This section highlights some typical FOC image characteristics. Rather than trying to present examples of every possible mode, we focus on the f/96 imaging mode, because it is the most commonly used. Examples of f/48 images, f/48 longslit spectra, and prism images appear in later sections.
Commonly Observed FeaturesIf your FOC data are well-exposed, you might see one or more of the following:
- Occulting fingers located near the aperture entrance if the image size is greater than 512 x 512 pixels or if the FUV prism is in the beam.
- Reseau marks etched onto the faceplate of the detector to aid in geometric correction (Figure 4.4).
- Blemishes (scratches on the faceplate, Figure 4.4).
- Vertical intensity variations along the right edge of the image (due to a -variation in camera scan speed).
- A faint diagonal parallel striping pattern called pattern noise. After geometric correction your images may additionally show:
- A very faint moiré pattern ("thumbprint"), which is a variation of the noise, not the signal, caused by the geometric correction (Figure 4.5).
- Warped edges (Figure 4.4).
Figure 4.4 is a positive rendition of an f/96 (F430W) 512 x 512 image of the reflection nebula LK-H alpha 233. The image has been fully calibrated by the FOC pipeline and shows features that are common in any well-exposed FOC image. The regular grid of Reseau spots are used for geometric distortion calibration. The warped edges are produced by the pipeline during the geometric transformation. A blemish is seen above and to the right of center.
Images that have been geometrically corrected often show the pattern evident in the above grayscale picture: a thumbprint pattern at low intensity levels. It is quite hard to see, appearing most clearly when the image has a low (~1 count per pixel or so) spatially flat background. The thumbprint pattern is a modulation of the local noise characteristics of the data, not of the intensities themselves. It is a by-product of the geometric correction process in which the raw (geometrically distorted) image is resampled with an interpolator that takes a weighted mean of the four nearest pixels to determine the geometrically corrected pixel value (see "Geometric Correction (GEOCORR)" on page 6-5 for details). The weightings vary smoothly with position in the image, such that at some places, a single pixel dominates the weightings (the noise of the resampled pixel is the same as that of the original data), while at other places the weightings favor all four pixels equally (the average noise is half of the noise of the individual pixels). The fringes are contours of constant weighting.
The actual pattern depends on the particular geometric correction file used, and thus depends on the format. The effect on the scientific utility of the data is minimal, unless one requires accurate values of the noise per pixel for each pixel.
Figure 4.6: Full-Format f/96 Image of a Bright Extended Source
The portion of a full-format f/96 image shown above illustrates 8-bit wrapover and saturation. The former occurs when the image format selected is 512 x 1024 (zoomed or unzoomed). In that case, the image memory is configured so that there are only 8 bits per pixel. The maximum pixel intensity in raw full-format data is therefore only 255 counts; a further detected photon in a pixel causes the recorded intensity to cycle back to zero. After dezooming a full-format image, the maximum pixel intensity in the raw data is 255/2 = 127.5. The two pixels indicated have suffered from wrapover-they appear as rectangular because the raw dezoomed image is displayed. The dark region is an area where the photon count rate is higher than the FOC can count without suffering coincidence losses.
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Last updated: 11/13/97 16:36:34