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Wide-Field Slitless Spectroscopy with JWST's NIRISS

  • William V. Dixon (a1), Swara Ravindranath (a1) and Chris J. Willott (a2)

Abstract

The Near Infrared Imager and Slitless Spectrograph (NIRISS) aboard the James Webb Space Telescope (JWST) will offer wide-field slitless spectroscopy (WFSS) with a resolving power R = 150 at wavelengths from 0.8 to 2.25 microns. In this band, NIRISS will be sensitive to Lyman α emission lines and continuum breaks in the spectra of galaxies with redshifts 6 < z < 17, allowing it to probe the first stars and ionizing sources in the early universe. NIRISS observations of the high-redshift universe will provide a wealth of information on foreground objects, creating a unique library of optical emission-line spectra from the faintest galaxies at lower redshifts. To explore its ability to identify and characterize galaxies at all redshifts, we have modeled a NIRISS observation of a massive strong-lensing galaxy cluster and analyzed the synthetic images using standard software tools. Our simulations demonstrate that WFSS with NIRISS will provide a powerful tool for the exploration of galaxies near and far.

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Copyright

References

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Bertin, E. & Arnouts, S. 1996, A&AS, 317, 393
Dixon, W. V. & Willott, C. J. 2013, STScI Newsletter, 31 (2), 28
Kümmel, M., Walsh, J. R., Pirzkal, N., Kuntschner, H., & Pasquali, A. J. 2009, PASP, 121, 59
Postman, M. et al., ApJS, 199, 25
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Keywords

Wide-Field Slitless Spectroscopy with JWST's NIRISS

  • William V. Dixon (a1), Swara Ravindranath (a1) and Chris J. Willott (a2)

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