Open Access
Table A.2.
Oscillating red giants in NGC 6819.
| ID | KIC | RA (°) | DEC (°) | Gaia (mag) | νmax (μHz) | Member (this work) | S11 member | C20 member |
|---|---|---|---|---|---|---|---|---|
| 92 | - | 295.2984 | 40.0901 | 13.60 |
 |
No | - | - |
| 93 | - | 295.2936 | 40.1458 | 14.06 |
 |
No | - | - |
| 94 | - | 295.2583 | 40.1445 | 14.24 |
 |
No | - | - |
| 95 | - | 295.2676 | 40.1656 | 13.61 |
 |
No | - | - |
| 96 | - | 295.3279 | 40.1953 | 12.26 |
 |
Yes | - | No (60%) |
| 97 | - | 295.2844 | 40.1772 | 13.29 |
 |
No | - | - |
| 98 | - | 295.3115 | 40.1835 | 12.52 |
 |
Yes | - | Yes |
| 99 | - | 295.4381 | 40.1639 | 14.69 |
 |
No | - | - |
| 100 | - | 295.4468 | 40.2657 | 14.45 |
 |
No | - | - |
| 101 | - | 295.3954 | 40.3276 | 13.06 |
 |
Yes | - | - |
| 102 | - | 295.3926 | 40.3291 | 13.12 |
 |
No | - | - |
| 103 | - | 295.3621 | 40.3200 | 13.91 |
 |
No | - | - |
| 104 | 4936825 | 295.2691 | 40.0808 | 13.14 |
 |
No | - | - |
| 105 | 5023953 | 295.2415 | 40.1382 | 12.59 |
 |
Yes | Yes | Yes |
| 106 | 5024043 | 295.2585 | 40.1078 | 12.78 |
 |
Yes | Yes | - |
| 107 | 5024268 | 295.2959 | 40.1866 | 11.31 |
 |
No | No | Yes |
| 108 | 5024297 | 295.3010 | 40.1927 | 12.90 |
 |
No | Yes | Yes |
| 109 | 5024312 | 295.3034 | 40.1915 | 13.54 |
 |
Yes | Yes | Yes |
| 110 | 5024322 | 295.3049 | 40.1116 | 13.09 |
 |
Yes | - | No (60%) |
| 111 | 5024327 | 295.3060 | 40.1989 | 12.75 |
 |
Yes | Yes | Yes |
| 112 | 5024404 | 295.3152 | 40.1696 | 12.86 |
 |
Yes | Yes | Yes |
| 113 | 5024414 | 295.3164 | 40.1865 | 12.65 |
 |
No | Yes | Yes |
| 114 | 5024456 | 295.3210 | 40.1811 | 11.08 |
 |
No | Yes | Yes |
| 115 | 5024476 | 295.3240 | 40.1544 | 12.51 |
 |
No | Yes | Yes |
| 116 | 5024512 | 295.3281 | 40.1985 | 13.29 |
 |
Yes | Yes | Yes |
| 117 | 5024517 | 295.3288 | 40.1947 | 13.00 |
 |
No | Yes | Yes |
| 118 | 5024582 | 295.3389 | 40.1992 | 12.67 |
 |
Yes | Yes | No (30%) |
| 119 | 5024583 | 295.3390 | 40.1834 | 12.73 |
 |
Yes | Yes | Yes |
| 120 | 5024601 | 295.3411 | 40.1968 | 12.46 |
 |
Yes | Yes | Yes |
| 121 | 5024750 | 295.3608 | 40.1949 | 11.81 |
 |
Yes | Yes | Yes |
| 122 | 5024967 | 295.3935 | 40.1461 | 12.79 |
 |
Yes | Yes | Yes |
| 123 | 5025021 | 295.4035 | 40.1508 | 12.84 |
 |
Yes | - | - |
| 124 | 5025101 | 295.4205 | 40.1867 | 13.00 |
 |
No | - | - |
| 125 | 5111718 | 295.1535 | 40.2548 | 13.80 |
 |
Yes | Yes | Yes |
| 126 | 5111767 | 295.1655 | 40.2312 | 13.64 |
 |
No | - | - |
| 127 | 5111940 | 295.2069 | 40.2420 | 13.00 |
 |
Yes | Yes | Yes |
| 128 | 5111949 | 295.2092 | 40.2197 | 12.76 |
 |
Yes | Yes | Yes |
| 129 | 5111987 | 295.2166 | 40.2600 | 14.95 |
 |
No | - | - |
| 130 | 5112072 | 295.2333 | 40.2276 | 13.74 |
 |
Yes | Yes | Yes |
| 131 | 5112118 | 295.2411 | 40.2314 | 12.59 |
 |
Yes | - | - |
| 132 | 5112281 | 295.2695 | 40.2476 | 12.18 |
 |
No | - | - |
| 133 | 5112361 | 295.2841 | 40.2524 | 13.05 |
 |
Yes | No | - |
| 134 | 5112373 | 295.2858 | 40.2250 | 12.76 |
 |
Yes | Yes | Yes |
| 135 | 5112387 | 295.2886 | 40.2454 | 12.78 |  |
Yes | Yes | Yes |
| 136 | 5112401 | 295.2913 | 40.2637 | 12.56 |
 |
Yes | Yes | Yes |
| 137 | 5112403 | 295.2919 | 40.2190 | 13.89 |
 |
No | Yes | Yes |
| 138 | 5112467 | 295.3033 | 40.2066 | 12.76 |
 |
Yes | Yes | Yes |
| 139 | 5112491 | 295.3064 | 40.2057 | 12.71 |
 |
Yes | Yes | Yes |
| 140 | 5112730 | 295.3395 | 40.2326 | 12.72 |
 |
Yes | Yes | Yes |
| 141 | 5112734 | 295.3407 | 40.2031 | 12.80 |
 |
No | Yes | Yes |
| 142 | 5112744 | 295.3426 | 40.2789 | 12.89 |
 |
Yes | Yes | Yes |
| 143 | 5112880 | 295.3628 | 40.2079 | 12.23 |
 |
Yes | Yes | Yes |
| 144 | 5112938 | 295.3714 | 40.2178 | 12.76 |
 |
Yes | Yes | Yes |
| 145 | 5112948 | 295.3726 | 40.2389 | 12.83 |
 |
No | Yes | Yes |
| 146 | 5112950 | 295.3731 | 40.2058 | 12.71 |
 |
Yes | Yes | Yes |
| 147 | 5112974 | 295.3761 | 40.2560 | 12.64 |
 |
Yes | Yes | Yes |
| 148 | 5113041 | 295.3888 | 40.2097 | 12.79 |
 |
Yes | Yes | Yes |
| 149 | 5200152 | 295.3494 | 40.3623 | 12.67 |
 |
Yes | Yes | Yes |
Notes. We report whether they are cluster members following our method (this work), and whether they were determined to be cluster members in Stello et al. 2011 (S11) and Cantat-Gaudin & Anders 2020 (C20; only when their membership probability is 100%).
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