From: Andrew Fruchter (fruchter@stsci.edu)
Date: Thu Apr 08 2004 - 09:12:28 PDT
Adam told me he had a direct image in every visit.
Your Phase II relies on a sole pointing for the offset between the
grism and the direct image. We can probably align the grism spectra
using something like tweakshifts. The only problem then may be a
small error in the spectral zeropoint (of order a fraction of an ACS
pixel -- perhaps 30A if we are not particularly lucky).
Andy
On Apr 7, 2004, at 3:26 PM, Rachel G. wrote:
>
> Hi Andy,
>
> I realized this would mean we'd have to think more, as
> opposed to using the Pirzkal et al. software in the
> straightforward way with the direct image and so forth. We
> do have some of Adam's data from last year, and I'd planned
> to start figuring out how to deal with it as soon as I'm
> back in Berkeley. Vallery Stanishev in Stockholm will also
> be working on this.
>
> Have you heard or do you have a sense for how large the
> calibration errors that will creep in might get? Because, I
> also thought Adam worked in this same mode. He could not
> have done all his observations in one Visit. And, as you
> know, his results look super.
>
> Ciao,
>
> Rachel
>
> On Wed, 7 Apr 2004, Andrew Fruchter wrote:
>
>> Hi Searchers,
>>
>> I have just approved visits F0-F5 for observation. However, you
>> should
>> know that you are using a very non-standard approach to grism
>> observations. You are not taking a direct image in each visit (indeed
>> the standard mode takes one associated with each dither position).
>> This opens you up to the possibility of sub-pixel shifts between the
>> direct image and the grism spectra.
>>
>> In principle one generally should not need a direct image. One should
>> be able to use the zeroth order image (and this could be a more
>> accurate way to align spectra in many cases). However, the
>> calibration
>> work necessary for this approach to be used has not been done, as far
>> as I know.
>>
>> Cheers,
>> Andy
>>
>
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