report on jwst science working group tucson, 10-11 feb 2004

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1 Report on JWST Science Working Group Tucson, 10-11 Feb 2004

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Report on JWST Science Working Group Tucson, 10-11 Feb 2004. Major news. No intention of accelerating the schedule. A list of items suitable for risk reduction is being prepared by the JWST project and were briefly discussed by the SWG. Instruments ok. JWST Field of View Layout. Major news. - PowerPoint PPT Presentation

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Page 1: Report on JWST Science Working Group Tucson, 10-11 Feb 2004

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Report on JWST Science Working GroupTucson, 10-11 Feb 2004

Page 2: Report on JWST Science Working Group Tucson, 10-11 Feb 2004

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Major news No intention of accelerating the schedule. A list of items

suitable for risk reduction is being prepared by the JWST project and were briefly discussed by the SWG.

Instruments ok.

Page 3: Report on JWST Science Working Group Tucson, 10-11 Feb 2004

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JWST Field of View Layout

Page 4: Report on JWST Science Working Group Tucson, 10-11 Feb 2004

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Major news No intention of accelerating the schedule. A list of items

suitable for risk reduction is being prepared by the JWST project.

Instruments ok.

Page 5: Report on JWST Science Working Group Tucson, 10-11 Feb 2004

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Major news No intention of accelerating the schedule. A list of items

suitable for risk reduction is being prepared by the JWST project.

Instruments ok. NIRCam : PIL is #1 risk reduction item. Tip-tilt focus mechanism.

Page 6: Report on JWST Science Working Group Tucson, 10-11 Feb 2004

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NIRCamPupil Imaging Lens would go here.

One half of NIRCam

OTE

Pick-off mirror andTip-tilt-focus mech.

Page 7: Report on JWST Science Working Group Tucson, 10-11 Feb 2004

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Major news No intention of accelerating the schedule. A list of items

suitable for risk reduction is being prepared by the JWST project.

Instruments ok. NIRCam : PIL is #1 risk reduction item. Tip-tilt focus mechanism. NIRSpec: issue of pupil shear, potential loss of sensitivity in

NIRSpec 14-15% for 5% shear. Swiss company has produced cryogenic mechanical slit selector (backup to MEMS)

SWG will carry out trade study for 1/10/100 slits by June 04 MIRI: shear also an issue for coronagraph. Extra background at

>20m. FGS-TF: the SWG voted for uninterrupted wavelength coverage

up to 5 m. Survey Fields

Page 8: Report on JWST Science Working Group Tucson, 10-11 Feb 2004

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Backgrounds – South galactic cap

Red = galactic dust, green = ecliptic declination, blue = selected fields (low dust, no bright stars, galaxies, radiosources)

Page 9: Report on JWST Science Working Group Tucson, 10-11 Feb 2004

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Backgrounds – South galactic cap

Red = galactic dust, green = ecliptic declination, blue = existing fields (symbol size proportional to quality)

Page 10: Report on JWST Science Working Group Tucson, 10-11 Feb 2004

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Major news – cont’d Discussion on need for some form of science parallels Long discussion about HST-JWST Legacy

JWST science may require visible imaging data How do we make sure those data are there when

needed? Full range of opinions (from do nothing to ask for a

fraction of HST time to be set aside). Too early for promising a JWST Quick look survey Agreement on doing nothing but informing the user

community about what JWST can and cannot do and where in the sky

Write a JWST Mini-handbook (?)