Table 1
Target information.
| Target name | Coordinates | Spectral | Membership | Date obs. | Exposure time | Comments | |
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| RA | Dec | type | (s) | ||||
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| GSC08056 | 02 36 51.5 | –52 03 04.4 | M2 | Tuc-Hor | 26/12/2009 | 91 × 150 × 0.2 | Pupil tracking |
| GJ3305 | 04 37 37.5 | –02 29 28.2 | M0 | βpic | 26/12/2009 | 64 × 300 × 0.2 | Binary; Pupil tracking |
| GJ3305 | 04 37 37.5 | –02 29 28.2 | M0 | βpic | 01/09/2011 | 250 × 150 × 0.2 | Binary; Pupil tracking |
| 2MASS J0443 | 04 43 37.6 | +00 02 05.2 | M9 | (1) | 27/12/2009 | 50 × 300 × 0.2 | Pupil tracking |
| V1005 Ori | 04 59 34.8 | +01 47 00.7 | M0 | βpic | 25/12/2009 | 16 × 150 × 0.2 | – |
| CD-571054 | 05 00 47.1 | –57 15 25.5 | M0V | βpic | 29/12/2009 | 64 × 150 × 0.2 | – |
| BD-21 1074A | 05 06 49.6 | –21 35 06.0 | M2V | βpic | 28/12/2009 | 32 × 120 × 0.25 | – |
| BD01 2447 | 10 28 55.6 | +00 50 27.6 | M2.5V | AB Dor | 02/05/2011 | 48 × 200 × 0.2 | Pupil tracking |
| 2M1139 | 11 39 51.1 | –31 59 21.5 | M8 | TWA | 26/12/2009 | 36 × 600 × 0.3 | – |
| 2MASS1207 | 12 07 33.5 | –39 32 53.9 | M8 | TWA | 26/12/2009 | 141 × 300 × 0.2 | – |
| TWA25 | 12 15 30.7 | –39 48 42.6 | M1V | TWA | 03/05/2011 | 24 × 100 × 0.4 | – |
| TYC7443-1102-1 | 19 56 04.4 | –32 07 37.7 | M0V | βpic | 03/05/2011 | 87 × 200 × 0.2 | Pupil tracking |
| HIP102409/AUmic | 20 45 09.5 | –31 20 27.2 | M1V | βpic | 28/07/2010 | 94 × 100 × 0.2 | Pupil tracking |
| WWPsA | 22 44 58.0 | –33 15 01.7 | M1 | βpic | 27/12/2009 | 32 × 150 × 0.2 | – |
| TXPsA | 22 45 00.0 | –33 15 25.8 | M5V | βpic | 26/12/2009 | 32 × 150 × 0.2 | – |
| HIP114046 | 23 05 52.0 | –35 51 11.1 | M2V | (2) | 28/07/2010 | 92 × 100 × 0.2 | Pupil tracking |
| BD-13 64 24 | 23 32 30.9 | –12 15 51.4 | M0V | βpic | 27/12/2009 | 32 × 150 × 0.2 | – |
Notes. Pupil tracking indicates observations were carried out in pupil tracking and with a field rotation enabling ADI reduction procedures. (1) Presence of lithium according to Reiners & Basri (2009) and low gravity (Cruz et al. 2007) ensures this object is younger than 120 Myr (see Sect. 2.3.2). (2) Age determination is presented in Sect. 2.3.3. For mass limit determination purposes we assumed an age range of 100–2000 Myr.
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