Last Updated Mar 24, 2017
JWST NIRCam coronagraphy offers round and bar occulting masks paired with pupil-plane Lyot stops, yielding inner working angles of 0.13"–0.88" HWHM.
Each NIRCam module includes a coronagraphic optical mount (COM) that carries three round and two bar-shaped coronagraphic occulting masks in the focal plane.
When centered on a bright point source, an occulting mask blocks the core of the point spread function (PSF). Diffracted light remaining in the PSF wings is blocked by a corresponding Lyot stop in the pupil plane. The pairing of the occulting mask and Lyot stop constitutes a coronagraph, which enables high-contrast imaging of faint features near bright point sources.
Three round occulting masks are available in the pupil plane with sizes optimized for observations at different wavelengths. Table 1 gives their radii (in arcseconds) and the wavelengths at which those radii correspond to 6 resolution elements, or 6 λ/D, where the D is the 6.5 m diameter of the JWST primary mirror. (Resolution at the diffraction limit is measured in units of λ/D.)
Table 1. 6λ/D wavelengths for the round occulting masks
Round coronagraphic mask
|Radius||λ for 6λ/D|
The 2 bar coronagraphic occulting masks are tapered, with radii varying by a factor of 3 along their lengths. Table 2 gives the half widths at half maximum (HWHM) at the bar end points and centers. Note these wavelengths extend beyond the observable range (see NIRCam Filters for Coronagraphy).
Table 2. 4λ/D wavelengths for the end points and center (in HWHM) of each bar coronagraphic mask
|Bar coronagraphic mask||HWHM||λ for 4λ/D|
In each module, NIRCam has two Lyot stops: one designed to suppress diffracted light from the round occulters, and the other to suppress diffracted light from the bar occulters. The final PSF is the Fourier transform of the Lyot stop.
Krist, J., et al., 2010, SPIE, 77313J
The JWST/NIRCam coronagraph flight occulters
Mao, Y., et al., 2011, SPIE, 81500E
NIRCam coronagraphic Lyot stop: design, fabrication, and testing
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