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Table 3:

Individual spectral types and projected separations.

2MASS ID 		Primary Secondary Separation
  SpT SpT [AU]
J00150240-7250326 M 0.5 M 3.5 11.0 $\pm$ 4.1
J00250428-3646176 M 2.5 M 5.0 16.9 $\pm$ 6.3
J00503319+2449009 M 3.5 M 4.5 15.7 $\pm$ 1.3
J01071194-1935359 M 0.5 M 2.5 12.5 $\pm$ 4.6
J01093874-0710497 M 1.0 M 4.0 97.1 $\pm$ 13.0
J01132817-3821024 M 0.0 M 1.0 52.0 $\pm$ 19.2
J01365516-0647379 M 4.0 >L0 206.7 $\pm$ 76.5
J01452133-3957204a K7.5 M 3.5 30.2 $\pm$ 2.2
J01535076-1459503 M 3.0 M 3.0 51.8 $\pm$ 19.2
J02002975-0239579 M 3.5 M 4.5 15.5 $\pm$ 5.7
J02133021-4654505 M 4.0 M 5.0 1.8 $\pm$ 0.7
J02155892-0929121AB M 2.5 M 5.0 16.4 $\pm$ 6.1
J02155892-0929121AC M 2.5 M 8.0 91.2 $\pm$ 33.8
J02165488-2322133 M 3.5 M 4.5 174.8 $\pm$ 64.7
J02271603-2929263 M 3.5 M 5.0 98.9 $\pm$ 36.6
J02335984-1811525 M 3.0 M 3.5 42.7 $\pm$ 15.8
J02411909-5725185 M 2.5 M 4.0 68.7 $\pm$ 25.4
J02451431-4344102 M 4.0 M 4.5 1.8 $\pm$ 0.7
J02490228-1029220AB M 1.5 M 3.5 16.4 $\pm$ 6.1
J02490228-1029220AC M 1.5 M 3.5 21.2 $\pm$ 7.8
J03033668-2535329 M 0.0 M 6.0 32.5 $\pm$ 2.8
J03050976-3725058 M 1.5 M 3.0 10.9 $\pm$ 4.0
J04071148-2918342a K7.5 M 1.0 15.1 $\pm$ 5.6
J04080543-2731349 M 3.5 M 4.5 7.8 $\pm$ 2.9
J04132663-0139211 M 4.0 M 4.0 9.3 $\pm$ 3.4
J04373746-0229282a,c K7.5 M 3.0 5.1 $\pm$ 1.9
J04441107-7019247 M 1.0 M 2.5 50.4 $\pm$ 18.7
J05241914-1601153 M 4.5 M 5.0 5.1 $\pm$ 1.9
J05254166-0909123 M 3.5 M 4.0 13.6 $\pm$ 5.0
J06161032-1320422 M 3.5 M 5.0 6.0 $\pm$ 2.2
J06583980-2021526AB M 4.0 M 4.0 45.4 $\pm$ 16.8
J06583980-2021526ACb M 4.0 >L0 223.7 $\pm$ 82.8
J06583980-2021526AD M 4.0 >L0 164.8 $\pm$ 61.0
J07102991-1637350AB M 2.5 M 3.0 27.8 $\pm$ 10.3
J07102991-1637350AC M 2.5 M 9.0 99.0 $\pm$ 36.6
J07105990-5632596 M 1.5 M 4.5 58.2 $\pm$ 21.6
J07174710-2558554c M 2.0 >L0 250.6 $\pm$ 92.7
J07285137-3014490 M 1.0 M 3.0 7.8 $\pm$ 0.3
J08224744-5726530AB M 4.5 >L0 5.2 $\pm$ 1.9
J08224744-5726530ACb M 4.5 M 6.0 67.4 $\pm$ 25.0
J19425324-4406278 M 3.5 M 4.5 30.1 $\pm$ 11.1
J19432464-3722108 M 3.5 M 6.0 50.3 $\pm$ 18.6
J20100002-2801410 M 2.5 M 3.5 16.0 $\pm$ 5.9
J20500010-1154092 M 3.5 M 4.5 18.5 $\pm$ 7.1
J21103147-2710578b M 4.5 M 5.5 152.0 $\pm$ 56.3
J22171899-0848122ABb M 4.0 M 4.5 79.5 $\pm$ 29.4
J22171899-0848122ACb M 4.0 M 8.5 77.9 $\pm$ 28.8
J22332264-0936537 M 2.5 M 3.0 37.0 $\pm$ 13.7
J22382974-6522423 M 3.5 M 3.5 12.6 $\pm$ 1.2
J22401867-4931045 M 5.5 M 5.5 40.4 $\pm$ 14.9
J23581366-1724338 M 2.0 M 2.0 55.7 $\pm$ 20.6

Notes. (a) The primary star spectral type is earlier than M 0 (see also Appendix). The system is therefore not included in the statistical analysis. (b) The survey is not complete for component separations greater than 6 $^{\prime \prime }$ and these stars are therefore not included in the statistical analysis (see Table 2). (c) Our primary star is the secondary star in a known binary system in which the primary star is of spectral type F. The system is therefore not included in the statistical analysis.


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