Gaia Data Release 3
Open Access

Fig. 7.

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Radial velocity shift that had to be applied by ESP-HS in CU8 to align the theoretical spectrum to the observed RVS spectrum as determined by MTA. It is plotted as a function of the Teff determined by ESP-HS. Top panel: running median (computed over consecutive Teff bins of 10 K) and the interquantile dispersion (15.85%–84.15%) of this offset as a function of the effective temperature. Bottom panel: how many stars went into each 10 K bin.

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