Opportunities with the James Webb Space Telescope
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1 Opportunities with the James Webb Space Telescope Nancy A. Levenson Space Telescope Science Institute image credit: J.Dore
2 JWST NASA, ESA, and CSA 6.5m mirror cooled instruments cover nearthrough mid-infrared imaging, spectroscopy, coronagraphs, integral field units, etc.
3 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
4 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
5 progress with testing
6 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
7 telescope
8 instruments NIRISS MIRI NIRCam NIRSpec
9 at Johnson Space Center
10 sunshield at Northrop Grumman
11 spacecraft bus at Northrop Grumman
12 telescope and sunshield at Northrop Grumman
13 October 2018
14 JWST s journey
15 deployment
16 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
17 science timeline you are here
18 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 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
19 resources: observer website jwst.stsci.edu
20 resources: pocket guide
21 resources: documentation and helpdesk jwsthelp.stsci.edu jwst-docs.stsci.edu
22 resources: observer website news and events Youtube: JWST Observer Channel Facebook: JWST Observer jwst.stsci.edu
23 resources: JWST Users Committee (JSTUC) chair: James Bullock, University of California Irvine jwst.stsci.edu/science-planning/user-committees
24 resources: outreach webbtelescope.org
25 webbtelescope.org
26 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
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