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Table 1

Hermes RV standard stars.

Star SpType FWHM (km s−1) HER rv (km s−1) HER err (km s−1) HER18 rv (km s−1) HER18 err (km s−1) HER–HER18 (km s−1) Comb. err (km s−1)
HD 154417(†) F8.5IV 10.883 −16.729 0.009 −16.668 0.005 −0.061 0.011
HD 168009(†) G1V 8.370 −64.570 0.002 −64.509 0.004 −0.061 0.005
HD 32923 G4V 7.982 20.623 0.005 20.747 0.004 −0.125 0.007
HD 197076 G5V 8.178 −35.417 0.005 −35.321 0.004 −0.097 0.006
HD 42807(†) G5V 9.412 6.067 0.003 6.148 0.006 −0.080 0.006
HD 141105 G8V 8.225 1.876 0.003 1.957 0.003 −0.081 0.004
HD 144579 G8V 7.532 −59.445 0.003 −59.372 0.002 −0.074 0.004
HD 10780 K0V 8.243 2.810 0.007 2.841 0.004 −0.031 0.008
HD 221354 K0V 8.284 −25.107 0.002 −25.049 0.002 −0.058 0.003
HD65583 K0V 7.523 14.810 0.037 14.886 0.006 −0.076 0.038
HD 82106 K3V 9.868 29.803 0.007 29.880 0.003 −0.076 0.008
weighted average difference HER–HER 18 (km s−1): −0.075 0.007

Notes. Spectral types from SIMBAD. HER and HER18 denote Hermes RVs before and after the upgrade of the optical fiber on 25 April 2018, respectively. Columns labeled ‘rv’ and ‘err’ refer to straight means and standard errors on the mean, respectively. The last two columns show the difference before minus after the upgrade and the square summed mean errors. Low-amplitude spectroscopic binaries exhibiting orbital signals have been marked with a(†). NB: These offsets have not yet been applied to VELOCE data.

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