From: clidman@eso.org
Date: Mon Nov 11 2002 - 08:56:36 PST
Hi Lifan,
The 2D FORS2 spectrum is available from http://www.sc.eso.org/~clidman/.
The line at 9178 is complex.
Cheers, Chris.
Lifan Wang wrote:
> Mamoru,
>
> On Keck spectrum, it seems the 9178 A is resolved into a doublet
> with split being consistent with [O II] identification.
>
> Lifan
> > From owner-deepnews@listserv.lbl.gov Sun Nov 10 20:51:04 2002
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> > Subject: Re: Lifan thinks we see the other NeV line for 026, implying
> > it's an AGN
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> >
> > Hi,
> >
> > I don't see NeV3426 at ~8430A on VLT spectrum.
> > Plobably in the Keck spectrum?
> >
> > Though I understand that this is not
> > a straight explanation, but how about the
> > following combinations?
> >
> > 9179 Hbeta(4863-4853)
> > 8263 Hgamma(4342-4346)
> > at z=0.90
> >
> > The latter wavelengths are from SDSS composite QSO
> > spectra (D.Vanden Berk et al. AJ, 122, 549-564, 2001)
> > I got this idea from Fig.6 of this paper
> > when I tried to fit those two lines with
> > SiIV and CIV (at z=4.92).
> >
> > The lines are not broad very much,
> > but the line at 9179 seems to me slightly
> > larger than velocity rotation/dispersion
> > of usual galaxies. There might be weak
> > broad-line components in this galaxy.
> >
> > The both photo-z codes give z=0.8 for this galaxy.
> >
> > Do we see [OIII] at 9510? Mmm...
> >
> > -Mamoru
> >
> > >Lifan thinks we see the other NeV line (restframe 3426 A) for 026,
> > >implying it is, in fact, an AGN, as we were suspecting. This also fits
> > >the fact that it is too bright for its redshift (z = 1.46) if were a
> > >normal SN Ia.
> >
> >
> >
> > 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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