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Table 1.

Properties of the radio-bright M-dwarf sample.

Source name Optical coordinates Sep. S144 MHz z mag J mag Distance Spec. type log10L150 MHz
(J2000) (″) (mJy) (AB) (AB) (pc) (erg s−1 Hz−1)
ILTJ0010+3239 00:10:08 +32:39:01 0.7 0.97 ± 0.23 21.24 ± 0.04 20.40 ± 0.17 870 ± 600 M7 17.9
ILTJ0754+3456 07:54:22 +34:56:26 0.3 0.79 ± 0.2 20.32 ± 0.01 19.58 ± 0.09 490 ± 240 M8 17.3
ILTJ1004+3424 10:04:10 +34:24:34 0.7 0.71 ± 0.2 22.02 ± 0.06 > 21.01 > 1200 M7
ILTJ1059+5516 10:59:22 +55:16:21 0.7 0.62 ± 0.18 20.74 ± 0.02 20.25 ± 0.14 810±550 M7 17.7
ILTJ1101+6507 11:01:31 +65:07:50 0.8 0.55 ± 0.16 21.18 ± 0.03 M7
ILTJ1124+5141 11:24:58 +51:41:16 0.6 0.58 ± 0.17 19.87 ± 0.01 19.25 ± 0.07 420 ± 240 M8 17.1
ILTJ1132+3651 11:32:13 +36:51:49 0.1 0.64 ± 0.15 20.83 ± 0.03 20.20 ± 0.19 650 ± 530 M8 17.5
ILTJ1755+3937 17:55:45 +39:37:44 0.5 0.92 ± 0.22 21.54 ± 0.04 > 20.86 > 1400 M6

Notes. The separation reported is the offset between the optical and radio-source positions from the Legacy surveys and LoTSS-DR2 catalogue, respectively. It is important to note that the distances we report here were estimated from the spectral types and photometry and are therefore highly uncertain. The radio luminosities were derived assuming isotropic emission.

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