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James Webb Space Telescope
Near-InfraRed Imager and Slitless Spectrograph

NIRISSA science instrument known as the Near-InfraRed Imager and Slitless Spectrograph (NIRISS) is packaged with the guide camera (FGS), but is functionally independent. The NIRISS will be capable of wide-field grism spectroscopy with R~150 between 1.0 – 2.5 microns; single-object grism spectroscopy with R~700 between 0.6 – 3.0 microns; aperture-masking interferometry with a non-redundant mask (NRM) between 3.8 - 4.8 µm; and broad-band imaging across its 2.2' x 2.2' field between 1.0 - 5.0 µm. NIRISS is expected to contribute to all of the JWST Science Themes: 1) The End of the Dark Ages: First Light and Reionization; 2) The Assembly of Galaxies; 3) The Birth of Stars and Protoplanetary Systems; and 4) Planetary Systems and the Origin of Life.

The Canadian Space Agency is providing the NIRISS to the JWST Project. The prime contractor is Com Dev. The Principal Investigator for the NIRISS is René Doyon from the Université de Montréal.

Latest News

2014 March 13
A revised version of NIRISS Pocket Guide is now available on NIRISS Document Archive.

2013 October 29
NIRISS completed its first suite of tests under cryogenic conditions in the large vacuum chamber at NASA's Goddard Space Flight Center. The tests featured "first light" observations for all the observing modes of NIRISS. Although a few glitches occurred, initial analysis of the test data show that NIRISS is performing marvelously.

2013 March 1
Integrated Science Instrument ModuleNIRISS and the FGS became the first flight instruments to be attached to the Integrated Science Instrument Module (ISIM), which is currently located in the large clean room at NASA's Goddard Space Flight Center.

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