Starlight Xpress SXVR-H18 Скачать руководство пользователя страница 21

Handbook for the SXVR-H18

Issue 1 March 2010

21

2) Press the ‘Start’ button and a series of 1 second exposure guider images will

begin to appear in the picture frame. If the images look too dim, use the
‘Stretch Image’ slider to increase its contrast and brightness until the noise
begins to be visible.

3) If you haven’t focused the guider lens or ‘scope, move the mount until a bright

star is visible on the guider image and then adjust the focus until it is as sharp
as possible.

4) At this point, you may want to test the guiding control by pressing the manual

‘Move Telescope’ buttons at the bottom left corner of the control panel. You
can watch the position of any stars in the guider image and confirm that they
move in response to the buttons. The movement should be slow if the correct
guiding rate is selected on your mount (typically 2x sidereal). Adjust this, if
necessary.

5) Move the mount until the required object for imaging is properly framed in the

main CCD image (leave the guider menu and use the main camera control
panel, as necessary).

6) Re-open the guider control panel, start imaging and try to locate a clearly

visible guide star. If necessary, make adjustments to the guide telescope or off-
axis guider until one is found.

7) Press ‘Stop’ and then press ‘Select Guide Star’. Use the mouse to left click on

the selected star and a green cross will highlight it and the co-ordinates will
appear in the text boxes above the image window.

8) The various guiding rate defaults, listed on the right-hand side of the control

panel, are unlikely to be perfect for your particular telescope 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 software to complete a sequence of automatic moves and
calculations. The training will also determine the angle at which the guide
camera is oriented with respect to the RA and Dec axes. If you do not wish to
train the system at this time, the default values of 6 pixels per second will
serve as a starting point.

9) Now press ‘Go to main camera’ and the guider control panel will be replaced

by the camera control panel. Set the required exposure time for the image (say
5 minutes) and press the ‘Autoguide next image’ button. The autoguider
window will reappear and, after a few seconds, you should see error values
appearing in the text windows at the top. The guide star will be fairly close to
the green cross, although not necessarily accurately centred, and you should
see the power/ guide LED on the rear of the camera brighten and change
colour with each correction.

10) If the star begins to drift away from the cross, despite the corrections being

made, the chances are that the N/S and/or E/W directions are set wrongly.
Judge which axis is incorrectly set by observing the direction of the drift and
then stop the exposure by pressing ‘Esc’. Open the guider control panel and
check the appropriate swap box(es). After this operation, you will probably
need to find the guide star again by taking a guider image and reselecting the
star, as before. Now return to the main camera menu and try the ‘Autoguide
next image’ button again.

11) Once guiding is taking place without problems, the main exposure can be

allowed to finish and, if all is well, you should see an image with tiny circular
stars.

Содержание SXVR-H18

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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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