Table 3
Image properties and measured fluxes of detected radio sources.
Synthesized beam | |||||
---|---|---|---|---|---|
Star ID | Epoch | Noise (µJy bm−1) | θmaj × θmin; PA (mas × mas; °) | Sv,Int. (µJy) | Sv,Peak. (µJy bm−1) |
V 875 Per | B1 | 26 | 3.1 × 1.3; −5.9 | 1042 ± 66 | 585 ± 26 |
B2 | 42 | 4.5 × 1.7; −9.0 | 1225 ± 86 | 885 ± 42 | |
B1+B2 | 23 | 3.3 × 1.4; −6.5 | 1156 ±56 | 667 ± 23 | |
HD 22213 | C1 | 24 | 3.6 × 1.3; +1.5 | 338 ± 88 | 142 ± 24 |
C2 | 26 | 3.5 × 1.1; +9.7 | 710 ± 54 | 552 ± 26 | |
C1+C2 | 17 | 3.9 × 1.4; +9.9 | 450 ± 40 | 297 ± 17 | |
HD 285281 | D1 | 17 | 4.0 × 1.7; −6.1 | 270 ± 62 | 96 ± 17 |
D2 | 24 | 3.9 × 1.6; −3.6 | 152 ± 47 | 141 ± 26 | |
D1+D2 | 13 | 3.9 × 1.6; −4.9 | 170 ± 33 | 103 ± 13 | |
AI Lep | F1 | 26 | 4.7 × 1.8; +6.7 | 541 ± 59 | 387 ± 27 |
F2 | 15 | 5.0 × 1.8; +0.1 | 105 ± 33 | 69 ± 15 | |
F1+F2 | 12 | 4.8 × 1.8; +1.9 | 220 ± 36 | 144 ± 16 | |
HD 62237 | G1 | 21 | 4.3 × 1.6; −1.8 | 415 ± 65 | 190 ± 21 |
G2 | 19 | 4.3 × 1.6; −0.2 | 172 ± 35 | 164 ± 19 | |
G1+G2 | 15 | 4.3 × 1.6; −1.0 | 280 ± 38 | 162 ± 15 | |
SAO 135659 | G1 | 20 | 4.2 × 1.6; −2.7 | 648 ± 41 | 540 ± 21 |
G2 | 22 | 4.2 × 1.7; −0.4 | 524 ± 41 | 444 ± 22 | |
G1+G2 | 16 | 4.2 × 1.7; −1.6 | 586 ± 31 | 489 ± 16 | |
HD 82159 | H1 | 66 | 3.9 × 1.6; +3.2 | 980 ± 138 | 734 ± 66 |
H2 | 47 | 4.0 × 1.7; +1.5 | 470 ± 76 | 503 ± 47 | |
H1+H2 | 38 | 3.9 × 1.6; +2.2 | 669 ± 74 | 577 ± 39 | |
HD 82558 | H1 | 38 | 4.0 × 1.6; +0.8 | 462 ± 77 | 362 ± 38 |
H2 | 25 | 4.2 × 1.6; −1.2 | 219 ± 40 | 230 ± 25 | |
H1+H2 | 22 | 4.1 × 1.6; −0.3 | 365 ± 65 | 260 ± 27 | |
HD 199143 | J1 | 30 | 5.1 × 1.9; −5.4 | 280 ± 81 | 155 ± 31 |
J2 | 20 | 5.7 × 1.6; −9.7 | 162 ± 57 | 81 ± 20 | |
J1+J2 | 17 | 5.4 × 1.7; −8.2 | 221 ± 64 | 113 ± 17 | |
GJ 4199 | K1 | 19 | 4.0 × 1.8; −15.9 | 350 ± 47 | 210 ± 19 |
K2 | 24 | 4.0 × 1.8; −12.0 | 273 ± 51 | 192 ± 24 | |
K1+K2 | 14 | 4.0 × 1.8; −13.8 | 306 ± 33 | 204 ± 15 |
Notes. Columns are (from left to right) the target star name, the epoch (for this table the epoch ID is constructed using the group name and the epoch number from Table 2), the image noise level, the synthesized beam size in units of milli-arcseconds, and the integrated and peak flux densities.
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