Gaia Data Release 3
Open Access

Fig. 10.

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Number of hot stars (log scale) with radial velocities in DR3, split up according to rv_template_teff, grvs_mag (left panel) and G magnitude (phot_g_mean_mag) (right panel). Each sub-panel lists the magnitude range and the number of stars within that range. While DR3 has a formal cutoff of magnitude 12, there are some stars fainter than this because of the difference between GRVS and grvs_mag (see Sect. 3).

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