APC AP9212 User's Guide Page 103

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103
The APT has the following filters available:
Ultraviolet (R)
Blue (B)
Visible (V)
Visible Red (VR)
Infrared (I)
Clear
E.5. Flat fielding
Flat Fielding refers to the process of calibrating the CCD to account for irregularities in the optics
and errors within the CCD itself. A reference image is taken when the CCD is expected to return
an image of constant intensity, such as the twilight sky. Any flaws in this reference image can be
used to correct images obtained in the future.
This is not to be confused with the focal plane within the Telescope, which has been flattened
using a field-flattening lens. Originally, images were obtained from the APT using photographic
film which was placed in a spherical shaped collection area within the telescope. Because the
CCD cannot be placed on a curved surface, the optics were modified with the addition of a
lens to make the telescope focal plane flat out to a diameter of 5 degrees.
E.6. Cosmic rays
Cosmic Rays or Cosmic Radiation, in simple terms, refers to energised particles travelling in all
directions throughout the universe. Very little is known of there origin. Optical astronomers are
concerned with cosmic rays as they can affect images obtained with the CCD. If a cosmic ray
strikes the CCD, the resulting image will falsely appear to show a bright star
To counteract this phenomenon, astronomers will typically take three images in succession, and
compare the results to identify any spurious data caused by cosmic rays.
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