Table D.2
Estimated masses of our MASSIVE targets, using their absolute magnitudes and the BT-Settl models (Allard et al. 2012).
| ID | Mass |
| (MJup) | |
|
|
|
| 2MASS J00243202–2522528 | 450 |
| 2MASS J00251465–6130483 | 700 |
| 2MASS J00255097–0957398 | 400 |
| 2MASS J00452814–5137339 | 700 |
| 2MASS J01033563–5515561 | 450 |
| 2MASS J01231125–6921379 | 65 |
| 2MASS J01365516–0647379 | 110 |
| 2MASS J01521830–5950168 | 500 |
| 2MASS J02224418–6022476 | 400 |
| 2MASS J02365171–5203036 | 400 |
| 2MASS J03350208+2342356 | 50 |
| 2MASS J03363144–2619578 | 230 |
| 2MASS J03472333–0158195 | 450 |
| 2MASS J04141730–0906544 | 310 |
| 2MASS J04373746–0229282 | 820 |
| 2MASS J04433761+0002051 | 20 |
| 2MASS J04464970–6034109 | 620 |
| 2MASS J04522441–1649219 | 500 |
| 2MASS J04533054–5551318 | 350 |
| 2MASS J04593483+0147007 | 750 |
| 2MASS J05004714–5715255 | 800 |
| 2MASS J05064991–2135091 | 570 |
| 2MASS J05195412–0723359 | 150 |
| 2MASS J06085283–2753583 | 12* |
| 2MASS J06255610–6003273 | 570 |
| 2MASS J07285117–3015527 | 250 |
| 2MASS J08173943–8243298 | 650 |
| 2MASS J10284580–2830374 | 90 |
| 2MASS J10285555+0050275 | 450 |
| 2MASS J11020983–3430355 | 250 |
| 2MASS J11210549–3845163 | 570 |
| 2MASS J11393382–3040002 | 150 |
| 2MASS J11395113–3159214 | 15 |
| 2MASS J12072738–3247002 | 500 |
| 2MASS J12073346–3932539 | 20 |
| 2MASS J12153072–3948426 | 700 |
| 2MASS J12265135–3316124 | 350 |
| 2MASS J13215631–1052098 | 182 |
| 2MASS J15385757–5742273 | 175 |
| 2MASS J16334161–0933116 | 600 |
| FS2003 0979 | 300 |
| 2MASS J18465255–6210366 | 750 |
| 2MASS J19560294–3207186 | 820 |
| 2MASS J19560438–3207376 | 750 |
| 2MASS J20333759–2556521 | 350 |
| 2MASS J20450949–3120266 | 620 |
| 2MASS J20450949–3120266 | 620 |
| 2MASS J21100535–1919573 | 600 |
| 2MASS J21443012–6058389 | 620 |
| 2MASS J22445794–3315015 | 450 |
| 2MASS J22450004–3315258 | 250 |
| 2MASS J23301341–2023271 | 500 |
| 2MASS J23323085–1215513 | 700 |
| 2MASS J23381743–4131037 | 450 |
Notes.
The association of this star (BPMG, Riedel et al. 2014; and Malo et al. 2013) were debated by Gagné et al. (2014b) who show that this target could be a member to the Columba association, but other radial velocity measurements are still needed to confirmed this. The mass of this object is quite low here, and is more certainly around 15−24 MJup, as reported by Riedel et al. (2014) and Gagné et al. (2014b). We however kept this low mass in order to have a consistent determination of all the stellar masses.
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