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Some General Rules for
Successful Imaging
Advanced CCD cameras caused a revolution in amateur astronomy. Amateurs
started to capture images of deep-sky objects similar or surpassing the ones
captured on film by multi-meter telescopes on professional observatories.
While the CCD technology allows capturing of beautiful images, doing so is
definitely not easy and straightforward as it may seems. It is necessary to gain
experience, to learn imaging and image processing techniques, to spend many
nights mastering the technology.
Although CCD camera can convert majority of incoming light into information,
it is not a miracle device. Keep on mind that laws of physics are sill valid.
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CCD camera does nothing more than converting image created on the
chip by telescope (or objective lens) into information. A quality
telescope and quality “photographic-class” mount is absolute must for
successful imaging. If the mount cannot keep the telescope on track or
the telescope cannot create perfectly focused image, result is always
distorted and blurred.
●
Ideally the exposures should be automatically guided using guiding
CCD camera or at last webcam or similar device. Tracking errors
caused by drive periodic error, mount polar misalignment or other
mechanical issues (often unnoticeable by eyes) cause streaking of star
images. Note the exposure time for each color often reaches tens of
minutes or even hours if the really high quality images are taken.
The G1 series of CCD cameras are especially designed with guiding
on mind. G1 CCD cameras are equipped with “autoguider” connector,
which allows direct connection between the G1 camera head and
telescope mount. 16-bit digitization and using of sensitive Sony ICX
CCD detectors provide higher sensitivity and dynamic range
compared to typical video or web cameras. The SIPS software
package supports both imaging and guiding cameras and implements
sophisticated guiding algorithms.
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Focus image properly. Almost unnoticeable focuser shift affects star
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