Table 2
DAOSPEC analysis of different Moon solar spectra.
Observation | RVc | RV | σ | N. lines | ΔRV(O–C)b | RV | σ | N. lines | ΔRV(O–C)r | |
km s-1 | km s-1 | km s-1 | km s-1 | km s-1 | m s-1 | km s-1 | ||||
|
||||||||||
2010-11-25, 05-47-20 | –1.190 | –1.181 | 0.267 | 494 | 0.009 | –1.169 | 0.061 | 239 | 0.020 | |
2010-11-25, 05-49-42 | –1.187 | –1.180 | 0.248 | 484 | 0.006 | –1.166 | 0.057 | 240 | 0.020 | |
2010-11-25, 05-53-19 | –1.182 | –1.176 | 0.256 | 487 | 0.007 | –1.158 | 0.059 | 236 | 0.024 | |
2010-11-25, 05-55-20 | –1.179 | –1.176 | 0.263 | 490 | 0.004 | –1.157 | 0.056 | 234 | 0.022 | |
2010-11-25, 05-57-54 | –1.176 | –1.171 | 0.264 | 493 | 0.005 | –1.158 | 0.057 | 236 | 0.019 |
Notes. RVc is the expected radial velocity computed with JPL ephemerides. RV, VR and σ are the mean radial velocities and dispersion of all the identified lines by DAOSPEC with respect to the input line list, separately for the two CCDs. ΔRV(O–C)b and ΔRV(O–C)r are the difference between the two quantities.
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