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SBIG ST-402 Operating Manual 

 

 Page 16 

 

Dark Frames

 – For most objects you won’t need to take dark frames in 

Focus mode to frame and focus the object because the exposures 
tend to be short and the build up of dark current minimal.  On 
some dim objects though, checking this item, which uses 

dark 

subtracted

 images for 

Focus

 mode can help to pull the object out 

of the noise.  It’s slightly slower when using dark frames so only 
use this when you need to. 

Update Mode

 – Sometimes you want to tweak the focus, look at an image, 

tweak it again, etc.  Setting this to 

Manual

 causes the Focus mode 

to pause between images until the 

Space Bar

 is hit or you click the 

Pause/Resume

 button. 

Peak

 – This shows the position and brightness of the brightest pixel in the 

Focus mode image.  We’ll use this later to get the best focus by 
maximizing the 

Peak

 on a 

star

Pause/Resume

 – Click this button at any time to pause or resume the focus 

mode.  This can be handy for going back and forth between the 
telescope and the computer or for studying the images. 

 
You can read more about the other items in the 

Help

 but we now know 

enough for basic operation.  Exit 

Focus Mode

 by closing the 

Focus Mode

 

dialog or closing the image window. 
 

You’ve come a long way in this brief tutorial.  If you want to spend 

some time reading the 

Help

 file or the 

CCDOPs Manual

, which is included 

on the CD-ROM that would be useful.  Otherwise it’s time for trying it out 
at the telescope. 

SBIG ST-402 Operating Manual 

 

 Page 17 

 

4.

 

At the Telescope 

Connect the camera to the computer and start 

CCDOps

.  Establish a link to 

the camera and run the 

Camera Setup

 command.  Enable the cooling to 20 

degrees below ambient and then watch the 

Link Status

 field to see the 

temperature come down.  Once the temperature reaches the Setpoint it will 
jump back and forth by about 0.5 degrees.  This is normal.  The ST-402 
regulates the CCD temperature by dithering back and forth across the 
Setpoint.  At this point we’re ready to hook up to the telescope. 
 

Focusing a CCD camera at the telescope can be a tedious operation, so 

a few hints should be followed.  Before using the software to focus the 
camera the first time you should place a diffuser (such as scotch tape or 
ground glass) at the approximate location of the CCD's sensitive surface 
behind the eyepiece tube and focus the telescope on the moon, a bright 
planet or a distant street lamp.  This preliminary step will save you much 
time in initially finding focus.  The approximate distance behind the 
eyepiece tube for the ST-402 

is

 0.690 inches

 (

backfocus

). 

 

To achieve fine focus, first center a bright star then insert the CCD head 
into the eyepiece tube, taking care to seat it, and then enter the CCDOps 

Focus Mode

. Do not initially try to focus on the moon or planet – they are 

harder.  As we learned in the tutorial, the 

Focus Mode

 automatically 

displays successive images on the screen as well as the peak brightness 
value of the brightest object in the field of view.  Using the telescope 
controls, center the star image in the CCD, and adjust the focus until the star 
image is a small as can be discerned.  Next, shift the telescope to fainter 
stars so the CCD is not saturated.  Further adjust the focus to maximize the 
displayed star brightness in counts and minimize the star diameter.  This can 
be tedious.  It helps considerably if a pointer or marker is affixed to the 
focus knob so you can rapidly return to the best focus once you've gone 
through it. 
 

An exposure of 1 to 3 seconds is recommended to smooth out some of 

the atmospheric effects.  While you can use the 

Full frame

 mode to focus, 

the frame rate or screen update rate can be increased significantly by using 

Planet mode

.  In Planet mode the Focus command takes a full image and 

Содержание ST-402ME

Страница 1: ...ion which can be determined by turning the equipment off and on the user is encouraged to try to correct the interference by one or more of the following measures Reorient or relocate the receiving antenna Increase the separation between the receiver and the equipment Connect the equipment into an outlet on a circuit different from that to which the receiver is connected Consult the dealer or an e...

Страница 2: ...ith internal shutter allowing exposures down to 40 milliseconds that makes taking dark frames a trivial task USB 2 interface yielding up to 1 2 megapixels per second download rates but full backward compatibility with USB 1 1 computers at 400 kilopixels per second Input power requirements of 10 0 14 5 Volts DC at 1 Amp through the new center positive locking power jack Telescope interface with fou...

Страница 3: ...e first time you MUST install the software as described below SBIG ST 402 Operating Manual Page 3 2 Installing the Software Installing USB drivers on a Windows system can be a difficult task if you don t follow the instructions to the letter Please don t plug the camera into the computer until instructed to do so below and please follow the instructions carefully 1 Disable Driver Signing Windows X...

