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Hubble Science Briefing Delivering JWST Science, from Exoplanets to First Light: The N ear- I nfra R ed I mager and S litless S pectrograph (NIRISS) March 6, 2014 Alex Fullerton (STScI). Agenda for Today. The Science Themes of JWST What is NIRISS and How Can It Help? Hardware
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Hubble Science Briefing Delivering JWST Science, from Exoplanets to First Light: The Near-InfraRedImager and Slitless Spectrograph (NIRISS) March 6, 2014 Alex Fullerton (STScI)
Agenda for Today The Science Themes of JWST What is NIRISS and How Can It Help? Hardware Observing Modes What’s happening next ? Your Questions!
James Webb Space Telescope Maryland Science Center, Baltimore’s Inner Harbor (2011 October 23)
The Frontiers of Knowledge: Science Themes of JWST 2.) Determine how galaxies evolve from the early Universe to the present day 1.) Seek the first stars and galaxies that formed in the early Universe 4.) Probe the chemistry of solar systems (including our own) to constrain the building blocks of life 3.) Solve the mysteries of star formation and birth of protoplanetary systems 5
JWST: Four Instruments NIRCam Near Infrared Camera NIRSpec Near Infrared Spectrograph MIRI Mid-Infrared Instrument NIRISS
What’s in a Name? Recall: The Discovery of Infrared Radiation Sir William Herschel’s Experiment 1800 Feb. 11 From: “Infrared Beyond the Visible” http://webbtelescope.org/webb_telescope/science_on_the_edge/beyond_the_visible/
“Slitless” Spectroscopy An objective prism spectrogram of a region near Gamma Cygni, taken October 16 – 17, 1950 with the 24-inch Schmidt telescope of the Warner and Swasey Observatory. The exposure was 4 minutes on Eastman IIa-O blue-sensitive emulsion by Daniel L. Harris. Objective Prism Spectroscopy Spectrographs typically use an entrance aperture (“slit”) to improve the resolving power (especially for spectrographs on ground-based telescopes) and to limit the region of the sky that enters the instrument. For example: A technological marvel developed for NIRSpec is the Multi-Shutter Array (MSA), which allows many slits to be configured “on the fly.”
FGS / NIRISS Fine Guidance Sensor (FGS) The camera to acquire targets and guide on them during observations. Used for purely functional purposes. Supplied by CSA. Prime Contractor: COM DEV International Optical Bench • NIRISS • A science instrument. • Supplied by CSA. • Prime Contractor: • COM DEV International • Principal Investigator: • René Doyon, Université de Montréal
Schematic: Optical Layout Image from Telescope
Enabling Elements Pupil Wheel Filter Wheel
Exoplanet Transit and Eclipse Science Seager & Deming (2010, ARAA, 48, 631) Precision needed: 1 part in 1,000 Transit Learn about atmospheric circulation from thermal phase curves Measure size of planet. Precision needed: 1 part in 100 See starlight transmitted through planet atmosphere. Precision needed: 1 part in 10,000
GR700XD Grism Weird Stuff! Prism: ZnS (Zinc Sulfide) Grism: ZnSe (Zinc Selenide) weak cylindrical surface (lens) Grism Side Prism Side
Real Data vs Simulations ISIM CV1 (October 2013) 2.5 microns 0.5 microns Simulation (U. de Montréal) 2nd Order 1st Order
Spectroscopy of the “Water World” GJ1214b Input spectrum Simulated NIRISS spectrum
JWST: First Light, First Galaxies JWST will Study the First Galaxies Simulation (U. de Montréal)
The First Galaxies HST can already see galaxies formed within 500 Myr of the Big Bang (redshift, z = 11). But neither Hubble nor JWST imaging will be able to measure the star formation rate or chemical evolution of these early galaxies. Instead: we need spectroscopy to detect spectral lines of hydrogen and oxygen to measure the detailed properties of the very first galaxies assembling from the products of the first stars, and to confirm their redshifts. 21
MACS J0647+7015: Image in NIRISS F200W HST Image: Composite of ACS and WFC3 exposures. Credit: NASA, ESA, M. Postman and D. Coe (STScI), and the CLASH Team. Simulation of the CLASH field through the NIRISS F200W filter by Chris Willott (NRC) and Van Dixon (STScI).
MACS J0647+7015: GR150R Grism GR150R Disperses Along Rows F200W Simulations by Willott and Dixon
MACS J0647+7015: GR150C Grism GR150C Disperses Along Columns F200W Simulations by Willott and Dixon
Extract Spectra From Both OrientationsAnd Identify Spectral Features Filter Image GR150R GR150C Hydrogen Emission at redshift of 9.25 GR150R GR150C Brightness Simulations by Willott and Dixon
What’s Happening Now? NIRCam is being worked on back here. ISIM Structure NIRSpec MIRI Stand for NIRCam http://www.jwst.nasa.gov/webcam.html
What’s Happening Next? Cryogenic Vacuum (CV) Testing at Goddard Space Environment Simulator One down, two to go ISIM being lowered into the SES chamber before CV1
Then: the Fun Really Begins! Thanks for your continued interest and support !
For More Information Arrival at Goddard Space Flight Center 2012 July 30