Starlight Xpress SXVR-H18 User Manual Download Page 22

Handbook for the SXVR-H18

Issue 1 March 2010

22

If the stars are not circular, you may need to alter the guiding parameters, or
investigate the rigidity and drive performance of your mount. A lot of information
can be deduced by watching the behaviour of the guide star in the guider frame. If
it is continually moving between two locations, either side of the green cross, then
the RA or Dec pixels per second value is set too low. The higher these values are
set, the gentler the guiding becomes. Too low a value will cause an over-
aggressive correction to be made and result in oscillation of the star position
between two points.

Another source of guiding errors can be a too accurately balanced telescope
mount! Good balance can result in the telescope mount ‘bouncing’ between the
gear teeth as corrections are made. A simple fix is to add a weight of about 0.5kg
(1 pound) on the eastern end of the declination axis, so that there is always some
pressure acting against the gear teeth.

Getting a good result from an autoguider will often entail a lot of detective work
to eliminate the sources of gear error, telescope flexure, mirror shift etc., but the
final result is well worth the effort!

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Camera maintenance:

Very little maintenance is needed to keep the SXVR-H18 in excellent operating order,
however two problems, which are common to all CCD equipment, are likely to show
up on occasion. These are dust and condensation.

Removing Dust:

1) Dust can be deposited on either the optical window (not a big problem to cure), or
on the CCD faceplate (difficult to eliminate entirely). When small particles collect on
the window they may not be noticed at all on deep sky (small F ratio) images, as they
will be very much out of focus. However, if a powerful contrast boost of the image is
carried out, they may well begin to show as the shadow ‘Do-nuts’ mentioned earlier.
Images taken with a large F ratio optical system are more likely to be affected by such
dirt, owing to the smaller and sharper shadows that they cast. There is no great
difficulty in removing such particles on the outside surface by the careful use of a lens
cleaning cloth or ‘air duster’ and so you should have little trouble with this aspect of
maintenance. Dust on the CCD faceplate is a much greater nuisance, as it casts very
sharply defined and dark shadows and it entails dismantling the camera to get rid of
it! To clean the CCD you will need a good quality lens cloth (no silicone) or tissues
and some high-grade isopropyl alcohol. A very suitable cloth is the ‘Micro-Fibre’
type marketed by PENTAX etc., and suitable alcohol is available from TANDY
(Radio Shack) etc. as tape head cleaning fluid. A bright light and a strong
watchmakers eyeglass will also be found essential.

Procedure:

1) Disconnect the lead from the camera head and remove it from the telescope. Place
it on a table with the optical window facing downward.

2) Remove the two M3 screws and the M8 nut from the camera back plate and ease
the plate out of the camera body. Unplug the fan lead from the camera PCB.

Summary of Contents for SXVR-H18

Page 1: ...CCD surface gives the greatest possible throughput of light to the pixels and the resulting QE is very good over the entire visible spectrum Our new R type USB2 interface hardware gives an exceptional...

Page 2: ...intend to view the finished images on its screen then you will also need a graphics card capable of displaying an image in a minimum of 1600 x 1200 pixels and 32 bit colour A medium specification 2 co...

Page 3: ...IOClass device and the camera software will be able to access it You can confirm that the installation is complete by checking the status of the USB devices in the Windows Device Manager see above Sta...

Page 4: ...the icon when you should see the main menu and image panel appear If this is the first time that it has been run you will receive a warning about the lack of an ini file just click on OK and then ope...

Page 5: ...you are imaging during the winter months Under indoor conditions the low airflow will limit the cooling capability and you should use a set point of no lower than 5C for stable cooling You can determi...

Page 6: ...aptor to achieve approximately the correct focal distance 2 Create a Pin hole lens by sticking a sheet of aluminium baking foil over the end of the lens adaptor and pricking its centre with a small pi...

Page 7: ...Also IR blocking filters are available from various suppliers True Technology Edmunds etc and are recommended for the best results when using a lens If you cannot record any kind of image please chec...

Page 8: ...brighten or dull the image highlights and shadows A Normal stretch is a simple linear operation where two pointers the black and white limits can be set at either side of the image histogram and used...

Page 9: ...nd select an exposure time of 1 second Press Take Picture and wait for the image to download There is a good chance that your selected star will appear somewhere within the image frame and with luck i...

Page 10: ...a few stars however there is a great deal of data hidden from view You can get to see a lot of this without affecting the image data if you go to the View menu and select Auto Contrast Stretch Image T...

Page 11: ...rocess in detail at a later stage Processing the deep sky image Below you will see typical examples of a dark frame and an uncalibrated raw image of M16 A typical 5 minute dark frame exposure Note the...

Page 12: ...curately match your darks to the light image If you average many dark frames together to create a master dark the readout noise will be much reduced by the square root of the number of averaged darks...

Page 13: ...are at the time of writing but Maxim DL can use this method The basic procedure is to capture a long exposure dark frame and then slice off all values below a threshold level which is selected so as t...

Page 14: ...to noise ratio Summing can be done in the Merge menu and involves loading the first finished image selecting a reference point a star then loading the second image and finding the same star with the...

Page 15: ...much better for this However lunar imaging is a different matter and the H18 can give impressive whole moon pictures Most deep sky objects are faint and relatively large so a long exposure is needed...

Page 16: ...conditions If you have exceptionally good conditions then a reduction to R 3 P 3 will probably give a more natural look to the image as too large a radius and power tends to outline edges with dark o...

Page 17: ...really do need to use a flat field for image correction then it must be taken with care It is most important that the optical system MUST NOT be disturbed between taking your original images and takin...

Page 18: ...des 4 active low opto isolator outputs and a common return line capable of sinking a minimum of 5mA per output This socket may be used for telescope control if the SXVR H18 is employed as an autoguide...

Page 19: ...declination axis of your mount This is not absolutely essential as the training routine will learn the angle of the head and compensate for it but it is easier to understand the motion of the guide st...

Page 20: ...on a 80mm refractor guide scope in the author s garden To use the autoguider please proceed as follows 1 Having started the SXVR H18 software open the autoguider control panel by clicking on the autog...

Page 21: ...scope and mount You have the option of manually selecting values or asking the software to attempt to determine what they should be This is done by pressing the Train button and waiting for the softwa...

Page 22: ...sation Removing Dust 1 Dust can be deposited on either the optical window not a big problem to cure or on the CCD faceplate difficult to eliminate entirely When small particles collect on the window t...

Page 23: ...disturbed renew it with fresh compound before reassembling 7 Replace all the camera parts in reverse order and the job is done Dealing with condensation The SXVR H18 is designed to avoid condensation...

Page 24: ...the CCD surface To make an adjustment slacken the appropriate set screw and then turn the adjacent cap head screw in the required direction Complete the adjustment by re tightening the set screw Avoi...

Page 25: ...ly be used for normal purposes described in the standard operating instructions and within the relevant safety standards of the country where the equipment is used 2 Repairs under guarantee will be fr...

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