Fig. 1
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HR diagram of all Gaia DR3 nearby stars with a parallax of π ≥ 5 mas, using the broad-band G magnitude versus the colour GBP (blue) minus GRP (red). The colours indicate log(g). Stars without a log(g) measurement are shown in grey. The six targets presented in this paper as part of the NIRPS-GTO giants sub-programme are overplotted (outlined black circles), along with five stars identified as giant stars using this method. TOI-3288 and TOI-4666 (outlined black squares), hosting gas giants, are visible on the main sequence. This figure can be generated using Gaia-HR, available at https://github.com/ygcfrensch/Gaia-HR.
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