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information from levels 1 to 254 and almost all the brightness information at level 
255. Thus a white image results.
If you plan to do all image processing within MaxIm DL Edition (or the optional 
full version of MaxIm DL), saving images in the FITS (.fit) 

File Format using the 

IEEE Float 

Size Format is recommended. This ensures that all saved data will 

be kept intact. If another 

Size Format is utilized, there may be some loss of data, 

especially when saving combined images.

6.  Multiple Camera Control 

for Autoguiding

One very nice feature of the MaxIm DL software is the ability to control two cam-
eras simultaneously. This way, you only need one computer and software program 
to image and autoguide at the same time. This feature is also compatible with older 
SSDSI cameras.
1.  Plug both cameras, one at a time, into the USB ports on your computer. 

Install the drivers for each camera as detailed prior in this instruction manual.

2.  Open the MaxIm DL software. In the 

Camera Control Window’s Setup 

tab that appears, select the imager as 

Camera 1 and the autoguider as 

Camera 2, then click Connect.

3.  Click on the 

Guide tab, Camera 2 will be assigned here.

6.1. Autoguider Calibration

If you are using a second camera as an autoguider, you must calibrate the system. 
The exact orientation of the camera, the focal length of the guide telescope optics, 
and the speed of the motor drive all affect the calibration. To perform autoguider 
calibration:
1.  Switch to the 

Guide tab.

2.  Set the 

X and Y Aggr (aggressiveness) to 8 to start with. Set the Exposure 

to 1.0 second. Under 

Guide Star, make sure the Watch box is checked.

Note: The 

and YAggr (aggressiveness) controls on the Guide tab allows you 

to adjust how vigorously star motions are tracked out in each axis. An aggres-
siveness setting 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 best tracking, since 
it reduces overshoot and helps ignore random motions due to atmospheric see-
ing and wind loads. You should experiment to determine the best setting for your 
particular telescope.
3.  Click the 

Settings button (Figure 32).

4.  Maxim DL needs to know how fast the telescope moves in right ascension 

(R.A.) and declination (Dec.) when the autoguider commands are issued. To 
do this, the software will 

Calibrate the mount by moving it back and forth on 

each axis. The 

Calibration Time determines how long it activates the motors 

each time. The usual value is 5-10 seconds; start out with a value of 5.

5.  Make sure all of the 

Guider Enables boxes are checked.

6.  For 

Autoguider Output, set Control Via. If you are using the Orion 

StarShoot AutoGuider for example, choose 

Guider Relays.

7.  Click 

Apply. You can leave this dialog box open, or Close it if you wish.

8.  Make sure that the telescope mount is set to move at 1X sidereal or slower. 

For some mounts, you must set the guide rate manually. The maximum 
usable rate is 1X sidereal. If your mount does not drift quickly, you can set 
the speed slower than 1X depending on your imaging configuration.

9.  On the 

Guide tab, set to Expose, and click the Start button. A single image 

will be taken. Ensure that a well-focused bright star (near the actual object 
to be imaged) appears in the image. If not, adjust the guide scope and try 
again. Make sure the star is roughly centered.

Note: The algorithm can be confused if another star appears in the frame; to mini-
mize this risk, calibrate on an isolated bright star.
10. Now, set to 

Calibrate, and click the Start button. A series of five exposures 

will be taken; each time the telescope will be moved slightly. If the telescope 

Figure 32. 

The 

Guider Settings configure your autoguider in MaxIm DL.

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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