The Pristine Inner Galaxy Survey (PIGS) - XI. Revealing the chemical evolution of the interacting Sagittarius dwarf galaxy

Open Access

Table 1

Observing setup used during the observation.

Filter	λ_in – λ_fin (nm)	R	< S/N >	Exp_time (h)
HR8	491.7–516.3	23 500	40	6.67
HR11	559.7–584	29 500	33	3.42
HR15N	647–679	19 200	53	1.65

Notes. Wavelength coverage, resolution, average signal-to-noise ratio, and exposure time of the GIRAFFE setups used for this work. The signal-to-noise ratio is given per pixel (1 pixel = 0.005 nm).

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