Opportunities with the James Webb Space Telescope

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Transcription:

Opportunities with the James Webb Space Telescope Nancy A. Levenson Space Telescope Science Institute image credit: J.Dore

JWST NASA, ESA, and CSA 6.5m mirror cooled instruments cover nearthrough mid-infrared imaging, spectroscopy, coronagraphs, integral field units, etc.

Ultra Sensitive and High Resolution Imaging Mid IR IFUs Single Object and Wide-Field Slitless Spectroscopy Space Based MOS Moving Target Support Bright Object Modes Near IR IFUs Science Capabilities NIR and MIR Coronagraphy

delay and current schedule NASA now planning for March 2021 launch delay (from 2018) announced in March 2018, following independent review board primarily requiring time for integration and testing secondary issue of sunshield fasteners

progress with testing

opportunities with current schedule with extra time, improvements that will especially benefit users: increase operational efficiency tools and documentation for users will be improved some options: Jupyter notebook infrastructure; light version of Exposure Time Calculator; cloud hosted data analysis infrastructure lessons learned from original Cycle 1 process Hubble example: find all IR sources in 2 minutes

telescope

instruments NIRISS MIRI NIRCam NIRSpec

at Johnson Space Center

sunshield at Northrop Grumman

spacecraft bus at Northrop Grumman

telescope and sunshield at Northrop Grumman

October 2018

JWST s journey

deployment

JWST Commissioning Phase (6 months) Phase I - Commission the Spacecraft (30 days) Launch and mid-course corrections Deployment of solar arrays, sunshield, mirrors Subsystem checkouts NIR instrument cooldown modifications Phase III - Commissioning the Science (60 days) Each instrument is independently focused, calibrated, and characterized Science instruments participate in observatory level tests (thermal slew, stray light, mechanism disturbance, moving target) Begin ERO, DD-ERS, Cycle 1 science and calibration programs Phase II - Commissioning the Telescope (90 days) Fine phasing of Optical Telescope Element (OTE) with NIRCam & Fine Guidance Sensors NIR instruments are activated and checked out MIRI cooldown via the cryocooler All science instruments used to align and optimize OTE

science timeline you are here

Director s Discretionary Early Release Science (DD-ERS) 13 approved programs across all science areas, using most key instrument modes selected programs have 253 investigators + 456 additional collaborators ~500 hours observing time observations soon after commissioning (mostly within 3 5 months) no exclusive access (proprietary period) eligible for archival research in Cycle 1 science teams will deliver science-enabling products, beyond raw data e.g., software for analysis, reduced data, leading workshops

resources: observer website jwst.stsci.edu

resources: pocket guide

resources: documentation and helpdesk jwsthelp.stsci.edu jwst-docs.stsci.edu

resources: observer website news and events Youtube: JWST Observer Channel Twitter: @JWSTObserver Facebook: JWST Observer jwst.stsci.edu

resources: JWST Users Committee (JSTUC) chair: James Bullock, University of California Irvine jwst.stsci.edu/science-planning/user-committees

resources: outreach webbtelescope.org

webbtelescope.org

summary March 30, 2021: JWST launch ~April 2020: Cycle 1 proposals due jwst.stsci.edu jwst-docs.stsci.edu ~January 2020: Cycle 1 call for proposals Start planning early! Complex instruments and modes jwsthelp.stsci.edu webbtelescope.org