| Instrument | 
			Takahashi FSQ-106ED @ 
			f/5.0 (530 mm F.L.) Captured at 2.1 arcsec/pixel.  Shown at 
			4.30 and 9.16 arcsec/pixel. | 
		
			| Mount | 
			
			Losmandy G11 with Gemini L4 v1.0 | 
		
			| Camera | 
			SBIG STF-8300M Self 
			Guiding Package w/ mono ST-i, using Baader LRGB filters. | 
		
			| Acquisition Data | 
			12/23/2014 to 
			2/9/2015 Chino Valley, AZ... with CCDSoft & CCD Commander | 
		
			| 
			
			Exposure | 
				
					| Lum | 399 
					min. (57 x 7 min. bin 1x1) |  
					| 
					Red | 
					119 min. (17 x 
					7 min. bin 1x1) |  
					| 
			Green | 
			154 min. (22 x 7 min. bin 1x1)
			
					 |  
					| 
			Blue 
					 | 
			175 min. (25 x 7 min. bin 1x1)
			
					 |  
				
					| 
			Nebula Core Exposures |  
					| Lum | 15 
					min. (30 x 30 sec. bin 1x1) |  
					| 
					RGB | 
					30 min. (20 x 
					30 sec. each bin 1x1) |  
					RGB combine 
					ratios were 1.0, 1.21 & 1.41 | 
		
			| 
			
			Software & Processing Notes | 
				
				
				CCDSoft, CCDStack, 
				PixInsight & Photoshop CS6. 
				
				
				A standard image-train 
				calibration was used, as determined by
				
				eXcalibrator v4.30, and then adjusted for altitude 
				extinction.
				
				
				CCDStack to 
				calibrate both luminance and color exposures, register the color 
				exposures and creating the two RGB images.
				
				PixInsight 
				processing includes registering the luminance 
				exposures and creating the two Lum images.  HDRComposition 
				was use to combine the long and short exposures.  
				Non-linear stretching was done with HistogramTransformation and 
				MaskedStretch. HDRMultiscaleTransform and 
				LocalHistogramEqualization were used to enhance the detail.  
				
				PhotoShop for the 
				LRGB combine & final touch-up. 
				
				Noiseware 5, a 
				PhotoShop plug-in. | 
		
			| 
			Comment | 
			North is to the top. 
			The Orion Nebula (also 
			known as Messier 42, M42, or NGC 1976) is a diffuse nebula situated 
			south of Orion's Belt. It is one of the brightest nebulae, and is 
			visible to the naked eye. M42 is located at a distance of 1,270±76 
			light years and is the closest region of massive star formation to 
			Earth. The M42 nebula is estimated to be 24 light years across. 
			Source:
			
			Wikipedia |