Chemical depletion in the Large Magellanic Cloud: RV Tauri stars and the photospheric feedback from their dusty discs

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This article has an erratum: [https://doi.org/10.1051/0004-6361/200912982e]

Table 2:

Log of the UVES observations and the obtained final S/N at a given spectral band.
Star	Exp. time	Wavelength	S/N
	(s)	(nm)
MACHO 79.5501.13	3600	375.8-498.3	70
		670.5-1008.4	100
MACHO 81.8520.15	3600	478.0-680.8	70
MACHO 81.9728.14	3600	478.0-680.8	65

Note: The S/N is measured in the middle of the spectral window covered.

Source LaTeX | All tables | In the text

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