From: Saul Perlmutter (saul@lbl.gov)
Date: Fri Nov 15 2002 - 19:25:25 PST
Hi Mamoru and Kentaro -- and Chris,
What do you think the chances are now that you will be able to do any of
071 (or even complete your main 017 target) at Subaru/CISCO? If the odds are
beginning to look bad, then perhaps Chris should raise the priority of 071, even
with some thin cirrus, just to try to get _something_ on it in J- band. But
you guys all know better than me whether this is worthwhile --so Mamoru and
Kentaro, can you give us your opinion on the best odds?
Thanks, --Saul
Chris Lidman wrote:
> Dear Saul,
> This is a difficult call. SuF02-071, which, given its magnitude, probably
>
> needs clear conditions. However, given the priority of our program relative
> to other programs, I do not think we can get 10 hours of clear time on this
> object over the next few nights. We may have to accept thin cirrus to get
> any data at all. Since the object is faint, I am pessimistic about our
> chance
> on getting useful data on this target.
>
> SuF02-019 and SuF02-001 are brighter and can be done with some cirrus.
>
> As it currently stands, I have asked SuF02-071 to be observed in clear
> conditions
> and the other SNe to be observed in thin cirrus. The alternative is to
> accept thin
> cirrus for Suf02-071 and put this as the highest priority target.
>
> Cheers, Chris.
>
> Saul Perlmutter wrote:
>
> > Hello Chris,
> > One quick addition to Mamoru's email: When we were discussing the
> > CISCO & ISAAC plan, we were also thinking that the absolute highest
> > priority was to complete the high-redshift SNe, -071 and -017, with all
> > the other supernovae only getting IR observations if there really is
> > enough CISCO & ISAAC time available. (We cannot use the high-redshift
> > SNe unless we get the J-band data, while the lower-redshift SNe would be
> > useful anyway.) So we don't want to take any risk of using up the ISAAC
> > time on the lower-redshift supernovae if you don't think there would
> > still be enough time to complete the high-redshift SNe in the worst-case
> > scenario that CISCO doesn't manage to get either of them. (Also, we
> > really want these two high-redshift supernovae observed near maximum, of
> > course, and we were aiming to get the one that is being observed at the
> > end of November with HST another time with ISAAC at the end of November
> > to match.)
> >
> > I think your current plan doesn't yet run into this problem -- but
> > I'm not quite sure, since I don't know how the fact that we are not the
> > highest ISAAC priority of figures into this calculation. What do you
> > think?
> >
> > --Saul
> >
> > Chris Lidman wrote:
> >
> > > Dear Mamuro,
> > > I need to correct my previous e-mail. For SuF02-017, please read
> > > SuF02-071.
> > >
> > > Cheers, Chris.
> > >
> > > Chris Lidman wrote:
> > >
> > > > Dear Mamuro,
> > > > I will ask Paranal to observe
> > > >
> > > > SuF02-017 if the conditions are clear - 10 hour integration
> > > >
> > > > SuF02-001 if the conditions are not clear (ie thin cirrus) - 3 hour
> > > > integration
> > > >
> > > > SuF02-019 if the conditions are not clear - 3 hour integration.
> > > >
> > > > There is a bit of this cirrus at the moment.
> > > >
> > > > Cheers, Chris.
> > > >
> > > > Mamoru Doi wrote:
> > > >
> > > > > Dear Chris,
> > > > >
> > > > > We had no useful observations with CISCO on Nov.14.
> > > > > Again there was a trouble of the telescope (possibly
> > > > > the IR secondary support) and we saw strong astigmatism.
> > > > > We spent half night for Mirror analysis. The image quality
> > > > > was acceptable in the middle of the night. But then we had
> > > > > cloudy/hazy sky.
> > > > >
> > > > > We will change the secondary from IR to optical, which is
> > > > > more reliable with little disadvantages for CISCO J-band
> > > > > observations.
> > > > >
> > > > > -Mamoru and Kentaro
> > > > >
> > > > > 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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