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Table 3

Intrinsic instabilities in rotations, glides, and quadrupole distortions between X/Ka and Gaia.

Parameter σquasar-like σintermediate σblazar-like σdefining
R1 37 51 19 28
R2 60 48 28 26
R3 42 58 23 26
D1 44 67 0 39
D2 47 48 18 31
D3 54 45 30 25
E20 62 56 29 40
M20 42 57 13 36
E21ReMathematical equation: $\[E_{21}^{\mathrm{Re}}\]$ 62 52 37 27
E21ImMathematical equation: $\[E_{21}^{\mathrm{Im}}\]$ 54 52 22 30
M21ReMathematical equation: $\[M_{21}^{\mathrm{Re}}\]$ 74 64 34 49
M21ImMathematical equation: $\[M_{21}^{\mathrm{Im}}\]$ 55 78 13 57
E22ReMathematical equation: $\[E_{22}^{\mathrm{Re}}\]$ 24 36 15 20
E22ImMathematical equation: $\[E_{22}^{\mathrm{Im}}\]$ 35 33 13 16
M22ReMathematical equation: $\[M_{22}^{\mathrm{Re}}\]$ 31 32 16 14
M22ImMathematical equation: $\[M_{22}^{\mathrm{Im}}\]$ 38 24 20 17

Average 48 50 21 30

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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