Table 6
Photometric rejection significance, spectroscopic reduced χ2 results, and corresponding formal significance without systematics for different comparison objects.
| Object | SpT | Photometry | add. | Spectroscopy | ||
| J−H | H−Ks | Ref. | H-band | K-band | ||
| [σ] | [σ] | [σ /  ] |
[σ / ] |
|||
|
|
||||||
| HD 237903 | K7V | 3.4 | 0.5 | [1] | >6/2.66 | >6/1.60 |
| Gl 846 | M0V | 2.8 | 1.8 | [1] | >6/2.38 | 5.4/1.51 |
| Gl 229 | M1V | 0.6 | 0.3 | [1] | >6/2.37 | 5.3/1.50 |
| Gl 806 | M2V | 4.5 | 2.5 | [1] | >6/2.73 | 4.3/1.40 |
| Gl 388 | M3V | 3.7 | 2.8 | [2], [1] | >6/2.57 | 3.7/1.33 |
| Gl 213 | M4V | 5.5 | 2.6 | [2], [1] | >6/2.80 | 2.5/1.21 |
| Gl 51 | M5V | 3.8 | 3.5 | [2], [1] | >6/2.47 | 2.6/1.21 |
| Gl 406 | M6V | 3.4 | 4.6 | [2], [1] | >6/2.50 | 2.5/1.20 |
| Gl 644C | M7V | 4.1 | 5.1 | [2], [1] | >6/2.87 | 2.2/1.17 |
| Gl 752B | M8V | 2.6 | 6.4 | [2], [1] | >6/2.76 | 2.3/1.18 |
| LHS 2065 | M9V | 1.7 | 7.5 | [1] | >6/2.45 | 2.2/1.17 |
| LHS 2924 | L0 | 1.4 | 6.5 | [2], [1] | >6/2.77 | 2.1/1.16 |
| 2MUCD 20581 | L1 | 2.2 | 7.5 | [2] | >6/3.96 | 3.7/1.33 |
| Kelu-1AB | L2+L3.5 | 2.2 | 9.8 | [2] | >6/3.68 | 3.6/1.32 |
| 2MUCD 11291 | L3 | 1.8 | >10 | [2] | >6/3.66 | 3.8/1.34 |
| 2MUCD 12128 | L4.5 | 5.5 | >12 | [2] | >6/3.09 | 3.4/1.29 |
| 2MUCD 11296 | L5.5 | 1.3 | >10 | [2] | >6/4.60 | 5.5/1.52 |
| 2MUCD 11314 | L6 | 2.0 | 8.4 | [2] | >6/3.64 | >6/1.66 |
| 2MUCD 10721 | L7.5 | 5.8 | >11 | [2] | >6/3.49 | 3.4/1.29 |
| 2MUCD 10158 | L8.5 | 2.5 | 9.8 | [2] | >6/4.87 | 5.0/1.47 |
| SDSS 1520+354 | T0 | 1.0 | 5.4 | [3] | >6/4.63 | >6/2.15 |
| SDSS 0909+652 | T1.5 | 0.3 | 0.4 | [4] | >6/8.04 | >6/3.64 |
| SDSS 1254-012 | T2 | 0.8 | 2.0 | [2] | >6/7.97 | >6/2.90 |
| 2MASS 055-140 | T4 | 9.4 | 0.1 | [2] | >6/16.2 | >6/19.1 |
|
|
||||||
| HD 204585 | M4.5III | 0.4 | 0.8 | [1] | >6/1.86 | >6/1.88 |
| HD 175865 | M5III | 0.1 | 0.5 | [1] | >6/1.91 | >6/1.78 |
| BK Vir | M7III | 0.4 | 0.9 | [1] | >6/2.47 | >6/1.72 |
| HY Aqr | M8-9III | 0.6 | 8.5 | [1] | >6/5.78 | >6/1.61 |
| Galaxies | various | 4.2 | 3.0 | [5], [6] | >6/2.28 | >6/1.61 |
| Quasars | – | 4.4 | 3.9 | [5] | – | – |
| White Dwarfs | various | 6.4 | 3.9 | [5] | – | – |
|
|
||||||
| CVSO 30 | M3 | 2.7 | 1.7 | >6/3.31 | 6.0/1.57 | |
| PZ Tel B | M7 | 2.1 | 1.4 | [7] | >6/3.29 | 3.0/1.25 |
| CT Cha b | M9 | 0.4 | 1.3 | [8], [9] | >6/2.27 | 1.8/1.13 |
| 2M0441 Bb | L1 | 0.5 | 2.4 | [10] | >6/3.13 | 1.9/1.13 |
| 1RXS 1609 b | L4 | 1.1 | 3.0 | [11] | >6/2.70 | 2.3/1.18 |
| β Pic b | L4 | 1.0 | 3.5 | [12] | >6/2.06 | – |
| 2M1207 b | L7 | 3.5 | 4.4 | [13] | >6/2.66 | 2.5/1.20 |
| S Ori 64 | L/T | 0.9 | 0.7 | [14] | – | – |
| DP (Fig. 4) | – | – | – | [15] | 2.2/1.16 | 2.0/1.14 |
Reference. [1] Rayner et al. (2009); [2] Cushing et al. (2005); [3] Burgasser et al. (2010a); [4] Chiu et al. (2006); [5] Hewett et al. (2006); [6] Mannucci et al. (2001); [7] Schmidt et al. (2014); [8] Schmidt et al. (2009); [9] Schmidt et al. (2008); [10] Bowler & Hillenbrand (2015); [11] Lafrenière et al. (2008); [12] Chilcote et al. (2015); [13] Patience et al. (2010); [14] Peña Ramírez et al. (2012); from VISTA to 2MASS magnitudes using colour equations from http://casu.ast.cam.ac.uk/surveys-projects/vista/technical/photometric-properties; [15] Helling et al. (2008).
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