Gaia Data Release 3
Open Access

Fig. 2.

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Saturation in an RVS spectrum. The CCD spectrum shown (in units of e per 4.4 s exposure) was obtained from the summing in the AC direction of a 2D-window spectrum including saturated AC-central pixels. The resulting 1D spectrum, which presents 99 saturated samples (marked in red), was discarded by the pipeline. The visible jumps (of ∼8000 e) originate from AC-central pixels exceeding 50 000 ADU (see Sect. 3.1). The corresponding star has grvs_mag = 3.471 ± 0.005 mag, Teff = 4735 K, log g = 1.45, and [Fe/H] = −0.13.

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