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Re: scaling the sne back a little
- To: Ray Carlberg <carlberg@astro.utoronto.ca>
- Subject: Re: scaling the sne back a little
- From: David Schade <david.schade@nrc.ca>
- Date: Fri, 11 May 2001 08:02:14 -0700
- CC: Christian Veillet <veillet@cfht.hawaii.edu>, Laurent Vigroux <vigroux@discovery.saclay.cea.fr>, Olivier LeFevre <Olivier.LeFevre@astrsp-mrs.fr>, Yannick Mellier <mellier@iap.fr>, Annie Robin <annie.robin@obs-besancon.fr>, Richard Wainscoat <rjw@IfA.Hawaii.Edu>, JJ Kavelaars <kavelaars@physics.mcmaster.ca>, Alain Blanchard <ablancha@ast.obs-mip.fr>, Ray Carlberg <carlberg@moonray.astro.utoronto.ca>, David Schade <David.Schade@hia.nrc.ca>
- References: <200105111457.f4BEvGN04416@qold.astro.utoronto.ca>
Ray,
As you point out, this is a very major cost. I see it as a drastic cutback.
David
Ray Carlberg wrote:
> How could we scale back a little? For the supernovae, the sampling
> rate can't change without endangering the program. However, to be most
> valuable the sampling has to relatively uniform with no big
> gaps. Although the "poor weather" months of Jan and Feb are acceptable
> time to observe, the Sne program could, if absolutely necessary, be
> suspended for those months. The sole purpose of this would be to
> lower the time request by about 15% (since when it is clear in those
> months, there are many dark hours!). Introducing the hiatus does lead
> to a cost, which is that any Sne that are on the rise in late December
> are "lost". This would of course lower the total number of sne by a
> total amount of 15+(5-10)= 20-25% from the request (detailed modelling
> will be done next week.).
>
> This discussion shows a possible scale-back, but shows that the costs for
> synoptic observations are larger than the scale-back itself.