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Table 6
Total number of single stars of each variability type, and the percentage of each that falls below each relative parallax error limit: 500%, 100%, 50%, 20%, 5%, and 1%.
Variability type | Total | σϖ/ϖ< 5 | σϖ/ϖ< 1 | σϖ/ϖ< 0.5 | σϖ/ϖ< 0.2 | σϖ/ϖ< 0.05 | σϖ/ϖ< 0.01 |
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Non-variables | 5.1 × 108 | 88 | 74 | 55 | 27 | 7.7 | 1.4 |
Emission | 3.3 × 106 | 99 | 97 | 92 | 62 | 16 | 2.4 |
Flaring | 2.1 × 105 | 99 | 99 | 98 | 88 | 33 | 4.6 |
δ Scuti | 3.3 × 106 | 90 | 78 | 61 | 35 | 13 | 3.5 |
Semi-regular | 3.6 × 106 | 92 | 82 | 68 | 40 | 14 | 1.4 |
Gammador | 6.0 × 105 | 91 | 80 | 63 | 35 | 13 | 3.2 |
RR Lyrae AB-type | 2.4 × 104 | 67 | 45 | 25 | 7.9 | 1.0 | 0.1 |
Mira | 2.3 × 105 | 92 | 83 | 70 | 44 | 16 | 1.2 |
ZZ Ceti | 1.9 × 104 | 100 | 100 | 99 | 94 | 33 | 4.1 |
ACV | 3.5 × 104 | 91 | 80 | 64 | 39 | 15 | 3.8 |
RR Lyrae C-type | 5.6 × 103 | 68 | 45 | 25 | 7.8 | 0.9 | 0.1 |
ρ Ap | 3.0 × 103 | 92 | 82 | 65 | 38 | 14 | 3.8 |
Cepheid | 1.8 × 103 | 95 | 88 | 78 | 59 | 30 | 0.1 |
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