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1.  Introduction

Welcome to the exciting world of astro-imaging. Your new 
Parsec

 Astronomical Imaging Camera is capable of captur-

ing professional quality astro-images of your favorite celestial 
objects. You can showcase spectacular images on your com-
puter, share them on the internet, or print them. The camera’s 
large 8.3 mega-pixel array provides very high resolution imag-
es which are great for publishing in large prints.

Please read this instruction manual before attempting to use the camera or install 
the needed software. For the most detailed information on specific camera and 
software functions, consult the Maxim DL 

Help Topics included with the CD; the 

tutorials found there are especially useful for familiarizing yourself with the soft-
ware and camera.

1.1. the Parsec 8300

The Parsec 8300 is a high resolution, 8.3 megapixel CCD with a dual-stage, 
regulated thermoelectric cooler to enable maximum imaging performance. Both 
the 8300M and 8300C are very sensitive and capable of detecting faint deep sky 
objects in a short exposure; and longer exposures can reveal extremely deep 
fields with subtle nebulosity and galaxies in the background.
The unique versatility of the Kodak KAF8300 full frame CCD lets you take advan-
tage of the densely-packed pixel array. 1x1 mode (3326 x 2504) utilizes the full 
resolution of the camera, providing the most detailed images and largest possible 
prints. Binning in 2x2 mode (1663 x 1252) increases the camera’s sensitivity and 
full well capacity (meaning it can collect more light) at the expense of resolution. 
Binning in 2x2 mode can be especially useful for longer focal length and higher 
focal ratio telescopes. Note that the Parsec 8300C model will not have any color 
in 2x2 mode.

1.2. the Parsec 10100C

The 10.7 megapixel Parsec 10100C uses Kodak’s KAI10100 interline CCD. It has 
the same cooling system and architecture as the Parsec 8300, but with slightly 
faster data transfer to accommodate the higher number of pixels (3760 x 2840 in 
1x1, 1880 x 1420 in 2x2). Additionally the number of binning modes includes 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 
general, the longer focal length telescopes (like RCs and SCTs) are more suited 
to image with in 2x2 for this particular CCD sensor, because the pixels are small. 
Imaging in 2x2 mode makes each pixel size the equivalent of 10.8 microns instead 
of 5.4 in 1x1 mode. Binning 2x2 with color cameras is normally captured in mono-
chrome only. But the Parsec 10100C can bin 2x2 in color. 

1.3. Feature Highlights

• 

Simple interface: A USB port and power port are all that’s needed to 
power and connect to the Parsec (Figure 1).

• 

Dual

-

stage thermoelectric cooler: Dramatically reduces thermal noise in 

all images.

• 

Regulated cooling: Enables you to set the exact temperature within the 
cooling range of the camera. This allows you to take calibration images like 
dark frames at the exact same temperature as your light frames, making for 
the cleanest images possible. Additionally, since you can match the CCD 
temperature at any time (within the range of the cooler), you have the freedom 
to take dark frames when it’s most convenient for you, so you don’t have to use 
up valuable imaging time to take dark frames.

• 

Regulated cooling fan speed: Three fan speed settings allow you to set 
the speed to your liking. High is the loudest but most effective setting.

• 

Shutter: A shutter is necessary for Kodak CCD chips, but it also enables 
you to automatically take dark frames without having to cap the front of 
your telescope. This is especially useful when taking autosave image 
sequences.

• 

High speed USB 2

.

0 interface and internal memory buffer: The full 

frame 32 megabyte SDRAM on-board memory ensures a clean image 
download each time, even if the system resources of your PC are 
temporarily compromised. The high-speed USB 2.0 downloads the full 
frame within 15 seconds depending on your computer speed.

• 

Compact design: With a footprint of just 4" x 4" with 3" of depth, the 
Parsec easily fits into your imaging setup. The Parsec’s compact size also 
makes the camera suitable for Celestron

®

 Hyperstar or Fastar systems.

Figure 1. 

Parsec ports and LEDs.

Tripod adapter

Power port

USB port

LED 2

LED 1

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...

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