Table A.1
Data available in the literature for the targets included in this work.
| Object/other name | RA(2000) | Dec(2000) | SpT | AV | References | McClure et al. (2010) | |
| h:m:s | ° ’ ” | [mag] | classification | ||||
|
|
|||||||
| ISO−Oph023/SKS1/CRBR 2317.3-1925 | 16:26:18.821 | −24:26:10.52 | M7.5, M5.5, M7 | 10.0 | 1, 2, 3 | Disk | |
| ISO−Oph030/GY5 | 16:26:21.528 | −24:26:00.96 | M5.5, M6, M6 | 2.8 | 4, 1, 3 | Disk | |
| ISO−Oph032/GY3 | 16:26:21.899 | −24:44:39.76 | M8, M7.5 | 0.0 | 4, 3 | ... | |
| ISO−Oph033/GY11 | 16:26:22.269 | −24:24:07.06 | M8.5, M6.5, M8.5 | 8.0 | 5, 1, 3 | ... | |
| ISO−Oph037/LFAM3/GY21 | 16:26:23.580 | −24:24:39.50 | M0, K5 | 16.1 | 7, 6 | Disk/FS | |
| ISO−Oph072/WL18 | 16:26:48.980 | −24:38:25.24 | K6.5 | 10.4 | 4 | Disk | |
| ISO−Oph087 | 16:26:58.639 | −24:18:34.66 | ... | ... | ... | ... | |
| ISO−Oph094 | 16:27:03.591 | −24:20:05.45 | M3? | 20.1 | 8 | ... | |
| ISO−Oph102/GY204 | 16:27:06.596 | −24:41:48.84 | M5.5, M6 | 0.5 | 4, 3 | Disk | |
| ISO−Oph115/WL11/GY229 | 16:27:12.131 | −24:34:49.14 | M0, M0 | 11.5 | 7, 6 | Disk | |
| ISO−Oph117/WLY2-32b/GY235 | 16:27:13.823 | −24:43:31.66 | M5, K8 | 7.5 | 7, 6 | Disk/FS | |
| ISO−Oph123 | 16:27:17.590 | −24:05:13.70 | M3.5 | 4.4 | 4 | ... | |
| ISO−Oph160/B162737-241756 | 16:27:37.422 | −24:17:54.87 | M6 | 6.0 | 3 | ... | |
| ISO−Oph164/GY310 | 16:27:38.631 | −24:38:39.19 | M8.5, M7, M6 | 5.7 | 1, 2, 3 | Disk | |
| ISO−Oph165/GY312 | 16:27:38.945 | −24:40:20.67 | M2 | 15.0 | 7 | Envelope/I | |
| ISO−Oph176/GY350 | 16:27:46.291 | −24:31:41.19 | M6, M6 | 7.0 | 3, 7 | Disk | |
| ISO−Oph193/B162812-241138 | 16:28:12.720 | −24:11:35.60 | M6 | 7.5 | 3 | ... | |
Notes. Spectral types, extinction, and mass accretion rates determined from the following studies: 1) Wilking et al. (1999); 2) Luhman & Rieke (1999); 3) Natta et al. (2002); 4) Wilking et al. (2005); 5) Comerón et al. (2010); 6) Gatti et al. (2006), 7) McClure et al. (2010, and references therein), 8) Alves de Oliveira et al. (2012).
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