Страница 4: ... copying the SBIG ST 402 Loader driver then show you the Completing the Found New Hardware Wizard page Click Finish At this point the Red LED on the back of the camera should be on and if you had been watching it you would have seen it blink several times while the PC was booting the camera SBIG ST 402 Operating Manual Page 5 11 After booting the camera Windows will bring up another copy of the Wi...

Страница 5: ...he Exposure Time was 1 0 second Spend some time inspecting the data then click in the dialog to close it Data like this is always attached to saved images and you can show it using the Parameters command in the Display menu After the Image Parameters dialog has gone you ll see the image displayed in its own window and the Contrast dialog will appear The image is shown below SBIG ST 402 Operating M...

Страница 6: ...open light frame and another of equal exposure with the shutter closed dark frame You then subtract the dark frame from the light frame and because the hot pixels and the readout glow repeat from one image to another they are removed by the subtraction Let s see how this works Close Image 2 and Open Image 3 which is a 10 second light frame where you can get a hint of the object but the hot SBIG ST...

Страница 7: ...mages Clicking Smooth can reduce the noise in underexposed images Clicking Sharpen reveals additional detail in well exposed images Establishing a Link It s time to actually connect up to your camera and take some images If you haven t installed the drivers already go back to Section 2 and do so now If you ve taken a break from the tutorial and the camera isn t powered up and attached to the compu...

Страница 8: ... the TE cooler We recommend choosing a temperature that is 20 to 23 degrees below the ambient temperature Choosing a lower temperature won t hurt the camera but you ll notice in the Link Status field bottom of screen that the CCD never attains the temperature and the TE stays at 100 It can take several minutes for the temperature to settle in but if you see the TE stuck at 100 simply increase the ...

Страница 9: ...our telescope would drive you crazy taking a single image at a time tweaking the telescope etc Instead we use the Focus command which is like Grab but it takes image after image SBIG ST 402 Operating Manual Page 15 automatically Use the Focus command in the Camera menu and set it up in the Focus Setup dialog as shown below Click OK and the camera will go into Focus mode You ll see image after imag...

Страница 10: ...e Setpoint it will jump back and forth by about 0 5 degrees This is normal The ST 402 regulates the CCD temperature by dithering back and forth across the Setpoint At this point we re ready to hook up to the telescope Focusing a CCD camera at the telescope can be a tedious operation so a few hints should be followed Before using the software to focus the camera the first time you should place a di...

Страница 11: ...rate If you have difficulty finding an object after obtaining good focus check to be sure that the head is seated at best focus then remove the head and insert a medium or low power eyepiece Being careful not to adjust the focus knob on the telescope slide the eyepiece in or out until the image appears in good focus Then visually find and center the object if it is visible to the eye If not use yo...

Страница 12: ...ooming Kodak CCDs like the KAF 0402LE with the antiblooming option can be used to help stop or at least reduce blooming when the brighter parts of the image saturate Astrometry Astrometry is the study of stellar positions with respect to a given coordinate system Autoguider All SBIG CCD cameras have auto guiding or Star Tracker functions This is accomplished by using the telescope drive motors to ...

Страница 13: ...ut Noise Readout noise is associated with errors generated by the actual interrogation and readout of each of the CCD pixels at the end of an exposure This is the result of fixed pattern noise in the CCD residual charge in the readout capacitors and to a small extent the noise from the A D converter and preamplifier Resolution Mode The resolution of a CCD camera is determined by pixel size Pixel s...

Страница 14: ...les Power Jack The Power Jack is used to supply 10 0 14 5 Volts DC at 1 amp to the camera The jack is locking and center positive The mating plug is the locking model Switchcraft S760K with 0 218 inch outer diameter and 0 080 inch inner diameter 5 5 2 0 mm Telescope Jack The Telescope Jack is used to provide tracking signals to the telescope Viewed from outside the camera looking in it has the fol...

Страница 15: ...with a cotton swab or Q tip and a little isopropyl alcohol Use one end of the Q tip to swab it with alcohol and the other to dry it Never re use a Q tip and do not scrub use gentle pressure 7 Replace the front lid 8 If you have a few small dust specs don t worry it is almost impossible to get them all and a flat field will take care of them well 9 Filters are cleaned the same way Replacing the Des...

Страница 16: ... Size 9 x 9 microns Full Well Capacity Non ABG CCDs ABG CCDs 100 000 electrons 50 000 electrons Dark Current 1 e pixel sec at 0 C Shutter Electromechanical Exposure 0 04 to 3600 seconds 10ms resolution A D Converter 16 bit with Correlated Double Sampling Read Noise 17e RMS Binning Modes 1x1 2x2 3x3 Full Frame Download USB 2 USB 1 1 Up to 1 200 000 pixels per second Up to 400 000 pixels per second ...

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