If time-stamp is check marked then the time stamp will be written to the video. Alignment will be done against the first image in the list after alphabetic sorting. If time-stamp is check marked then the time stamp will be written to the aligned images.
Photometry tab. This tab allows measuring the magnitude change of one object in a series of images and detects automatically the four most variable objects. The butttons work the same as in the blink tab. Select the images to analyse. Preparation and usage of DSLR images for photometric measurements:. The light curve area has a pop-up menu to save it to file or copy it to the clipboard.
Measure variable stars. Mount analyse tab. This tab is intended to study mount pointing accuracy. Usage: take several images at different location in the sky.
Load the images in the tab. Selected the desired equinox. Click on the button add the astrometric solutions. Study the result and if required select all rows, copy and paste the whole result to a spreadsheet for further analysis.
This is normal the case. The solution can be written either in the orginal FITS file or in a seperate. Pixel math1 tab. Background equalization tool:. This background will be subtracted from the orginal image.
Step 6 will save the image with a new file name ending with "equalised". The same as 1 and needs to be overwritten.
Pixel math2 tab. Just select a number of images, click on the Analyse button. Then select all relevant files and copy the data with right mouse button.
Then copy the data into a spreadsheet for analysis. Here and example of the result in a spreadheet: Back to index. Viewer, file menu, thumbnail viewer for FITS files. Viewer, Tools, Batch processing :. With the batch routine several FITS image can be "astrometric solved" or converted.
Automatic conversion is integrated in the menus. They are displayed in the memo. Values are separated by a tab 9 and can be selected and copied to a spreadsheet. It can display only one table and will display the first table only. The file can be saved again but all binary values will be all written as 4 byte float.
Back to index. You could argue that a Johnson-V filter or green channel is required for the image but in practice the error is limited depending on the spectrum. Other popup menus:. Search for an object position:. Usage as astrometric solver and command line options :. For images in the viewer:. The simplest way to solve an image is just to load an image in the viewer and hit the solve button. Click on the save button to save the FITS file with the solution.
With the solution, the status bar will show the astronomical position of the mouse pointer. The program can be executed using command line options to solve images astrometric. Commandline parameters have priority above fits header values. Front-end programs should provide access to -z and -r options. Default value for -z should be 0 auto. Typical command lines :. If a FITS file is not available, preference is a non lossless image format like. PNG or. If possible in 16 bit or original 12 bit format.
Not stretched or saturated, as raw as possible. This setting can be learned and updated automatically with the parameters -fov 0. For the next solve using images from the same source the -fov 0 parameters can be omitted and solving will be fast.
The debug option allows to set some solving parameters in the GUI graphical user interface and to test the commandline.
In debug mode all commandline parameters are set and the specified image is shown in the viewer. Only the solve command has to be given manually:.
Raw format send via stdin should start with three longwords of 4 bytes. The first longword contains a format identification. The second longword contains the image width. The third longword contains the image height followed by the image raw data. Command-line, output files. In command line mode the program produces two output files at the same location as the input image.
In case a solution is found it will write a. No data, just the header. Any warning is added to the. This warning could be presented to the user for information. To have. Command-line, error codes. This is the same error as reported in the. Command-line pop-up notifier. To refresh the value move the mouse away and back. If the search spiral has reached a distance more then 2 degrees from the start position then a popup notifier will show the actual search distance and solver settings:.
Tray icons are default off in the latest Win10 version. Blind solving performance. Blind solving performance for a 90 degrees offset:. Usage as a solver with other programs or as PlateSolve2 substitute. Progress is shown in tray icon and popup notifier. Solving should be reliable. In case of failure, have a look to conditions required for solving. In case of solve failure please check the FOV indicated. EXE program as Platesolve2. Installation as solver for ModelCreator:.
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The cookie is used to store the user consent for the cookies in the category "Other. The cookie is used to store the user consent for the cookies in the category "Performance". It does not store any personal data. Image stacking Extremely fast and accurate. Several algorithms for every situation star fields, comets, planets, spectrums, etc. Color imaging Native 96 bit 32 bit for each color plane , visualized in real time without modifying the underlying data.
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