
|
|||||||||||
| V1146 Sco | 15:57:20.0 | –23:38:50.0 | M0 | 28 | |||||||
| J1603-1751 | 16:03:23.7 | –17:51:42.3 | M2 | 36 | |||||||
| AS 205A | 16:11:31.4 | –18:38:26.0 | 27.2 | 450 | HBC 254 | K5 | 4.0 | 67 | |||
| SR 4 | 16:25:56.1 | –24:20:48.3 | 4.4 | 31 | AS 206 | K5 | 2.17 | 1.14 | 1.1 | 41 | |
| GSS 26 (⋆) | 16:26:10.3 | –24:20:54.9 | 24.2 | 125 | M0 | 1.39 | 0.56 | 0.5 | 34 | ||
| EL 20 | 16:26:18.9 | –24:28:20.2 | 7.3 | 50 | VSSG 1 | M0 | 0.93 | 0.62 | 1.1 | 54 | |
| LFAM 1 | 16:26:21.7 | –24:22:50.8 | 17.5 | 250 | 37 | ||||||
| DoAr 24E | 16:26:23.4 | –24:21:00.7 | 8.3 | 70 | GSS 31 | 35 | |||||
| DoAr 25 | 16:26:23.7 | –24:43:14.1 | 25.0 | 280 | WSB 29 | K5 | 1.43 | 1.12 | 2.1 | 40 | |
| EL 24 | 16:26:24.1 | –24:16:14.0 | 48.8 | 390 | WSB 31 | K6 | 2.58 | 0.96 | 0.6 | 38 | |
| EL 27 | 16:26:45.0 | –24:23:08.2 | 38.7 | 300 | GSS 39 | M0 | 0.78 | 0.58 | 1.2 | 38 | |
| WL 18 | 16:26:49.0 | –24:38:25.7 | 3.1 | 85 | GY 129 | K7 | 0.3 | 70 | |||
| SR 24S | 16:26:58.5 | –24:45:37.1 | 26.6 | 530 | HBC 262 | K2 | 4.4 | 78 | |||
| SR 21 | 16:27:10.2 | –24:19:12.9 | 4.2 | 95 | EL 30 | G3 | 11.38 | 1.97 | 2.2 | 33 | |
| J1627-2451B | 16:27:15.1 | –24:51:38.8 | M2 | 28 | |||||||
| IRS 41 | 16:27:19.3 | –24:28:44.4 | 6.2 | < 60 | WL 3 | K7 | 1.61 | 0.80 | 0.8 | 50 | |
| CRBR 85 | 16:27:24.7 | –24:41:03.2 | 1.5 | 150 | 1.4 | 22 | |||||
| YLW 16c | 16:27:26.5 | –24:39:23.4 | 6.5 | 60 | GY 262 | M1 | 1.11 | 0.48 | 0.5 | 23 | |
| IRS 49 | 16:27:38.3 | –24:36:58.8 | 4.4 | 25 | GY 308 | M0 | 1.02 | 0.64 | 1.0 | 47 | |
| DoAr 33 | 16:27:39.0 | –23:58:19.1 | 3.7 | 40 | WSB 53 | K4 | 1.81 | 1.44 | 2.9 | 38 | |
| WSB 52 | 16:27:39.5 | –24:39:15.9 | 10.2 | 51 | GY 314 | K5 | 0.95 | 1.04 | 4.2 | 41 | |
| IRS 51 | 16:27:39.8 | –24:43:15.0 | 12.7 | 110 | GY 315 | 83 | |||||
| Flying Saucer(⋆) | 16:28:13.7 | –24:31:39.1 | 3 | M1 | 0.14 | 40 | |||||
| WSB 60 | 16:28:16.5 | –24:36:58.0 | 15.3 | 89 | YLW 58 | M4 | 0.23 | 0.20 | 0.9 | 31 | |
| SR 13 | 16:28:45.3 | –24:28:19.2 | 10.0 | 60 | HBC 266 | 37 | |||||
| DoAr 44 | 16:31:33.5 | –24:27:37.7 | 10.4 | 105 | HBC 268 | K3 | 1.55 | 1.29 | 5.1 | 38 | |
| RNO 90 | 16:34:09.2 | –15:48:16.9 | 7.6 | 25 | HBC 649 | G5 | 10.24 | 1.87 | 2.3 | 31 | |
| Wa Oph 6 | 16:48:45.6 | –14:16:36.0 | 10.3 | 130 | HBC 653 | K6 | 2.32 | 0.98 | 0.7 | 26 | |
| AS 209 (⋆) | 16:49:15.3 | –14:22:08.6 | 17.5 | 300 | HBC 270 | K5 | 2.11 | 1.18 | 1.2 | 24 | |
| HD 163296 (⋆) | 17:56:21.3 | –21:57:22.0 | A1 | 2.25 | 5.0 | 50 | |||||
Notes. Sources in upper Scorpius are listed in italics. Sources marked with (⋆) are the sources for which CN emission from disk has been detected. The epoch 2000 coordinates are adopted from SIMBAD. Sν is the continuum flux at 3.4 mm and 1.3 mm. Spectral types and luminosities (given for ~130 pc) are taken from Ricci et al. (2010) except for AS 205A (Bast et al. 2011), WL 18 (Andrews et al. 2010), SR 24S (Andrews et al. 2010), CRBR 85 (Pontoppidan et al. 2005), and the Flying Saucer (Grosso et al. 2003). Masses and ages are derived from the tracks reported in Palla & Stahler (1999) using the luminosities and effective temperatures from Ricci et al. (2010).
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