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Table 1
Description of columns in the catalogue of the final sample available at the CDS.
Column number | Column name | Description |
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1 | COUP_no | COUP identification number |
2 | RA | RA from the COUP catalogue |
3 | Dec | Dec from the COUP catalogue |
4 | NH | NH from the COUP catalogue [cm-2] |
5 | NH_err | 1σ error of NH as assumed in this work [cm-2] |
6 | VISION_no | VISION identification number |
7 | J | J magnitude from VISION [mag] |
8 | J_err | 1σ error of J magnitude from VISION [mag] |
9 | H | H magnitude from VISION [mag] |
10 | H_err | 1σ error of H magnitude from VISION [mag] |
11 | Ks | Ks magnitude from VISION [mag] |
12 | Ks_err | 1σ error of Ks magnitude from VISION [mag] |
13 | sptype | Spectral type as deduced from Hillenbrand et al. (2013) |
14 | JH0 | Intrinsic (J − H) magnitude as deduced from Scandariato et al. (2012) [mag] |
15 | JH0_err | 1σ error of intrinsic (J − H) magnitude [mag] |
16 | HK0 | Intrinsic (H − Ks) magnitude as deduced from Scandariato et al. (2012) [mag] |
17 | HK0_err | 1σ error of intrinsic (H − Ks) magnitude [mag] |
18 | AV | AV for RV = 3.1a as deduced in this work [mag] |
19 | AV_err | 1σ error of AV for RV = 3.1 as deduced in this work [mag] |
20 | class | Classification (p – protostar, d – disc star, cl3 – Class III source, uncl – unclassified) |
Notes.
(a)
AV for RV = 5.5 can be calculated by multiplication with the factor 1.18 (see Sect. 4.2.2).
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