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Table 3.

Astrometric results (estimated minus true) for test 2.

Magnitude range Step Median
RSE
ϖ α* δ μα* μδ ϖ α* δ μα* μδ
G < 13 1 −0.9 3.1 1.8 3.7 −0.8 8.5 13.1 9.8 14.2 7.6
3 0.2 −0.3 0.1 −0.4 0.1 7.9 7.0 6.2 4.9 4.4
AGIS 7.5 6.6 5.7 4.5 4.0
13 ≤ G < 15 1 −0.9 2.3 2.4 3.1 −0.8 14.8 17.0 13.4 16.4 10.4
3 0.0 −0.3 0.1 −0.3 0.0 14.4 11.8 10.5 8.4 7.4
AGIS 14.9 12.4 10.6 8.7 7.5
15 ≤ G < 16 1 −0.9 1.3 3.0 2.3 −0.7 25.3 24.6 20.2 21.7 15.0
3 0.1 −0.5 0.1 −0.4 0.0 25.1 20.2 17.9 14.2 12.6
AGIS 24.9 20.2 17.3 14.3 12.3
16 ≤ G < 17 1 −1.0 0.7 3.1 1.8 −0.4 40.2 35.2 29.7 29.0 21.8
3 −0.2 −0.6 0.0 −0.3 0.1 40.0 31.9 27.7 22.5 19.7
AGIS 38.4 30.8 26.7 21.8 19.0
17 ≤ G < 18 1 −1.0 0.1 3.6 1.2 −0.1 65.5 54.6 46.0 41.9 33.5
3 −0.2 −0.4 0.1 −0.1 −0.1 65.4 52.4 44.9 36.7 32.0
AGIS 61.8 49.4 42.8 34.8 30.4
18 ≤ G < 19 1 −0.9 0.1 3.9 0.5 −0.2 110.8 90.3 76.1 65.7 54.8
3 −0.1 0.1 0.6 −0.1 −0.2 110.8 89.0 75.4 62.4 53.8
AGIS 104.1 83.3 70.7 58.9 50.8
19 ≤ G 1 −0.2 −0.3 2.8 0.1 −0.4 199.7 161.5 134.3 115.3 95.8
3 0.3 0.4 −0.3 0.1 −0.5 199.5 160.8 134.0 113.6 95.4
AGIS 207.6 167.9 140.0 118.5 100.2

Notes. Units are in μas for parallaxes and positions and μas yr−1 for proper motions. Right ascension and the corresponding proper motion are provided as α* = αcosδ and μα* = μαcosδ. The RSEs of the AGIS demonstration run as reported in Lindegren et al. (2012) are shown for an easier comparison.

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