'Jwst' diaporamas de présentation

The James Webb Space Telescope

The James Webb Space Telescope. Peter Stockman STScI. JWST. Introduction Architecture overview Project Status Science Capabilities Optical Performance Science Instruments JWST Science 4 Science Themes Ices in YSO disks Lab Astro needs Summary. JWST Observatory : Overview.

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Resolved Stellar Populations in the Near IR

Resolved Stellar Populations in the Near IR. Jason Kalirai (STScI). Outline - Frontier science opportunities for JWST in the arena of resolved stellar populations. - Characteristics of JWST that will enable this science. - Some hints from Hubble. - Synergies with HST, LSST, and GSMT.

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The Final (?) Frontier of Star and Planet Formation: Piled Deeper and Wider Michael R. Meyer

The Final (?) Frontier of Star and Planet Formation: Piled Deeper and Wider Michael R. Meyer Institute for Astronomy, ETH, Zurich, Switzerland 8 June 2011, Frontier Science Opportunities with the James Webb Space Telescope. Context for JWST in Kourou:. COROT/Kepler as well as

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JWST and MIRI STATUS

JWST and MIRI STATUS. Dutch MIRI Day June 3 rd at ASTRON (Hooghoudt room) JWST and MIRI STATUS Bernhard Brandl. JWST STATUS. JWST STATUS. Heading. Heading. Heading. Heading. JWST STATUS. JWST STATUS. BUT:. JWST STATUS. In January, the director of astrophysics at GSFC, Jon.

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Mid-InfraRed Instrument (MIRI) Delta-Systems Requirements Review: March 9

Mid-InfraRed Instrument (MIRI) Delta-Systems Requirements Review: March 9. Margaret Meixner MIRI support scientist. Result of MIRI delta-SRR. MIRI project successfully completed the delta System Requirements Review.

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JWST Science Timeline: Current Status

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The JWST Detector Characterization Project in the Independent Detector Testing Laboratory

The JWST Detector Characterization Project in the Independent Detector Testing Laboratory Don Figer, STScI/JHU January 9, 2003 AAS 201 Seattle, WA. 4. 1.E+02. Sunshield. Dark current =. -. 0.126 e. /sec. 1.E+01. -. 0.020 e. /sec. Spectra. 3. JWST requirement. -.

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The JWST Detector Characterization Project in the Independent Detector Testing Laboratory

The JWST Detector Characterization Project in the Independent Detector Testing Laboratory Don Figer, STScI/JHU January 9, 2003 AAS 201 Seattle, WA. 4. 1.E+02. Sunshield. Dark current =. -. 0.126 e. /sec. 1.E+01. -. 0.020 e. /sec. Spectra. 3. JWST requirement. -.

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JWST Status

JWST Status. Eric P. Smith JWST Program Scientist. Topics. JWST Cost Growth Science Assessment Team Findings and Program Response JWST Plans. Recent Programmatic Changes. ~$1B net cost growth ~$180M at NGST and ~$35M at subs Reevaluation of I&T effort (metrology, GSE)

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JWST calibration requirements

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

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.

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Introduction: Goals for JWST Transit Meeting

Introduction: Goals for JWST Transit Meeting. C. Beichman Jonathan Lunine March 11, 2014. JWST and Exoplanets.

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AMES Space Science & Astrobiology Division Strategic Plan YIR

AMES Space Science & Astrobiology Division Strategic Plan YIR. Laboratory Astrophysics and Astrochemistry. L. Allamandola , S. Bejaoui , P. Bera , C. Boersma , J. Bregman , G. Cruz-Diaz, D. Dubois, L. Gavilan, X. Huang,

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Coronagraphic characterization of exoplanets with the instrument MIRI of the JWST

4 coronagraphs in MIRI/JWST : 10.65, 11.40, 15.50, 23 m m. Coronagraphic characterization of exoplanets with the instrument MIRI of the JWST. Cavarroc C . & Boccaletti A. (CEA/Saclay, Obs. Paris). - Target samples : 850 F-L stars (distance and age constrained) Planets generated with MC

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