Starlight Xpress SXVR-M25C - Manual (Page 18)

Handbook for the SXVR-M25C Issue 1 June 2009
18
at a rate proportional to the square root of the number of summations (summing 4
images will double the signal-to-noise), but different exposures must be used.
Summing an image with itself will not improve the S/N ratio!
Although I have concentrated on the use of a telescope for deep-sky imaging, do not
forget that you have the option of using an ordinary camera lens for impressive wide-
field shots! A good quality 200mm F3.5 lens with an infrared blocking filter will yield
very nice images of large objects, such as M31, M42, M45 etc. If you cannot obtain a
large IR blocker for the front of the lens, it is quite acceptable to place a small one
behind the lens, inside the adaptor tube. You can even try using a hydrogen-alpha
filter to bring out nebulae, reduce light pollution and sharpen the star images to pin-
points, although the results will be monochrome red!
Taking pictures of the planets:
The SXVR-M25C has a large CCD with 6 million pixels and so it is not well suited to
planetary imaging, where a small CCD is ideal. However, it can be used if you accept
the relatively large amount of wasted image area, or use a sub-frame download.
Planetary imaging is in many ways quite different from deep sky imaging. Most deep
sky objects are faint and relatively large, so a short focal length and a long exposure
are needed, while planets are bright and very small, needing long focal lengths and
short exposures. High resolution is critical to achieving good results and I have
already shown how a suitable focal length can be calculated and produced, using a
Barlow lens.
Many camera users comment on the difficulty of finding the correct focus when
taking pictures of Jupiter etc. This is usually due to poor seeing conditions, which are
only too common, but may also be due in part to poor collimation of your telescope.
Please ensure that the optics are properly aligned as shown by star testing, or by using
one of the patent collimation aids that are widely available. It is also better to use a
star for initial focusing, as planetary detail is difficult to judge in bad seeing. Although
the star will also suffer from blurring, the eye can more easily gauge when the most
compact blur has been achieved!
You could begin by imaging lunar craters, or the planets, Jupiter, Saturn or Mars. The
rapid variations of seeing which accompany planetary imaging, will ruin the
definition of about 95% of your images and so I recommend setting the camera to run
in ‘Autosave’ mode. This will automatically take a sequence of images and save them
with sequential file names in your ‘Autosave’ directory. Dozens of images will be
saved, but only one or two will be satisfactory for further processing. The ‘Subframe’
mode of the SXVR may be found useful for limiting the wasted area and reducing the
download time of small planetary images.
To start the Autosave process, call up the SXVR Camera Interface and select the
‘Continuous Mode’ check box at the top (make sure the rest are unchecked). Now
check the ‘Autosave Image’ checkbox near the bottom of the window. If you now
click on ‘Take Picture’ the automatic sequence will begin and will not stop until you
press a computer key. The images will be saved in FITs format with sequential names