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Table 2
Upper limits on the radio flux and radio luminosity at 4.9 GHz (present survey) and 8.5 GHz (McLean et al. 2012) of the seven dwarfs that are present in both surveys.
| Name | Other name | F (4.9 GHz) | L ν,4.9 | F (8.5 GHz) | L ν,8.5 | |||
| (10-5 Jy) | (erg s-1 Hz-1) | (10-5 Jy) | (erg s-1 Hz-1) | |||||
|
|
||||||||
| 2MASS J10481258-1120082 | GJ 3622 | <6.3 | <1.53 × 1012 | <9.6 | <2.33 × 1012 | |||
| 2MASS J17571539+7042011 | LP 44-162 | <8.1 | <1.51 × 1013 | <11.7 | <2.19 × 1013 | |||
| 2MASS J11554286-2224586 | LP 851-346 | <6.6 | <7.43 × 1012 | <9.0 | <1.01 × 1013 | |||
| 2MASS J12505265-2121136 | <6.6 | <9.73 × 1012 | <7.2 | <1.06 × 1013 | ||||
| 2MASS J09211410-2104446 | <7.2 | <1.14 × 1013 | <7.5 | <1.29 × 1013 | ||||
| 2MASS J08283419-1309198 | <6.3 | <1.01 × 1013 | <6.6 | <1.06 × 1013 | ||||
| 2MASSI J0700366+315726 | <4.2 | <8.01 × 1012 | <7.8 | <1.39 × 1013 | ||||
Notes. We used the distances listed in Table1 to calculate Lν,8.5.
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