The NIRSPEC OH Page
All wavelengths are vacuum. Wavelengths from Abrams & Davis.
The wavelengths of unresolved lambda-doublets separated by less then two
pixels have been averaged. Doublets separated by between two and four pixels
have been deleted. Typically, a second order wavelength solution should
achieve fit residuals of < 0.02 A rms using these data.
James R. Graham
Professor of Astronomy
University of California
Berkeley CA 94720-3411
tel: (510) 642-8283
fax: (510) 642-3411
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Last updated July 2001