Table 5.
Properties of detected radio sources.
| VLBA | Julian | RA | σα | Dec | σδ | Flux | ||
|---|---|---|---|---|---|---|---|---|
| Name | Project | Date | (h m s) | (s) | (° ′ ″) | (″) | (μJy) | MPC |
| GBS-VLA J053428.42+100422.6 | BL175GO | 2456733.58 | 05 34 28.418538 | 0.000034 | +10 04 22.54831 | 0.00075 | 1838 ± 271 | J0536+0944 |
| GBS-VLA J053428.42+100422.6 | BL175FX | 2457294.01 | 05 34 28.418489 | 0.000010 | +10 04 22.55126 | 0.00025 | 1421 ± 202 | J0536+0944 |
| GBS-VLA J053455.56+095713.2 | BL175GO | 2456733.58 | 05 34 55.558763 | 0.000060 | +09 57 13.11874 | 0.00126 | 1463 ± 387 | J0536+0944 |
| GBS-VLA J053503.54+095640.8 | BL175GO | 2456733.58 | 05 35 03.536585 | 0.000045 | +09 56 40.76773 | 0.00100 | 970 ± 220 | J0536+0944 |
| GBS-VLA J053503.54+095640.8 | BL175ER | 2456950.00 | 05 35 03.536520 | 0.000023 | +09 56 40.77070 | 0.00125 | 543 ± 165 | J0536+0944 |
| GBS-VLA J053459.44+095312.0 | BL175GO | 2456733.58 | 05 34 59.441635 | 0.000014 | +09 53 11.91540 | 0.00023 | 1797 ± 115 | J0536+0944 |
| GBS-VLA J053459.44+095312.0 | BL175ER | 2456950.00 | 05 34 59.441575 | 0.000016 | +09 53 11.91674 | 0.00034 | 1492 ± 159 | J0536+0944 |
| GBS-VLA J053459.44+095312.0 | BL175FL | 2457096.60 | 05 34 59.441538 | 0.000010 | +09 53 11.91680 | 0.00034 | 1057 ± 115 | J0536+0944 |
| GBS-VLA J053459.44+095312.0 | BL175FX | 2457294.01 | 05 34 59.441626 | 0.000005 | +09 53 11.91970 | 0.00011 | 2210 ± 200 | J0536+0944 |
| GBS-VLA J053449.71+095153.8 | BL175GO | 2456733.58 | 05 34 49.707676 | 0.000033 | +09 51 53.77293 | 0.00075 | 3156 ± 384 | J0536+0944 |
Notes. Columns are (left to right): The source name as they appear in SIMBAD astronomical database and/or previous radio surveys; in particular, GBS–VLA refers to sources identified in the Gould’s Belt VLA Survey (Kounkel et al. 2014), the VLBA code of the observation, the Julian date, the measured position in right ascension and declination with their respective uncertainties, the measured flux densities corrected by the primary beam attenuation, and the MPC used to observe the target. This table is available at the CDS. A portion is shown here for guidance regarding its form and content.
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