NIRCam Coronagraphic Occulting Masks and Lyot Stops

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.

On this page

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.

Occulting masks

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 six 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

Radiusλ for 6λ/D
MASK210R10.40"2.1 μm
MASK335R0.63"3.35 μm
MASK430R0.81"4.3 μm

The two bar coronagraphic occulting masks are tapered, with radii varying by a factor of three 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 maskHWHMλ for 4λ/D


0.13"1.03 μm
0.26"2.1 μm
0.39"3.1 μm


0.29"2.3 μm
0.58"4.6 μm
0.87"6.9 μm

When a bar mask is used with a given filter, the source is placed behind the occulter at a position (shown in Figure 1) that provides HWHM = 4λ/D for the central wavelength λ of the filter.

Figure 1. NIRCam bar occulting masks and their corresponding nominal pointing positions for each filter

The NIRCam module A coronagraphic substrate is shown with marked nominal pointing positions for each filter. The large back rectangles correspond to the neutral density filters.
Figure 2. NIRCam coronagraphic occulting masks

NIRCam coronagraphic occulting masks and neutral-density squares for target acquisition

The NIRCam module A coronagraphic substrate, which includes bar and round masks for occulting bright objects and 5" × 5" neutral density squares for acquisition of bright targets (K < 12). The three lines of information at the top are the nominal wavelength range, mask name, and inner working angle for each occulting mask. The etched metal patterns deliver the desired radial profiles within tolerances. Adapted from Krist et al. 2010, Figure 3.
The filter transmission changes with radius and is different for each occulting mask (Figure 2).
 Figure 3. Filter transmission as a function of distance for round and bar masks

Transmission changes with distance and with the occulter. The plots for the bar masks show the allowed filter range. Vertical lines mark the 50% transmission point. The files used to create these plots are available here: transmissions.tar.
Bold italics style indicates words that are also parameters or buttons in software tools like the APT and ETC. Similarly, a bold style represents menu items and panels.

Lyot stops

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.

Figure 4. NIRCam coronagraph diffraction and Lyot stops

Diffraction from the NIRCam occulting masks (top row) and Lyot stops designed to suppress diffracted light (bottom row) from the round occulters (left) and bar occulters (right). In all images, white indicates light transmission. Adapted from Mao et al. 2011, Figure 3.


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



Latest updates
    Added figure: nominal pointing positions

    Added figures: transmission vs. radius