MIRI Point Spread Functions

The simulated JWST MIRI imaging point spread functions (PSFs) in each filter and predicted values for the full width at half maximum (FWHM), radial profiles, and encircled energy curves can be found using WebbPSF.

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Predicted point spread functions (PSFs) for every JWST instrument can be simulated using WebbPSF. Given a wavefront error budget for the mirror alignment, WebbPSF can create multiple realizations of the PSF with a given filter. Each of these realizations assumes various contributions to the wavefront error from several optical components, which cause the PSF shape and orientation to vary slightly.

WebbPSF allows the user to select between a "predicted" optical path difference (OPD) map and a slightly more conservative "requirements" OPD map. The following figures show one realization for MIRI imaging in each filter for the "requirements" OPD map. Below is some introductory information used to calculate the following PSFs.

At wavelengths λ > 2 μm, JWST obtains diffraction-limited imaging with a Strehl ratio = 0.8 and PSF full width at half maximum (FWHM) of ~λ/D radians (JWST's D = 6.5 m mirror). The MIRI detector achieves Nyquist sampling or better (FWHM > 2 pixels) above ~7 µm. Below these wavelengths, the PSF is undersampled. PSF sampling may be improved by performing dithers between exposures.

Simulated MIRI PSFs

The PSFs were made with a wavelength sampling of 10 wavelengths per filter and a pixel oversampling of 5. Both the detector and oversampled PSFs are centered on the pixel (rather than on the pixel corner).

Figure 1 shows the detector-sampled PSF with each MIRI filter on a log scale. Figure 2 zooms in to the cores of the PSFs.

Figure 1. One realization of simulated MIRI PSFs
MIRI PSFs with each filter were simulated by WebbPSF. Each PSF image is 109 × 109 detector pixels (~12.1" on a side). All are displayed with the same log scale. PSFs are shown in the detector pixel scale (0.111”).

Figure 2. One realization of simulated MIRI PSF cores

These are zooms into the central 18.02 × 18.02 pixels (2" on a side) of each simulated PSF shown in Figure 1. Each PSF is centered within a pixel, displayed with the same log scaling as Figure 1.


Figure 3 shows the FWHM as a function of the filter’s average wavelength for each simulated PSF. Numerical values for each FWHM, in units of arcsec and pixel, are reported in Table 1. These values were calculated with WebbPSF v0.7.0 using the PSF parameters described in the previous section. Note: due to undersampling below ~7 µm, the oversampled PSFs were used to calculate the FWHM.

Figure 3. PSF FWHM in each filter, as measured in one realization of simulated PSFs

This figure shows the FWHM measured for each of the oversampled PSFs simulated by WebbPSF, shown in Figures 1 and 2. Each point, color-coded by wavelength, corresponds to one of the 9 filters in Table 1.

Table 1. FWHM values for each PSF, from Figure 3

FilterWavelength (μm)PSF FWHM (arcsec)PSF FWHM (pixel)



Radial profiles

Figure 4 shows the radial profiles for each simulated, oversampled PSF. The radial profiles have been normalized to the value of the peak pixels.

Figure 4. PSF radial profiles

In these plots of the radial profiles for each simulated PSF, the pixel size (0.11") is reported in each panel as a dotted line.

Encircled energy

Figure 5 shows the encircled energy curves for each simulated, oversampled PSF. Numerical values for 50% and 80% encircled energy (the fraction of light contained in a circular aperture) can be found both in Figure 5 and Table 2.

Figure 5. PSF encircled energy curves

In these encircled energy curves for each PSF, the radius (in arcsec) at which the encircled energy is 50% and 80% is reported in the Figure 5 and in Table 2.

Table 2.  Radius (in arcsec and pixels) at which the encircled energy (EE) is 50% and 80%

Filterradius(EE=50%) (arcsec)radius(EE=50%) (pixel)radius(EE=80%) (arcsec)radius(EE=80%) (pixel)


Figures and tables on this page were generated using the 0.9.1 development version of WebbPSF.

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