
QSI 500 SERIES USER GUIDE
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Single-shot color CCDs, like those found in almost all general use digital cameras, are
made by placing red, green and blue filters over adjacent pixels in the CCD. The image
processing program then has to separate the three different color images and recombine
25% are covered in a red filter. This
ed because the
set of
you
Signal versus noise
For an astronomer, “signal” is the photons coming an
ideal world, there would be steady stream of phot
photon striking a pixel would be converted into ex
number of electrons would be precisely counted a
photographer exactly how much light struck each
converting light to pixel values in a CCD image is ical
laws and other factors that introduce “noise” into a
pixel values that make the image a less than exac
Noise in CCD images can manifest itself in multipl
background areas, “hot” pixels, faint horizontal or
signal areas of the image, blotchy gradients between darker and lighter regions in a nebula,
a gradient from dark to light from one corner or sid of an image to the other, and especially
as low contrast images — the result of a reduced signal to noise ratio. Achieving high
s from a cooled CCD camera requires a basic
them into a
single color image.
Single-shot color CCDs use a “Bayer
filter” with alternating red, green and blue
pixels covering adjacent pixels in a
checker board pattern as shown in the
image to the right.
50% of the pixels are covered in a green
filter, 25% are covered in a blue filter and
arrangement is us
human eye is most sensitive to green
light. The green pixels correspond to
luminance and record the greatest detail
while the red and blue filters record
chrominance.
After the raw image is read from the
CCD, a demosaicing algorithm must be applied to the image to produce a complete
red, green and blue images by interpolating the missing pixel values. This is exactly what
normal digital cameras do, but it’s all hidden inside the camera’s electronics. You only see
the final processed image. With a CCD camera, the raw image is read into the camera
control program and then processed on your computer. This has the advantage that
can directly manipulate the raw image to, for instance, vary the color balance.
Single-shot color models offer the easiest way to take color images of the night sky. The
trade off is reduced QE and detail because of the demosaicing and pixel interpolation.
from the stars in the night sky. In
ons from every bright object and every
actly one electron in the CCD. Then the
nd converted to a number telling the
pixel. Unfortunately, the process of
governed by some fundamental phys
n image. Noise is unwanted variations in
t representation of the original scene.
e ways, including “graininess” in darker
vertical lines that become visible in low
e
dynamic range, low noise image
understanding of how CCDs work and the different sources of noise that can reduce the
quality of your images.
Courtesy Wikipedia
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