Table 2
Summary of the comparison between the TGAS parallaxes and the external catalogues.
Catalogue | Outliers | ϖ difference | ϖ extra dispersion |
|
|||
Hipparcos | 0.09% | −0.094 ± 0.004 | 0.580 ± 0.005 |
|
|||
VLBI | 0/9 | 0.083 ± 0.12 | – |
HST | 2/19 | −0.11 ± 0.19 | 0.6 ± 0.2 |
RECONS | 0/13 | −1.04 ± 0.58 | −0.9 ± 0.5 |
VLBI & HST & RECONS | 2/41 | −0.08 ± 0.12 | 0.42 ± 0.13 |
|
|||
Cepheids | 0/207 | −0.014 ± 0.014 | −0.18 ± 0.01 |
RRLyrae | 0/130 | −0.07 ± 0.02 | −0.16 ± 0.02 |
Cepheids & RRLyrae | 0/337 | −0.034 ± 0.012 | −0.17 ± 0.01 |
|
|||
RAVE | 47/5144 | 0.070 ± 0.005 | −0.06 ± 0.02 |
APOGEE | 0/2505 | −0.060 ± 0.006 | −0.12 ± 0.01 |
LAMOST | 6/317 | −0.01 ± 0.02 | −0.17 ± 0.02 |
PASTEL | 1/218 | 0.05 ± 0.02 | 0.10 ± 0.05 |
APOKASC | 0/969 | −0.070 ± 0.009 | −0.15 ± 0.01 |
|
|||
LMC | 2/142 | 0.11 ± 0.02 | −0.14 ± 0.03 |
SMC | 0/58 | −0.12 ± 0.05 | −0.09 ± 0.09 |
|
|||
ICRF2 QSO auxiliary solution | 1/2060 | −0.046 ± 0.010 | −0.17 ± 0.01 |
Notes. The number of outliers (at 5σ) vs. the total number of stars is presented. The parallax difference (ϖG−ϖE, in mas) and the extra uncertainty (in mas) that needs to be quadratically added or subtracted to the data to adjust the residuals are indicated in red when they are significant and in green when they are not (p-value limit: 0.01). A global estimate of the parallax offset as given by the weighted average of these various tests is −0.036 ± 0.002 mas, very similar to the estimate found using quasars, and the median of the extra dispersion is −0.14 ± 0.08 mas.
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