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does not move, check the 

Settings. Remember, you have to set up a 

method for sending the autoguider commands to the telescope!

11. The star should move in an L shape. If it does not move enough, a warning 

message will appear. The recorded positions will be displayed in the scrolling 
log, along with any error messages.

Note: If the star does not move far enough, or moves too far (i.e. the star leaves the 
field), the duration of the calibration move commands can be adjusted by clicking 
the 

Settings command and changing the Calibration Time fields (measured in 

seconds). A longer calibration time will increase the motion of the star; a shorter 
time will decrease the motion. Typical values range from five to ten seconds, 
depending on the correction speed, focal length, and pixel size.
12. Once you have successfully calibrated, switch to the 

Track mode. Click 

Start, and watch the star. It should move to the center of the small track box, 
and whenever it drifts off it should be pulled back again. You can zoom in 
the window for a better look. Also the tracking errors will be displayed in the 
scrolling log.

13. If the star bounces back and forth, reduce the aggressiveness for that 

axis. If it corrects too slowly, increase the aggressiveness. Changes to the 
aggressiveness settings take effect immediately.

You are now ready to take a long-exposure image through the main telescope and 
imaging camera. The Parsec will continuously send small correction factors to the 
mount’s motor drive to insure steady and accurate tracking throughout the dura-
tion of the exposure, however long that may be.

Other Autoguiding notes:

•  If you are using a German equatorial mount you must calibrate with the 

tube on the same side of the mount as it will be when actually imaging.

•  The calibration settings need changing if you move the telescope in 

declination by more than about five degrees. Select another bright star, 
and Calibrate again.

•  If you experience bad guiding in declination and cannot resolve it through 

adjusting the calibration or aggressiveness, you may have a stiction 
problem with your declination drive. Watch which way the star drifts, 
and turn off the Guider Enable checkbox (in the Settings window) that 
pushes the star in that direction. That will prevent the stiction cycle from 
happening.

•  Make sure that any backlash compensation in the mount is turned off.

•  On most telescopes, the Right Ascension drive likes to have some load 

pushing against sidereal tracking. If the mount is balanced such that it is 
pulling the mount forwards slightly, the gear teeth may bounce back and 
forth resulting in terrible guiding that cannot be corrected by an autoguider. 
Be sure to always balance the telescope such that it “lifting the weight” 
rather than “allowing it to fall”; i.e. heavier on the East side. Note that this 
may require balancing the telescope differently when it is pointed East 
versus West.

7.  Other Features Of MaxIm Dl

This manual only covers a small fraction of all the capabilities and features of 
MaxIm DL. We strongly recommend reading through MaxIm DL’s 

Help Topics for 

more detailed information about all of the features once you have become more 
familiar with setting up and using your Parsec camera.

7.1. Information Window

The Information window displays numerical information about selected areas of 
the image. The window can be switched on and off using the 

Information Window 

command on the 

View menu, or by using the cursor button on the Toolbar. The 

window can remain open as a floating toolbox without interfering with other com-
mands.
The 

Information window has four modes of operation: ApertureRegion, Area, 

and

 Astrometric. There is also a Magnitude display that can be calibrated to show 

accurate stellar magnitudes. Except in 

Area mode, the mouse cursor will change to 

a crosshair and “bullseye” when the 

Information window is active and the mouse is 

over the selected image or preview. The sizes of the various elements of the circular 
cursor can be changed using the mouse with the 

right-click menu.

To lock the cursor at a specific position and freeze the information display, 
double-click on the image. When locked, the circular cursor can be moved using 
the 

arrow keys. You can then copy text from the status area of the Information 

window to the clipboard using the 

mouse and CTRL-C (or right-click the mouse 

in the status area and select 

Copy from the resulting context menu). To restore 

normal operation, 

click the mouse again on the image.

Numbers exceeding one million are shown in scientific notation; a lower case e 
followed by an integer means the preceding quantity must be multiplied by that 
power of ten.

7.2. night Vision

Selecting 

Night Vision toggles the night vision mode on and off. Three types of 

night vision display are available, selected by a dropdown on the 

General tab of 

the 

File Settings dialog:

Summary of Contents for PARSEC 10100C

Page 1: ...ec 10100C Color 52078 instruction Manual Providing Exceptional Consumer Optical Products Since 1975 OrionTelescopes com Customer Support 800 676 1343 E mail support telescope com Corporate Offices 831...

