Fig. 28
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Example VELOCE model template fits to Gaia RVs. Top row: the full set of Gaia RVs for SS CMa is fitted at once (left) or split into two epoch (center and right). gaiadr3.gaia_source does not provide the template parameters for SS CMa despite Gaia RVs being available in gaiadr3.vari_epoch_rv. Bottom row: stars whose Gaia RVs were determined using different temperatures (from left to right: TX Cyg (4250K), WX Pup (5250K), AV Cir (6250K)). VELOCE uses a correlation mask created to match spectral type G2.
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