ATIK Cameras ACIS Series Manual - Halaman 6
Jelajahi secara online atau unduh pdf Manual untuk Kamera Digital ATIK Cameras ACIS Series. ATIK Cameras ACIS Series 11 halaman. Advanced cmos imaging systems
Dark Frames
To get the most out of your Atik ACIS camera for astrophotography, we
recommend processing your images using dark frames. You can take dark
frames by covering the front of the camera with a lens cap. Dark frames should
be taken at the same temperature, exposure length and with the same gain and
offset settings as your light frames.
A master dark should be generated by averaging a large number of individual
dark frames. This can then be subtracted from the individual image sub frames
during processing. Further information on using dark frames should be available
in the manual of whichever image processing software you choose to use. Dark
frames are not required for High Speed Imaging.
Binning
Binning is a technique where groups of pixels are added together, with the
result being a brighter image. The CMOS sensor in the Atik ACIS only supports
binning in software. This is where the pixel values are added together after
image acquisition, as opposed to hardware binning where pixels are combined
on the sensor.
Gain and Offset
Your Atik ACIS allows you to change the gain and offset settings for the camera.
In very simple terms, this is analogous to the volume control on a radio. The
greater the gain, the easier it is to detect faint signals; however, less detail
might be seen in the brighter ones.
The full well depth (i.e. maximum signal) of the Atik ACIS is around 20,000e-,
which we map to a pixel value of 65,535. By increasing the gain, we reduce the
full well depth, which has the effect of making the images appear brighter. Using
a gain of x2, the full well depth is around 10,000e-. This 10,000e- now gives a
pixel value of 65,535, which makes the image appear twice as bright. The read
noise, or how 'grainy' the background looks, will also increase. However, this
increases a little less than two times.
The useful range for gain is up to x30. Here, the image is 30 times as bright, but
the full well depth is only ~650e-. This means bright objects will saturate very
quickly. Although it may look bad due to the small full well depth, the read noise
will only be about 1/3 of what it was at x1 gain. These kinds of settings are very
useful for very dim objects if you don't mind the bright objects saturating.
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