NGSTNGST ASWG 22 Oct. ASWG Charter & Role  NGST Scientific Goals & Metrics  Refine actual goals and put in DRM √  Refine DRM model assumptions √  Assist.

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Presentation transcript:

NGSTNGST ASWG 22 Oct. ASWG Charter & Role  NGST Scientific Goals & Metrics  Refine actual goals and put in DRM √  Refine DRM model assumptions √  Assist in developing scientific "metrics"  Recommend scientific "strategy" for achieving the balance between desires and feasibility  Represent NGST and the Community Interests  Key meetings (Decade Survey, OSS) √  Community interests in science goals √ √ = actual studies and/or homework, otherwise advisory JWST-PRES

NGSTNGST ASWG 22 Oct. ASWG Charter & Role Cont.  NGST Observatory Development  Review and advise on ISIM studies √  Assess design concepts and implementation plans for their scientific impact.  Help in formulating an operating scenario for NGST. √  Advise and assist Project in formulating Project Plans and solicitation strategies.  Participate in various IPTs and study teams √  Travel, travel, travel

NGSTNGST ASWG 22 Oct. Science Goals and Metrics  Current DRM is shaped to HST & Beyond and ideal 6-m monolith in terms of capabilities.  2.5 yr. core mission is not the GTO science program but represents a core science program to accomplish the OSS long-range goals, as we develop and present them.  Extended program should show potential of NGST but no single part should be a show-stopper.  The development and periodic modifications in the DRM must be done deliberately, in consultation with everyone!

NGSTNGST ASWG 22 Oct. Suggested Process  ASWG members will represent astronomical disciplines/subfields.  Each subfield may develop a small working group to propose science goals and document them.  ASWG to prioritize each goal/observations in either core or extended program.  Each goal has a "roadmap."  Priorities based upon overall importance and NGST uniqueness.  New DRM leads to solicitation of flight ASWG & ISIM

NGSTNGST ASWG 22 Oct. Suggested Science Disciplines  Early Universe -- the earliest stars, QSOs, reionization  Cosmic evolution of the elements -- star formation -- SNe -- the early IGM  The evolution of galaxies and galactic structure  Central, dusty AGN and star-forming regions  Stellar Populations  Stellar Astrophysics and Evolution  ISM  Star formation: processes, populations, IMF etc.  The formation of planets and planetary systems

NGSTNGST ASWG 22 Oct. Participate in Observatory Design  Attend ISIM, Architecture & Mirror Demonstrator Reviews.  Participate in IPTs, including Operability IPT.  Raise issues at reviews and also at ASWG meetings  Action items or new studies  DRM model upgrade and study  Perform specific technical studies that address impacts on scientific goals.

NGSTNGST ASWG 22 Oct. Suggested Technical Study Areas  Image quality and its effects on science  Detectors, what can we expect?  Formats, wavelengths, noise, stability  Electronic and thermal requirements.  Backgrounds and their effects on science  Mike Hauser will permit use of COBE model  Other orbits besides L2  Cosmic rays and rejection techniques  Data Archives and Analysis in the 21st Century

NGSTNGST ASWG 22 Oct. ASWG-approved Standards Science  Cosmology (   Early star cluster  Early Protogalaxy  z = 4 early spheroid  cold white dwarf  old brown dwarf  early protostar  young Jupiter-sized planet  Kuiper Belt Object. Technical  Zodiacal Background model.  Reflectivities, noise estimates, etc. for Yardstick.  Mirror temps, emissivity.  Sky coverage  GO usage: programs, times, etc.

NGSTNGST ASWG 22 Oct. NGST Census  Piero Madau is working on NGST Census -- how many and what kinds of objects will we see?  My early version looks interesting: