This was supplied in hardcopy only, for the purpose of the
Phase B review in Leiden on July 19 1999. The RSAA team was
thanked for its tremendous efforts.
Here is a summary (by Koen Kuijken) of the issues raised:
Technical issues:
- filter round or square. Decision requires us to check footprints of beam at
the location of the filter, as well as better understand the
manufacturing issues. Action by Nigel (optical design), NFRA (who will
make the hole).
- gratings. everybody happy with 600-line gratings in V
shape. 1200-line grating for single-grating mode would be great---cost this.
- AR coatings. Cost estimates to be verified. Could be significant overrun.
- Halpha arm. Concensus seems to be that operations at WHT could be
done with 3 observatory CCDs, but at TNG this is very unlikely. If we
want to acquire our own CCD for the Halpha arm, it might be desirable
to make this one that fits naturally into TNG's data acquisition system.
Could consider funding a TNG CCD on condition that we can use it for
PNS when required, in exchange for their maintaining it. It might
also be possible within the developing La Palma cooperatin agreement
to use a ING CCD at TNG. Action by Magda on TNG CCD, controller and
data acquisition situation; by KK on WHT situation.
- Matrix mask design to be finalized. Action Nigel
- Dichroic: manufacturer, cost? Action Nigel
- Ghost problem looks to be solved with the 600-line grating.
- Account details of AAO to be provided to Magda. Action KK
Halpha arm funding: explore possibility to find UK collaborator, who
would also bring in more WHT access. Mike Merrifield to be approached.
Lyman-alpha interlopers. Looks as if spectral resolution will catch
many of these (Ly alpha widths are larger than for PNe in known cases
from 2DF work). Otherwise Halpha or 4959 could be a useful diagnostic,
but not perfect since fainter than O[III] and hence not detectable in
faintest PNe. Checking results on nearby starbursts would be useful to
see how effective spectral OIII line width is as a discriminant.
Document date: October 14, 1999