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Table 2

Intrinsic instabilities in rotations, glides, and quadrupole distortions between K and Gaia.

Parameter σquasar-like σintermediate σblazar-like σdefining
R1 55 59 28 26
R2 78 47 23 22
R3 42 46 24 22
D1 69 62 36 37
D2 59 46 30 32
D3 63 46 27 16
E20 90 51 26 32
M20 50 51 27 34
E21ReMathematical equation: $\[E_{21}^{\mathrm{Re}}\]$ 95 48 37 29
E21ImMathematical equation: $\[E_{21}^{\mathrm{Im}}\]$ 73 57 33 26
M21ReMathematical equation: $\[M_{21}^{\mathrm{Re}}\]$ 82 61 33 38
M21ImMathematical equation: $\[M_{21}^{\mathrm{Im}}\]$ 86 78 45 48
E22ReMathematical equation: $\[E_{22}^{\mathrm{Re}}\]$ 26 28 13 15
E22ImMathematical equation: $\[E_{22}^{\mathrm{Im}}\]$ 35 25 15 15
M22ReMathematical equation: $\[M_{22}^{\mathrm{Re}}\]$ 42 30 19 10
M22ImMathematical equation: $\[M_{22}^{\mathrm{Im}}\]$ 39 25 18 12

Average 61 48 27 26

Notes. Values given in μas, estimated as σ2=σtotal2σstat2Mathematical equation: $\[\sigma^{2}=\sigma_{\text {total}}^{2}-\sigma_{\text {stat}}^{2}\]$, where σtotal is the dispersion observed in the samples, and σstat is the dispersion due to sample size.

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