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Handbook for the TRIUS PRO 694      Issue 19th April 2019 

 

 

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Starlight Vision has a focus routine that will repeatedly download and display a 128 x 

128 pixel segment of the image at relatively high speed. This focus window may be 

positioned anywhere in the camera field. To use this mode, start up the software 

and select the Exposure mode. Set the camera mode to Binned 1x1 and select an 

exposure time of 1 second. Press ‘Start Exposure’ and wait for the image to 

download. There is a good chance that a suitable star will appear somewhere within 

the image frame. Now go to the ‘Focus’ tab and press ‘Get focus object’ - you can 

now click on a suitable star in your main image and its co-ordinates will be shown. 

Now click ‘Run focus exposure’ and you will see a steady stream of star images in the 

focus window. adjust the focusing of your telescope to get the sharpest definition. 

Once you are happy with the focus quality achieved, you might like to trim the 

settings of your par-focal or flip mirror eyepiece to match the current camera 

position. 

 

Although you can reach a good focus by the above method, many observers prefer 
to use additional aids, such as Hartmann or Bahnitov masks (an objective cover with 

several spaced holes) or diffraction bars (narrow parallel rods across the telescope 

aperture). These make the point of precise focus easier to determine by creating 

‘double images’ or bright diffraction spikes around stars, which merge at the setting 

of exact focus.  

 

Taking your first astronomical image: 

 

I will assume that you are now set up with a focused camera attached to a telescope 

with an operating sidereal drive. If so, you are now in a position to take a moderately 

long exposure of some interesting deep-sky astronomical object (I will deal with 

planets later). As many sidereal drives are not very accurate beyond a minute or two 

of exposure time, I suggest that you find a fairly bright object to image, such as M42, 

M13, M27 or M57. There are many others to choose from, but these are good 

examples. 

 

Use the finder to align on your chosen object and then centre it accurately. Once 

properly centred and focused, take an exposure of about 60 seconds, and observe 

the result. Initially, the image may appear rather barren and show only a few stars, 

however, a great deal of data is hidden from view. You can get to see a lot of this, 

without affecting the image data, if you go to the Histogram window and adjust the 

two sliders to frame the main peak in the image data. The faint image details will 

then appear in good contrast and I think that you will be impressed by the result! 

 

If you are happy with the image, go to the ‘File’ menu and save it as a FITS file in a 

convenient directory.  

 

 

 

 

 

Summary of Contents for TRIUS PRO 694

Page 1: ...b with 3 external ports and a dry argon CCD chamber fill The USB hub permits several other devices to share the single USB connection and greatly reduces the number of cables required in a typical set...

Page 2: ...p sky imaging especially with an H alpha filter The H alpha QE is about 65 considerably better than many other interline chips The full frame download time is only around 2 5 seconds and a binned 4x4...

Page 3: ...024 x 768 pixels and 24 bit colour A medium specification i7 machine is ideal but most modern computers are OK Please note that USB 2 0 operates at a very high speed and cannot operate over very long...

Page 4: ...4 Now connect the USB cable to the socket on the camera rear panel Windows will report Found new hardware and will automatically find the drivers You can check this by opening Device Manager and looki...

Page 5: ...t the top right hand side of the panel I recommend using the set point to about 10C for general imaging but you can go much colder especially if you are imaging during the winter months Under indoor c...

Page 6: ...is introduces additional complications which are best avoided at this early stage There are two simple options one of which is available to everyone with a sheet of aluminium baking foil 1 Attach a st...

Page 7: ...ise focus problems and keep the light level reasonable for daytime testing The pin hole needs no such adjustments and will work immediately although somewhat fuzzily Point the camera lens or pinhole t...

Page 8: ...age to darken 3 If the USB did not initialise properly the camera start up screen will tell you that the connection is defective Try switching off the power supply and unplugging the USB cable Now tur...

Page 9: ...ld stop is located at the same distance from the barrel end as the CCD is from the camera barrel end approximately 16mm When the par focal eyepiece is fitted into the telescope drawtube you can adjust...

Page 10: ...fect and so any F ratio from about F4 5 to F6 3 will give good results It is clear from this result that the Starizona Hyperstar adaptor is very well suited to use with the 694 as it operates at aroun...

Page 11: ...arrow parallel rods across the telescope aperture These make the point of precise focus easier to determine by creating double images or bright diffraction spikes around stars which merge at the setti...

Page 12: ...gth as that of the light frame This image will be a picture of the dark signal generated during your exposure and it should be saved with your image for use in processing the picture If many such dark...

Page 13: ...the colour data will be destroyed 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 wid...

Page 14: ...hat you uncheck Autosave when finished or you will save every image that you take The exposure time needed for good planetary images is such that the image histogram has a peak value at around 40 000...

Page 15: ...lens If you 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 ima...

Page 16: ...e original artefacts and you can then process it in the normal way The TRIUS PRO guider port The TRIUS PRO is provided with a guide port for use with ST4 compatible mounts The Autoguider output port i...

Page 17: ...no great difficulty in removing such particles on the outside surface by the careful use of a lens cleaning cloth lens pen or air duster and so you should have little trouble with this aspect of maint...

Page 18: ...ive action DO NOT rub vigorously and be very careful to avoid scratching the window Finish off by giving the CCD a short blast from an air cannon 6 Before re assembly make certain that the inside surf...

Page 19: ...leave the camera cooling switched on for long periods between uses The cold CCD will collect ice by slow diffusion through any small leaks and this will become corrosive water on the cooler and CCD p...

Page 20: ...e imager CCD size Active area 12 5mm x 10mm CCD pixels 2750 x 2200 pixel array Each pixel is 4 54 x 4 54uM square Well depth Full res mode 17 000e Binned 2x2 mode approx 22 000e Mean visual QE 70 77 a...

Page 21: ...GUARANTEE 1 The equipment shall only 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...

Page 22: ...Handbook for the TRIUS PRO 694 Issue 19th April 2019 22...

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