| Session 2: On-board data handling | ||
| 8.1 | Y. Viala | Compare Y. Viala/U. Lammers telemetry predictions |
| 8.2 | Y. Viala | Implement A. Vallenari selection strategy in the telemetry model |
| 8.3 | Y. Viala | Implement RVF star counts in the telemetry model |
| 8.4 | A. Vallenari | Write technical note on the selection strategy |
| 8.5 | TBD | Define scientific specifications for the calibration of the sky background |
| Session 3: Star and RVS simulation | ||
| 8.6 | U. Munari | Observe low metallicity reference stars: [Fe/H] < -2 |
| 8.7 | U. Munari | Contact authors of spectral libraries in the RVS domain, for inclusion of their libraries in the "ESTEC/Gaia spectra archiving system" |
| 8.8 | S. Ansari | Include Asiago observed spectra in the "ESTEC/Gaia spectra archiving system" |
| 8.9 | A. Recio-Blanco | Consult ESO spectrographs (GIRAFFE, ...) archives: spectra in the RVS domain |
| Session 4: On-ground data calibration & analysis, RVS performances and science case | ||
| 8.10 | D. Katz, F. Crifo | Estimate number of "RVS selected reference stars" available for wavelength calibration |
| 8.11 | D. Katz | Provide spectral dispersion law as function of location in the field of view |
| 8.12 | A. Gomboc | Assess impact of mismatch on v sin i performances |
| 8.13 | T. Zwitter, D. Katz | Assess impact of crowding in very high stellar density fields |