The NIRSPEC OH Page



 

NIRSPEC-5 OH

  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
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University of California
Berkeley CA 94720-3411

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Last updated July 2001