Name | Spectral | Binarity | Selection | Observed in | Bolometer | Publication |
criterium | survey # | arrays | ||||
GJ82 | M4 | Single | 20-150 Myr | I | SCUBA | Lestrade et al. (2006) |
GJ212 | M0.5 | '' | '' | I | '' | '' |
GJ507.1 | M1.5 | '' | '' | I | '' | '' |
GJ696 | M0 | '' | '' | I | '' | '' |
GJ876 | M4 | '' | '' | I | MAMBO | '' |
GJ628 | M3.5 | '' | '' | I | '' | '' |
GJ402 | M4 | '' | '' | I | '' | '' |
GJ234 | M4.5+M8 | Binary | '' | I & II | '' | Lestrade et al. (2006) and this work |
GJ285 | M4.5 | Single | '' | I | SCUBA & MAMBO | Lestrade et al. (2006) |
GJ393 | M2 | '' | '' | I | '' | '' |
GJ9809 | M0 | '' | '' | I | '' | '' |
GJ875.1 | M3 | '' | 35-55 Myr | I | SCUBA | '' |
GJ856A | M3 | '' | 100-125 Myr | I | MAMBO | '' |
GJ277B | M3.5 | '' | 200 Myr | I | SCUBA | '' |
GJ842.2 | M0.5 | '' | '' | I | '' | '' |
GJ890 | M2 | '' | '' | I | '' | '' |
GJ1111 | M6.5 | '' | '' | I & II | MAMBO | Lestrade et al. (2006) and this work |
GJ408 | M2.5 | '' | '' | I & II | '' | '' |
GJ4247 | M4 | '' | '' | I & II | SCUBA & MAMBO | '' |
GJ447 | M4.0 | '' | 500 Myr | I & II | MAMBO | '' |
GJ625 | M1.5 | '' | '' | I & II | '' | '' |
GJ569 | M2.5+M8.5 | Binary | '' | I & II | '' | '' |
GJ873 |
M3.5 | Single | '' | I | '' | Lestrade et al. (2006) |
GJ65 | M5.5+M5.5 | Binary | 600 Myr | I | '' | '' |
GJ3379 | M4 | Single | '' | I | '' | '' |
GJ849 | M3.5 | '' | '' | I | '' | '' |
GJ791.2 | M4.5 | '' | '' | I | '' | '' |
GJ109 | M3.5 | '' | '' | I & II | '' | Lestrade et al. (2006) and this work |
GJ699 | M4.0 | Single | 1.82 pc | II | MAMBO | this work |
GJ406 | M6.0 | '' | 2.38 pc | II | '' | '' |
GJ411 | M2.0 | '' | 2.54 pc | II | '' | '' |
GJ905 | M5.5 | '' | 3.16 pc | II | '' | '' |
GJ725 | M3+M3.5 | Binary | 3.57 pc | II | '' | '' |
GJ54.1 | M4.5 | Single | 3.72 pc | II | '' | '' |
GJ273 | M3.5 | '' | 3.79 pc | II | '' | '' |
GJ83.1 | M4.5 | '' | 4.44 pc | II | '' | '' |
GJ687 | M3.0 | '' | 4.53 pc | II | '' | '' |
LHS292 | M6.5 | '' | 4.54 pc | II | '' | '' |
GJ1002 | M5.5 | '' | 4.69 pc | II | '' | '' |
GJ412 | M2+M6 | Binary | 4.83 pc | II | '' | '' |
GJ388 | M3.0 | Single | 4.89 pc | II | '' | '' |
GJ445 | M3.5 | '' | 5.38 pc | II | '' | '' |
LHS1723 | M4.5 | '' | 5.43 pc | II | '' | '' |
GJ526 | M1.5 | '' | 5.43 pc | II | '' | '' |
GJ251 | M3.0 | '' | 5.57 pc | II | '' | '' |
GJ205 | M1.5 | '' | 5.71 pc | II | '' | '' |
GJ213 | M4.0 | '' | 5.87 pc | II | '' | '' |
GJ908 | M1.0 | '' | 5.93 pc | II | '' | '' |
GJ581 | M3 | '' | 6.27 pc | II | '' | '' |
GJ102 | M4 | '' | 7.75 pc | II | '' | '' |
Survey I was presented in Lestrade et al. (2006) and its data are included in the statistical analysis of the present paper. Survey II is based on new data with MAMBO-2 presented in the present paper. Selection criteria are ages <600 Myr for survey I and the nearest M-dwarfs but of undetermined ages for survey II. Ages are based on Moving Groups (Local Association (20-150 Myr), IC 2391 (35-55 Myr), AB Dor (100-125 Myr), Castor (200 Myr), Ursa Maj (500 Myr) and Hyades (600 Myr)) identified by Montes et al. (2001) and Zuckerman & Inseok Song (2004a,b). Some stars were observed in both surveys.
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