Hi Tomoki,
   I've compared the listed redshifts with those that were measured at 
the
VLT for objects that are common.

Object          Subaru VLT    VLT classification
==================================
SuF02-060 1.062     1.063 Ia*
SuF02-065 0.554     1.181 Ia

They are both interesting candidates.

SuF02-060
----------------

There was some doubt in the classification. With a spectrum of the host 
without
the SNe, we might be able to make a more secure classification.

SuF02-065
---------------

The classification is secure. The redshift is based on identifying 
[OII]. I believe this
is a case of a distant SN with a faint host and bright nearby galaxy.

SuF02-061
---------------

There was an earlier Subaru spectrum of SuF02-061. From that spectrum,
I measured z=1.085 from a number of lines.  See

http://www.sc.eso.org/~clidman

Regards,

Chris.


On Apr 4, 2005, at 11:33 AM, Tomoki Morokuma wrote:

> Dear Gerson,
>
> I have received spectroscopic results in last fall in the SXDS
> from a person who analyzes Subaru/FOCAS data.
>
> See the table on the web.
> http://www.ioa.s.u-tokyo.ac.jp/~tmorokuma/study/SN/subaru2002fall/host>
> 6 host galaxies are identified, but one (SuF02-097) is an AGN.
> In the list of SNe whose redshift you want to know,
> only SuF02-004 with "brass quality" light curve
> turns out to be at z=1.187.
>
> Thank you.
>
> Tomoki
>
>>> 'SuF02-004','SuF02-034','SuF02-051'
>>>      .95        .9          1.3
>>>      c          a            a
>>>
>>> SuF02-056','SuF02-057','SuF02-058','SuF02-068',
>>>     .82        1.5         .95         --
>>>      b           a          a          d
>>>
>>> 'SuF02-076','SuF02-079','SuF02-086','SuF02-J01','SuF02-J02'
>>>     1.4         0.96        1.4           1.08     1.08
>>>     a*             c          c            b          a
>>>
>>> ,'SXDS_1-a','SXDS_1-b','SXDS_2-4','SXDS_2-9','SXDS_4-3'
>>>     1.05          0.75     0.5        0.8       --
>>>       a          a          a         a           d
>>>
>>> These are the SNe which need a spectrum measurement.
>>> a= gold quality   a* very narrow, not Ia ?
>>> b= silver quality
>>> c= brass quality
>>> d= no good light curve
>>> the z values are given as estimated from the light curves (very
>>> approximate)
>>> the spectra should be taken starting with the highest z and highes 
>>> quality