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ACKNOWLEDGMENTS
Images have been provided by the Jet Propulsion Laboratory, Meade Instruments Corporation, Santa Barbara Instrument Group, Astrolink, Inc., SSC
Observatories and other private sources.
LIMITED WARRANTY
LIMITED WARRANTY. Meade Instruments warrants that (a) the SOFTWARE will perform substantially in accordance with the accompanying written
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NO LIABILITY FOR CONSEQUENTIAL DAMAGES. In no event shall Meade Instruments, or its suppliers, be liable for any damages
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Instruments Corporation, 16542 Millikan Avenue, Irvine, California 92714.
A Note on Accuracy ....................................................................................................................................................... 7
System Requirements................................................................................................................................................... 7
Registering the Program .............................................................................................................................................. 7
2. Features ........................................................................................................................................................... 9
Tool Bar ................................................................................................................................................................ 9
8 Bit versus 12 or 16 Bit or Floating Point Grayscale Images................................................................................................. 11
Close ................................................................................................................................................................................12
Save As Fits Image ..................................................................................................................................................... 13
Median Filter.................................................................................................................................................................. 23
Fix Hot Pixels................................................................................................................................................................. 23
Set Reference Magnitude ........................................................................................................................................... 28
List Pixel Values ........................................................................................................................................................... 31
Group Edit ....................................................................................................................................................................... 33
Night Vision.................................................................................................................................................................... 37
Grayscale Palette and Standard Palette................................................................................................................. 38
Appendix A ........................................................................................................................................................ 39
Welcome to Meade Autostar IP astronomical image processing software. Now you can perform many of
the same image processing tasks that a professional astronomer would do on a large institutional
computer. With Meade Autostar IP you can:
•Enhance high resolution images using advanced image processing techniques.
•Determine stellar magnitudes directly from electronic images, and a number of other powerful
features.
A Note on Accuracy
Meade Autostar IP was designed to be extremely powerful and accurate. Many programs designed for
the PC have taken shortcuts to appear faster, but at the expense of accuracy! Not Meade Autostar IP! By
carefully coding each section of the program using 64 bit floating point numbers, Meade Autostar IP takes
full advantage of your computer to provide fast and accurate performance. This gives you the power and
accuracy that rivals main-frame computer performance.
System Requirements
The minimum system required to run Meade Autostar IP are as follows:
•64 MB RAM.
•Hard Disk with 20 Megabytes of free space.
•An VGA or better adapter and compatible monitor.
•Microsoft Windows 98SE or above.
•A Microsoft compatible mouse.
Autostar IP
Registering the Program
Please take the time to fill out and mail the Registration Card you received with Meade Autostar IP.
Registering Meade Autostar IP entitles you to the following additional benefits:
•Meade 's technical support, if you have difficulty using Meade Autostar IP.
•Automatic notification of upgrades or revisions to Meade Autostar IP.
•Automatic notification when new images or data become available.
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1. Installation
Autostar IP is installed as part of Meade’s Autostar Suite. If you have not yet installed the Suite, consult
the quickstart instructions for the complete instructions.
Typcially, when the Autostar Suite CD ROM is inserted in your computer it will automatically begin the
install process. If your system has “autoplay” disabled, click on START, then click on RUN. When the run
dialog box appears, type
A:SETUP then press Enter.
The Setup program will prompt you for the desired drive and path in which to install the program and data
files. Then it will begin uncompressing the files from the distribution disks and copying them to the
appropriate locations on the Hard disk. Make sure you have at least 60 Megabytes of free space on the
destination drive.
Once the installation is complete, Meade Autostar IP will be ready to help you begin processing your own
images.
Autostar IP
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2. Features
Tool Bar
Autostar IP's Tool Bar gives you immediate access to image files to perform complex image processing
with the click of a button.
Status Bar
Autostar IP's "live" Status Bar constantly updates the coordinate display of the image, and the pixel value
(Dn.) of the image, as well as the local time. The Status Bar can also be customized under the
Preferences command under the File menu.
Menu Bar
Autostar IP
The familiar W indows Menu Bar gives you access to every function of Autostar IP. To access a drop down
menu file, either click with the mouse or press Alt and the letter underlined from the keyboard.
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3. File
Open
Autostar IP
The file menu contains a number of commands for opening and closing image files, and printing
images.
The Open command from the File menu or the button of the Tool Bar allows you open either images or
spectrographs in any of the following formats:
TIFF- Tagged Image File Format (16bit grayscale)
FITS- Flexible Information Transport System (8 or 16 bit or floating point grayscale)
BMP- Windows Bitmap Format (8 bit grayscale, 256 color, or 24 bit color)
LNX- Spectra Source Lynxx format (12 bit grayscale)
ST7- Santa Barbara Instrument Group (16 bit grayscale)
ST6- Santa Barbara Instrument Group (16 bit grayscale)
ST4- Santa Barbara Instrument Group (8 bit grayscale)
08B- Raw (8 bit grayscale). Similar to ST4.
In addition there is a RAW format for reading unknown image formats.