Page 2: ...eep Sky Objects 20 5 Image Processing 26 5 1 Image Calibration 26 5 2 Convert Raw to Color For Parsec 8300C and 10100 27 5 3 Stacking Combining Images 28 5 4 Filter 32 5 5 Color Balance 32 6 Multiple...

Page 3: ...ludes 1x1 full resolution 2x2 3x3 and 4x4 This CCD chip offers the unique ability to image in color at 1x1 mode as well as 2x2 mode This is advantageous when imaging with different focal lengths In ge...

Page 4: ...edge darkening may occur Caution Be sure to always firmly tighten the thumbscrew s that secure the Parsec in the telescope focuser or it could fall out and onto the ground If your telescope has T thr...

Page 5: ...plorer 4 or higher required to display on line help High speed USB 2 0 port Power The Parsec requires 12 volts DC 12VDC with approximately 2 amperes of cur rent Power to the entire camera including th...

Page 6: ...he following section of the manual will walk you through the basic features mostly found in the Camera Control Window The Parsec includes a free 60 day trial of MaxIm DL 5 Pro Start by opening MaxIm D...

Page 7: ...it a few seconds for the image to appear It may be over exposed or grossly out of focus Adjust the telescope s focus and adjust the exposure time as needed to get a focused image 4 Look at the Pixel v...

Page 8: ...image has a different histogram depending on how much of the image is bright or dark Directly viewing the histogram of your image in the Screen Stretch Window provides an easy interface for making de...

Page 9: ...se The camera will only download the area you previously selected which makes each image download significantly faster than the whole frame Note If the Parsec is grossly out of focus no object will ap...

Page 10: ...quality of your focus Caution Once you have achieved focus be sure to click the Reset but ton in the Subframe box otherwise the camera will crop all your images into a small square 4 2 Setting the Coo...

Page 11: ...eep sky object into the field of view of your eyepiece If you are using a mount with an accurate computerized go to system you can keep the camera installed in your telescope s focuser without using t...

Page 12: ...iminate most of the camera noise you can take several dark frames average them then subtract them from your astro images also called light images Note Make sure the cooler set point and CCD temperatur...

Page 13: ...flat frames it s a good idea to assign a preset such as F to better organize your different images 4 Set the Seconds to 0 1 for now and click OK then Expose You want the Max Pixel to read somewhere ar...

Page 14: ...s appear in the window 3 Select the Source Folder where you saved your dark frames Figure 23 4 Click Auto Generate and MaxIm DL will automatically find all of your calibration images such as darks and...

Page 15: ...ged into groups according to their FITS header You can open the groups to view the files by clicking on the sign If you would like to view an individual file right click it and select Display Image Al...

Page 16: ...e Add Folder option calibration files are automatically ignored the other methods for adding files will include them Usually you don t want to stack the calibration files automatically since the Set C...

Page 17: ...re a background level adjustment This is accomplished by bringing the background level or bias in each color plane down to zero Each of the Background Level values is subtracted from every image pixel...

Page 18: ...ting of 10 means that the Parsec attempts to track out 100 of the motion whereas a setting of 1 means that the Parsec only tracks out 10 of the motion Usually a setting of around 8 or 9 provides the b...

Page 19: ...mpensation in the mount is turned off On most telescopes the Right Ascension drive likes to have some load pushing against sidereal tracking If the mount is balanced such that it is pulling the mount...

Page 20: ...drift and correct by moving the mount in the appropriate direction To perform the drift method of polar alignment 1 Do a rough polar alignment by pointing the R A axis of the mount at Polaris the Nor...

Page 21: ...ng images of wide field deep sky objects such as the Andromeda Galaxy or the Pleadies star cluster Focal reducers will usually thread onto the nosepiece of the Parsec Barlow lenses increase the focal...

Page 22: ...ith anti reflection coatings Backfocus Distance from T threads 29 24mm 1 15 Weight 900g 32 oz Autoguider capability Yes Mounting 2 nosepiece or T thread Parsec 10100C CCD Sensor Kodak KAI 10100 CXC CC...

Page 23: ...wing two conditions 1 this device may not cause harmful interference and 2 this device must accept any interference received including interference that may cause undesired operation Changes of modifi...

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