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Cosmic Origins Spectrograph Instrument Handbook for Cycle 17

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6.4 Image Characteristics


Figure 6.2 shows an image of a point source obtained in ground testing as seen on the NUV MAMA (i.e., fully corrected for HST's aberrations). A 2-dimensional Gaussian fit to this PSF has the following characteristics:

FWHM: 1.93 pixels = 45.5 mas

Fraction of light in brightest pixel: 14.3%.

Figure 6.2: Two-dimensional PSF for COS in imaging mode.


 

Figure 6.3 shows the profile through the PSF of Figure 6.2 in the x direction.

Figure 6.3: Profile through COS imaging PSF in the x direction.


 
This is a slice through the center of the profile.
 

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