Re: Hbeta ?

From: Mamoru Doi (doi@ioa.s.u-tokyo.ac.jp)
Date: Sun Nov 10 2002 - 23:16:30 PST

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Lifan and Chris,

O.K. Then there is little doubt about z=1.46.
The line at 8263.4A may not completely correspond
the wavelength of [NeV] 3346.8, but I have no
better idea than that.

-Mamoru

> On Keck spectrum, it seems the 9178 A is resolved into a doublet
>with split being consistent with [O II] identification.

Mamoru Doi
Institute of Astronomy
School of Science
University of Tokyo
voice +81-422-34-5084
fax. +81-422-34-5041
doi@ioa.s.u-tokyo.ac.jp

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