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Table 2

Coralie RV standard stars.

Star SpType FWHM (km s−1) COR07 rv (m s−1) COR07 err (m s−1) COR14 rv (m s−1) COR14 err (m s−1) COR07–COR14 (m s−1) Comb. err (m s−1)
HD1581 F9.5V 7.83 9315.71 1.34 9342.99 0.40 −27.28 1.39
HD65907A F9.5V 7.55 14987.94 3.27 15 017.66 0.26 −29.72 3.28
HD108309 G2V 8.37 30 617.57 2.12 30 642.60 0.33 −25.03 2.14
HD 144585 G2V 8.52 −14016.01 2.12 −13 995.28 0.32 −20.73 2.14
HD20794 G6V 7.67 87 907.57 0.66 87 938.41 0.23 −30.84 0.69
HD 10700 G8V 8.19 −16568.22 1.24 −16546.5 0.20 −21.72 1.25
HD 161612 G8V 8.40 2488.82 1.26 2509.41 0.50 −20.59 1.35
HD 190248 G8IV 8.37 −21 511.53 3.78 −21 492.73 0.29 −18.8 3.79
HIP 75386 G6III 8.37 −13 723.49 3.74 −13 694.49 3.37 −29.00 5.03
HIP 10440 G9III 8.88 20615.30 3.95 20 641.42 2.72 −26.12 4.79
weighted average difference COR07–COR14 (m s−1): −26.8 0.5

Notes. Coralie RV standard star measurements in m s−1. The finer scale compared to Table 1 is warranted by the better precision due to the available simultaneous drift correction. COR07 refers to Coralie after instrument upgrades installed in 2007 and before upgrades installed in 2014, label henceforth as COR14. The RV zero-points and their uncertainties were determined using DACE5 (Buchschacher & Alesina 2019). The two last columns list the difference between COR07 minus COR14 and the square-summed errors. The weighted average of the offsets is −26.8 ± 0.5 m s−1. NB: These offsets have not yet been applied to VELOCE data.

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