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Table 2

DAOSPEC analysis of different solar spectra.

Target RVred σ N. lines RVblue σ N. lines Input lines ΔRV(o − e)red ΔRV(o − e)blue
km s-1 km s-1 km s-1 km s-1 m s-1 m s-1

FTS-2005 –0.515 0.260 1208 –0.552 0.986 2682 APGL –122 –84
FTS-1984 0.006 0.222 1189 0.005 0.572 2647 APGL
FTS-2011* –0.221 0.292 450 –0.157 1.357 1043 APGL –84 143
FTS-2011** –0.322 0.173 672 –0.173 0.436 1523 APGL 34 –36
Ceres 3.911 0.422 1217 3.962 1.483 2386 APGL –11 40
FTS-2005 –0.537 0.115 464 –0.645 1.017 1798 this paper –99 8
Ganymede 5.9384 0.070 501 5.9386 0.232 1713 this paper 0.4 0.6
Vesta (23) 3.843 0.079 488 3.836 0.140 1714 this paper 8 1
Vesta (24) 3.783 0.084 495 3.779 0.141 1723 this paper 9 5
Vesta (25) 3.714 0.074 488 3.709 0.140 1701 this paper –2 –7
SKY –0.026 0.061 480 –0.086 0.220 1712 this paper –26 –86

Notes. 

(*)

Refers to the Wallace et al. (2011) spectrum in the ranges 5335 − 5747 and 4015 − 4443 Å.

(**)

The same, but for the ranges 5747 − 6859 and 4443 − 5304 Å.

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