background image

20

21

should drop below 100% (Figure 17.3). If the 

Cooler Power does not drop 

below 100% after a couple of minutes, you will need to raise the 

Setpoint.

5.  Monitor the 

Sensor Temp and Setpoint and make sure they match. If the 

Senor Temp is higher than the Setpoint, you will need to raise the Setpoint.

We recommend keeping the 

Cooler Power to about 80% (or less) for the best 

performance while still having the ability to match the temperature later if needed. 
Pushing the cooler to near 100% will hinder the accuracy if your dark frames if the 
dark frame temperature does not match your light frame.

4.3. Imaging Deep Sky Objects

Capturing impressive images of deep sky objects, such as galaxies, nebulae, and 
star clusters, require relatively long exposures. You will take several individual 
images and stack them together to form one high-quality resultant image.
Very accurate polar alignment is essential for deep sky imaging. Stars will streak 
across the field of view without precise polar alignment and tracking. Longer expo-

sures of 60 seconds or more also require autoguiding with a separate camera. 
The Orion StarShoot AutoGuider can be operated with the Parsec in MaxIm DL.
To start:
1.  Acquire and center the deep 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 the eyepiece.

2.  Remove the eyepiece and replace it with the Parsec.
3.  Set the 

Exposure Preset to Focus and precisely focus the camera. If 

necessary, move the telescope to a nearby star to determine the best focus. 
For best results, when using the Parsec 8300C, select 

Light Raw for Frame 

Type so you can properly calibrate your astro-images later, see section 
5, “Image Processing”. For Parsec 8300M users, simply choose 

Light for 

Frame Type

.

4.  In the 

Expose tab, set Seconds to 10-20 and click Expose

.

 After the image 

downloads check to see if the deep sky object is centered well in your 
camera. Adjust the camera orientation if needed, keeping in mind that you 
may have to refocus the camera after making the adjustment. Reposition the 
telescope if needed to center the deep sky object.

5.  Set the 

Exposure Preset to LRGB, even if you are using the Parsec 8300C. 

You can always rename the 

Exposure Preset with your custom settings.

6.  Click the 

Autosave button, and select your exposure times, and frame type 

(Figure 18.1).

Figure 17.3. 

Monitor the 

Cooler PowerSensor Temp, and Setpoint and make sure 

they reach your goals.

Figure 18.1. 

The 

Autosave Setup window sets all of your options to autosave your 

image in a sequence.

Содержание PARSEC 10100C

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Отзывы: