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Table 1

Target list with integrated fluxes and distances.

Target RA Dec M (a) L (a) log Lacc (a) FC_2H F890μm (b) (b) d (c)
[J2000] [J2000] [M] [L] [L] [mJy km s−1] [mJy] [mJy km s−1] [pc]
Sz 98 16:08:22.481 −39:04:46.812 0.67 1.53 −0.71 1101 ± 57 237.29 ± 0.51 506 ± 120 156.2
Sz 71 15:46:44.716 −34:30:36.057 0.41 0.33 −2.17 1101 ± 46 166.04 ± 0.37 1298 ± 107 155.9
J16070854-3914075 16:07:08.539 −39:14:07.885 647 ± 55 92.07 ± 0.49 1232 ± 173 175.8
Sz 114 16:09:01.836 −39:05:12.790 0.19 0.21 −2.68 383 ± 32 96.41 ± 0.50 716 ± 50 162.2
MY Lup 16:00:44.503 −41:55:31.271 1.09 0.85 −1.00 284 ± 21 176.81 ± 0.56 874 ± 54 156.6
J16090141-3925119 16:09:01.405 −39:25:12.345 0.2 0.07 −1.5 200 ± 46 17.50 ± 0.68 1637 ± 89 164.3
Sz 129 15:59:16.458 −41:57:10.662 0.78 0.43 −1.13 107 ± 16 181.12 ± 0.52 636 ± 80 161.7
J16070384-3911113 16:07:03.825 −39:11:11.756 0.003 −5.40 <16.1(d) 4.52 ± 0.55 1242 ± 98 150.0
Sz 68 15:45:12.848 −34:17:30.986 5.42 1.18 <5.3(d) 150.37 ± 0.46 915 ± 131 154.2

Notes. (a) Stellar properties corrected after Gaia DR2 (Alcalá et al. 2019). (b)Ansdell et al. (2016). (c)Distance measured by Gaia (Gaia Collaboration 2018). Typical errors on the distance are 1–2% of the measured distance for these sources. (d) 3σ upper limits.

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