From: Lori Lubin (lubin@physics.ucdavis.edu)
Date: Tue Jan 24 2006 - 16:42:27 PST
We have not quantified it entirely, but based on the first look, we also
see a higher fraction in the field.
Cheers,
Lori
On Tue, 24 Jan 2006, Marc Postman wrote:
> Yes true - do you also see a higher fraction of [OII} emission for
> ellipticals not in the cluster but at those same redshifts? I believe
> we saw some evidence for this in Postman, Lubin, Oke 2001.
>
> On Jan 24, 2006, at 4:00 PM, Lori Lubin wrote:
>
> > Hi Marc,
> >
> > That is very interesting. It should be noted (though probably not in
> > this proposal) that about 60% of the spectroscopically-confirmed
> > red-sequence galaxies in the ACS field of CL1604+4304 at z = 0.9 show
> > detectable [OII] emission in our DEIMOS spectra. This suggests at
> > least some star formation in the cluster early-types at these
> > redshifts. it is important to get high S/N and
> > high-spectral-resolution spectroscopy to quantify this accurately.
> >
> > Cheers,
> > Lori
> >
> -----------------------------------------------------------------
> Marc Postman Email: postman@stsci.edu
> STScI - CMO Phone: +1-410-338-4340
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>
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