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| | 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 |