Table 1
Observed sample.
Target | Obs. date | J | H | K | M (M⊙) | Ref. | |
|
|||||||
RM 231 | 2008 Dec. 18 | 11.12 | 10.56 | 10.25 | 0.306–0.321 | 2 | |
RM 346a | 2008 Dec. 20 | 11.18 | 10.55 | 10.28 | 0.308–0.317 | 2 | |
RM 132 | 2008 Dec. 18 | 11.16 | 10.57 | 10.28 | 0.305–0.317 | 2 | |
RM 221a | 2008 Oct. 20 | 11.19 | 10.59 | 10.32 | 0.302–0.310 | 2 | |
RM 49a | 2008 Dec. 20 | 11.21 | 10.59 | 10.33 | 0.302–0.309 | 2 | |
RM 182 | 2008 Dec. 20 | 11.24 | 10.63 | 10.36 | 0.296–0.304 | 2 | |
RM 60 | 2008 Dec. 20 | 11.34 | 10.76 | 10.47 | 0.277–0.287 | 2 | |
RM 376 | 2008 Dec. 20. | 11.38 | 10.79 | 10.53 | 0.273–0.280 | 2 | |
RM 126b | 2008 Oct. 20 | 12.06 | 11.47 | 11.16 | 0.192–0.200 | 2 | |
CFHT 13 | 2009 Dec. 8 | 12.45 | 11.87 | 11.51 | 0.160–0.170 | 1 | |
|
|||||||
RM 165c | 2009 Dec. 7 | 13.49 | 12.86 | 12.51 | 0.107–0.111 | 2 | |
CFHT 19 | 2008 Oct. 20 | 14.16 | 13.43 | 12.90 | 0.085–0.099 | 1 | |
UKIDSS 1 | 2008 Oct. 20 | 14.60 | 13.85 | 13.42 | 0.075–0.084 | 3 | |
UKIDSS 8 | 2009 Dec. 7 | 15.60 | 14.55 | 14.02 | 0.060–0.070 | 3 | |
UKIDSS 5 | 2009 Dec. 7 | 15.81 | 14.72 | 14.05 | 0.057–0.069 | 3 | |
UKIDSS 3c | 2009 Dec. 7 | 15.75 | 14.78 | 14.17 | 0.058–0.066 | 3 | |
UKIDSS 4 | 2008 Oct. 20 | 15.60 | 14.97 | 14.23 | 0.059–0.065 | 3 | |
UKIDSS 6 | 2009 Dec. 7 | 15.50 | 14.81 | 14.25 | 0.061–0.064 | 3 | |
UKIDSS 2 | 2009 Dec. 8 | 15.94 | 14.81 | 14.26 | 0.056–0.064 | 3 | |
UKIDSS 11 | 2008 Oct. 20 | 16.11 | 15.05 | 14.28 | 0.054–0.063 | 3 | |
UKIDSS 7 | 2008 Oct. 20 | 15.99 | 15.03 | 14.36 | 0.055–0.061 | 3 | |
UKIDSS 9 | 2008 Oct. 20 | 16.68 | 15.29 | 14.52 | 0.045–0.058 | 3 | |
UKIDSS 12 | 2008 Oct. 20 | 16.73 | 15.77 | 14.80 | 0.044–0.054 | 3 | |
UKIDSS 10 | 2009 Dec. 7 | 16.54 | 15.43 | 14.84 | 0.049–0.053 | 3 | |
CFHT 20 | 2008 Oct. 20 | 17.02 | 16.51 | 16.08 | 0.037–0.039 | 1 | |
CFHT 21 | 2008 Oct. 20 | 18.48 | 17.36 | 16.59 | 0.020–0.035 | 1 |
Notes.The horizontal line demarcates low-mass from very low-mass targets. Masses are estimated (using integrated system magnitudes for binary systems) comparing the near-infrared magnitude to BT-Settl models at an age of 600 Myr. Boldfaced entries indicate the masses derived from the K band photometry.
Known binary (Reid & Gizis 1997).
Suspected binary (Reid & Gizis 1997).
Reference. 1) Bouvier et al. (2008); 2) Reid (1993); 3) Hogan et al. (2008).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.