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Using eXcalibrator w/ PixInsight 
Data 
  
	
		| 
		 
		With version 4.2, 
		eXcalibrator supports PixInsight (PI) 32-bit floating point and both 
		16-bit signed and unsigned FITS files.  This document assumes that 
		the reader is familiar with eXcalibrator. 
		
		PixInsight offers multiple 
		options for the FITS format. This introduces two problems for 
		eXcalibrator, data scaling and the vertical flip. To keep things simple, eXcalibrator assumes 
		that the files are created with the PixInsight default settings. 
		EXcalibrator only checks the WCS File for the use of PI images.  
		
		Data Scaling 
		
		In the case of 32-bit floating-point data, PI scales the 
			pixel values from 0.0 to 1.0. Internally, eXcalibrator equally 
		rescales the three color files to a 16-bit (0.0 to 65535.0) scale. 
		
		The Vertical Flip 
		
		PixInsight allows the user 
		to choose how 
		FITS images are displayed. The default method is 
		with no vertical flip. The dialog window, in Image1, shows the default 
		settings. The Upper Left Corner selection displays a FITS image without 
		a vertical flip. This agrees with most amateur astronomy software, 
		including eXcalibrator. 
		
		With the Lower Left Corner 
		setting, PI displays the image flipped vertically. Apparently, this 
		method is preferred by the professional astronomers. 
		To display the PI FITS Format 
		Preferences window click View | Explore Windows | Format Explorer and 
		double-click FITS.  | 
	 
 
  
  
Image1 
	
		| 
		 
		Now here is where it gets 
		interesting 
		
		The PixInsight image 
		solver always puts a vertical flip in the FITS Scale Matrix, relative to 
		how the image is displayed. This gives a FITS image with no vertical 
		flip in the data and a vertical flip indication in the Scale Matrix. 
		This confuses many programs such as eXcalibrator and Aladin. Image2 
		is a partial Aladin screenshot showing this problem.  | 
	 
 
 
  
Image2 
  
	
		| 
		 
		In the case for
		Image3, the 
		FITS file was loaded with the Lower Left Corner option for the 
		coordinates origin. This displays the image flipped vertically in 
		PixInsight. Once again, the Image Solver flips the Scale Matrix 
		vertically relative to the displayed image. This results in a saved 
		image with the Scale Matrix in agreement with the image data. Now 
		programs, other than PixInsight, can correctly analyze the image. See 
		Image3 for the Aladin result.  | 
	 
 
  
Image3 
	
		| 
		 
		eXcalibrator's Solution 
		
		When eXcalibrator loads 
		the WCS File, 
		the user is asked if the RGB data should be flipped vertically. If you 
		are not sure, try it both ways. The correct choice will return more 
		stars. 
		
		Here are some guidelines. 
			- 
			
			With PixInsight, plate 
			solve one of the three color images and save all three as a 32-bit 
			floating point FITS. In eXcalibrator, load the plate solved image 
			into the WCS File text box. Finally, load all three files into their 
			respective Red, Green and Blue text boxes. 
			In this case, 
			use the vertical flip function.
			  
			- 
			
			With other plate 
			solving software... 
			In PixInsight, save all three color images as 32-bit floating point 
			FITS. With your favorite software, plate solve one of these three 
			images and save it separately. In eXcalibrator, load the plate 
			solved image into the WCS File text box and the other three files 
			into their respective Red, Green and Blue text boxes. 
			In this case, 
			do not use the vertical flip function.  
		 
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