Polaroid CCD Camera User Manual

Page 50

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Section 8 - Glossary

Page 46

Flat Field

- A Flat Field is a image with a uniform distribution of light entering the telescope.

An image taken this way is called a flat field image and is used with CCDOPS to correct

images for vignetting.

Focal Reducer

- A Focal Reducer reduces the effective focal length of an optical system. It

consists of a lens mounted in a cell and is usually placed in front of an eyepiece or

camera. With the relatively small size of CCDs compared to film, focal reducers are

often used in CCD imaging.

Frame Transfer CCDs

- Frame Transfer CCDs are CCDs that have a metal mask over some

portion (usually half) of the pixel array. The unmasked portion is used to collect the

image. After the exposure is complete, the CCD can very quickly shift the image from

the unmasked portion of the CCD to the masked portion, thus protecting the image

from light which may still be impinging on the CCD. This acts as an electronic shutter.

Full Well Capacity

- Full Well Capacity refers to the maximum number of electrons a CCD

pixel can hold. This number is usually directly proportional to the area of the pixel.

Histogram

- The Histogram is a table of the number of pixels having a given intensity for each

of the possible pixel locations of the image file. Remember that, in the end, the image

file is nothing more than a list of pixel values, one for each CCD pixel. These value

numbers can be displayed in two formats; as a table or plotted as a graph.

Light Frame

- The Light Frame is the image of an object before a Dark Frame has been

subtracted.

Path/Filter

- For PC users the Path setting tells CCDOPS which directory and disk drive to find

and store the image files. In essence, it defines the current directory. The filter controls

which image files are shown in the Open directory. Only files that match the filter are

shown. For example, a filter setting of "*.ST6" will only show files that have an "ST6"

extension.

Photometry

- Photometry is the study of stellar magnitudes at a given wavelength or

bandpass.

Pixel Size

- The smallest resolution element of a CCD camera is the CCD pixel. The pixel sizes

for each of the SBIG cameras are as follows:

Camera

Pixel Size (microns)

Tracking CCD13.75 x 16

ST-5C

10 x 10

ST-237/237A 7.4 x 7.4

STV

14.8 x 14.8

ST-6

23 x 27

7

ST-7E/ST-8E 9 x 9

ST-9E

20 x 20

ST-10E

6.8 x 6.8

ST-1001E

24 x 24

7

The TC241 CCD used in the ST-6 actually has 11.5 x 27 micron pixels. The CPU combines two 11.5

micron pixels to make the 23 micron pixel . This gives pixel with a more square aspect ratio.

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