Table A2.
Open in new tab

An example covariance matrix for the star 5220895866301073408. The diagonal values are the square of the standard deviations and the off-diagonal values indicate the correlation between the parameters.

Teff|$\rm \log \mathit{g}$||$\rm [Fe/H]$||$\rm \varpi$|E(B−V)
Teff34320.921.79−0.240.56
|$\rm \log \mathit{g}$|0.00 0450.00 0982.65e−50.0002
|$\rm [Fe/H]$|0.0026−0.00 0130.00 046
|$\rm \varpi$|0.00 018−4.59e−05
E(B−V)0.00 012
Teff|$\rm \log \mathit{g}$||$\rm [Fe/H]$||$\rm \varpi$|E(B−V)
Teff34320.921.79−0.240.56
|$\rm \log \mathit{g}$|0.00 0450.00 0982.65e−50.0002
|$\rm [Fe/H]$|0.0026−0.00 0130.00 046
|$\rm \varpi$|0.00 018−4.59e−05
E(B−V)0.00 012
Table A2.
Open in new tab

An example covariance matrix for the star 5220895866301073408. The diagonal values are the square of the standard deviations and the off-diagonal values indicate the correlation between the parameters.

Teff|$\rm \log \mathit{g}$||$\rm [Fe/H]$||$\rm \varpi$|E(B−V)
Teff34320.921.79−0.240.56
|$\rm \log \mathit{g}$|0.00 0450.00 0982.65e−50.0002
|$\rm [Fe/H]$|0.0026−0.00 0130.00 046
|$\rm \varpi$|0.00 018−4.59e−05
E(B−V)0.00 012
Teff|$\rm \log \mathit{g}$||$\rm [Fe/H]$||$\rm \varpi$|E(B−V)
Teff34320.921.79−0.240.56
|$\rm \log \mathit{g}$|0.00 0450.00 0982.65e−50.0002
|$\rm [Fe/H]$|0.0026−0.00 0130.00 046
|$\rm \varpi$|0.00 018−4.59e−05
E(B−V)0.00 012
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