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This atlas is intended at providing a useful tool for the wavelength
calibration of the VLT/ISAAC and NTT/SOFI spectra. Since OH lines
are imprinted on all sky spectra (provided they are deep enough, which
might not always be the case for standard stars), they provide
an in-situ reference for wavelength calibrating the spectra.
The material presented in this document is published in A&A.
If you publish using the content of this document, please refer to:
Rousselot et al., 2000, A&A, in press.
Jean Gabriel Cuby