Images may only be saved in TIFF, FITS or BMP formats.
To open a file:
- Select the desired format.
- Select the directory and filename from the list boxes
OR
- Enter the desired filename in the edit box.
If the filename is specified without an extension, a default extension will be automatically added to the
filename to reflect the current format. If the extension is provided, it will over-ride the current selection
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Autostar IP
Regardless of the file type, the image data will be converted to 16 bit integer data. This assures that high
precession is maintained throughout image processing.
If the image is an RGB color image, you will be prompted as to which color plane you wish to load. The
following dialog will appear:
If you select Load As Color Image, the program will load all three color planes and display the image. As
an astronomical image processing program, Autostar IP is designed primarily to work on gray scale
images. Some of the more advance processing features will not be available when a color image is
loaded. If you wish to apply these more sophisticated techniques, load each plane individually, process it
and save it in a temporary file. These can later be combined back together to form the desired color
image.
8 Bit versus 12 or 16 Bit or Floating Point Grayscale Images
When 12 or 16 bit or Floating point images are loaded, they need to be scaled down to 8 bits (256 gray
levels) for display, which is the maximum number of simultaneous gray shades that Windows can display
at one time. All of the image information is loaded an processed by the program, but it needs to be
scaled down to 256 gray levels for presentation. This scaling is called Prescaling. By default the program
is options are set to automatically prescale image data. At anytime you can manually prescale the data to
suite your taste.
If you elected to disable automatic prescaling, the program displays the Image Prescale dialog box when
an image is loaded that allows manual setting of the parameters used to compress the data into an 8 bit
display format. This dialog box displays the histogram of the raw data in a large graph at the top and, at
the bottom, a smaller graph of the resulting data after the display scaling operation.
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Autostar IP
Although the display shows only 256 levels, all of the image data are retained and processed by the
program. Whenever you perform a processing step, you are given an opportunity to rescale the display
data. The scale command, also allows you to rescale the image any time you desire.
When prescaling an image, a histogram is constructed that shows the distribution of the data contained in
the image. Normally the data is distributed in a rather narrow range of values which lends itself to scaling
to the 8 bit format. Once the histogram is constructed, the Threshold values of the data is calculated and
are used to set the scaling range. This gives a reasonable starting point for scaling most images. The
threshold values may be reset at any time by pressing the Threshold button.
Close
Since the data is not evenly distributed, some fine-tuning of the limits is usually needed. This is
accomplished by using one of the predefined scaling options or by moving the red markers located under
the main histogram display. Generally, the best images are obtained with the markers set just at the high
and low edges of the important data. Values that are above the upper marker result in pure white pixels,
while those below result in pure black.
If the Std. Dev. button is depressed the Mean and Standard Deviation of the image are calculated. The
upper limit is set to the Mean plus 5 Standard Deviations, while the lower limit is set to the Mean minus 1
Standard Deviation.
The Min Max button sets the pointers to the extreme minimum and maximum values contained in the
image, while Full Scale sets the values to maximum and minimum values in the image.
If you are loading images from an RGB composite set of files, you may find it useful to use the same
scaling values for each of the individual images. This is easily accomplished by using the Use PreviousScale Values button located at the bottom the dialog box. Since many astronomical images contain a
large amount of red light, you may want to load the red image first, scale it properly, then use the same
scaling values for both the green and blue images.
Selecting Close will close the current file and remove its display window and any support windows, such
as the Histogram.
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Save As Fits Image
Displays the Save As dialog box and allows saving the current image data in a floating point FITS
formatted file. This method of saving insures that all of the information in the image is maintained. This is
the format recommended for keeping archival copies of your image data.
To save a file:
- Select the directory and filename from the list boxes
- Enter the desired filename in the Edit box.
If the filename is specified without an extension, a default extension will be automatically added to the
filename to reflect the current format. If the extension is provided, it will over-ride the current selection
Export Display As
Saves the currently display image to a file. This function is only available if the current format type is TIFF,
FITS or BMP. This command will save the image as displayed on your computer as an 8 bit or 24 bit data
in the format you request. Saving images this way will allow you to save images ready for use in
documents, but will discard part of the original image data
Autostar IP
OR
Revert
Print
To save a file:
- Select the desired format.
- Select the directory and filename from the list boxes
OR
- Enter the desired filename in the Edit box.
If the filename is specified without an extension, a default extension will be automatically added to the
filename to reflect the current format. If the extension is provided, it will over-ride the current selection
NOTE: All images are saved in the 8 bit versions of their respective format type, Some original
information may be lost.
The Revert command allows you to revert the image to the last saved version.
Selecting the Print command or pressing the Print button from the Tool Bar prints the current image on
the system’s default printer. The image is scaled so that it completely fills the printing area of the paper in
the horizontal direction. The vertical scale is then chosen to preserve the original aspect ratio of the
image. Additional information pertaining to the image is also printed at the bottom of the page, below the
image.
Printer Setup
Displays the Printer Setup dialog box which allows the selection of any of the currently installed printers.
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