Table 1
Journal of observations of the solar spectra, obtained from the reflected light on the bright asteroids 4 Vesta and 12 Victoria.
| Point | Date | Date | Exp. time | Airmass | BVC | RV |
| source | [Gregorian] | [HJD – 2 456 500.0] | [s] | [] | [km s-1 ] | [km s-1 ] |
|
|
||||||
| Vesta | 2014, July 30 | 369.374174 | 1200 | 1.48 | –29.171 | –10.710 ± 0.001 |
| Vesta | 2014, July 30 | 369.388641 | 1200 | 1.59 | –29.199 | –10.718 ± 0.001 |
| Vesta | 2014, July 30 | 369.403109 | 1200 | 1.73 | –29.225 | –10.725 ± 0.001 |
|
|
||||||
| Victoria | 2014, July 31 | 369.580444 | 1200 | 1.20 | +19.638 | 12.405 ± 0.001 |
| Victoria | 2014, July 31 | 369.594914 | 1200 | 1.15 | +19.600 | 12.403 ± 0.002 |
| Victoria | 2014, July 31 | 369.609384 | 1200 | 1.11 | +19.561 | 12.405 ± 0.001 |
Notes. The heliocentric Julian date (HJD), the dimensionless air mass, as well as the barycentric velocity correction (BVC) calculated by the pipeline, are given for the midpoint of the exposure time (Exp. time). The barycentric radial velocity (RV) and the corresponding uncertainty were determined from a weighted cross-correlation, as described in the text. All observations were taken during the night from July, 30 to July 31, 2014.
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