Table 1
Herschel/PACS fluxes for the detected brown dwarfs in ρ Ophiuchi.
| Identifier | RA | Dec | SpT | A V | Ref. | 70 μm | 100 μm | 160 μm |
| (mag) | (mJy) | (mJy) | (mJy) | |||||
|
|
||||||||
| GY92 154 | 16:26:54.79 | −24:27:02.1 | M6 | 20.1 | 1, 4, 8 | 87.5 ± 10.3 | 172.8 ± 32.8 | 399.6 ± 246.4 |
| GY92 171 | 16:26:58.41 | −24:21:30.0 | M6 | 6.6 | 1, 4, 8 | 41.2 ± 10.5 | 53.6 ± 34.8 | <189.0 |
| GY92 204 a | 16:27:06.60 | −24:41:48.8 | M6(M5.5) | 0.5 | 1, 4, 5, 6 | 80.1 ± 5.6 | 48.4 ± 19.1 | <115.2 |
| ISO-Oph 160 | 16:27:37.42 | −24:17:54.9 | M6 | 6.0 | 4, 5 | 38.8 ± 7.6 | 61.9 ± 20.5 | <93.8 |
| GY92 344 | 16:27:45.78 | −24:44:53.6 | M6 | 16.2 | 1, 4, 8 | 727.3 ± 4.4 | 1338.8 ± 12.8 | 2675.6 ± 87.4 |
| GY92 371 | 16:27:49.77 | −24:25:22.2 | M6 | 5.4 | 1, 4, 8 | 42.5 ± 6.3 | 68.4 ± 19.8 | <139.7 |
| GY92 397 | 16:27:55.24 | −24:28:39.7 | M6 | 5.0 | 1, 4, 8 | 64.5 ± 6.1 | 74.7 ± 18.4 | <103.4 |
| ISO-Oph 193 | 16:28:12.72 | −24:11:35.6 | M6 | 7.5 | 4, 5 | 43.2 ± 4.6 | 38.6 ± 11.8 | 63.2 ± 58.8 |
| CFHTWIR−Oph 66 | 16:27:14.34 | −24:31:32.0 | M7.75 | 15.1 | 7, 9 | 46.2 ± 9.6 | 51.6 ± 28.2 | <201.0 |
| GY92 3 | 16:26:21.90 | −24:44:39.8 | M8(M7.5) | 0.0 | 1, 4, 5, 6 | 45.6 ± 6.1 | <27.2 | <65.7 |
| GY92 264 | 16:27:26.58 | −24:25:54.4 | M8 | 0.0 | 1, 6 | 26.1 ± 8.6 | 64.1 ± 28.4 | <158.3 |
| GY92 310 | 16:27:38.63 | −24:38:39.2 | M8.5(M7,M6) | 5.7 | 1, 2, 3, 4, 5 | 93.8 ± 5.5 | 80.8 ± 15.8 | <119.4 |
Notes. Upper limits for non-detections are listed in Table A.1.
GY92 204 corresponds to ISO−Oph 102 observed with ALMA by Ricci et al. (2012).
Reference. (1) Greene & Young (1992); (2) Wilking et al. (1999); (3) Luhman & Rieke (1999); (4) Bontemps et al. (2001); (5) Natta et al. (2002); (6) Wilking et al. (2005); (7) Alves de Oliveira et al. (2010); (8) McClure et al. (2010); (9) Alves de Oliveira et al. (2012).
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