| 
			 Instrument  | 
			
			 
			Takahashi FSQ-106ED @ 
			f/5.0 (530 mm F.L.) Captured at 2.1 arcsec/pixel.  Shown at 
			2.93 and 5.29 arcsec/pixel.  | 
		
		
			| 
			 Mount  | 
			
			 
			
			Losmandy G11 with Gemini L4 v1.0  | 
		
		
			| 
			 Camera  | 
			
			 
			SBIG STF-8300M Self 
			Guiding Package w/ mono ST-i, using Baader RGB filters.  | 
		
		
			| 
			 Acquisition Data  | 
			
			 
			2/8/2015 & 
			2/10/2015  
			Chino Valley, AZ  | 
		
		
			| 
			 
			
			Exposure  | 
			
			
				
					| 
					 
					Red  | 
					
					 
					 70 min. (10 x 
					7 min.)   bin 1x1  | 
				 
				
					| 
					 
			Green 
					  | 
					
			 84 min. (12 x 7 min.)        
			"  | 
				 
				
					| 
					 
			Blue 
					  | 
					
					 
			105 min. (15 x 7 min.)        
			"  | 
				 
				 
			
			eXcalibrator RGB 
			ratios are 1.00, 1.22, 1.39  | 
		
		
			| 
			 
			
			Software  | 
			
			
				- 
				
				CCDSoft, CCDStack, 
				PixInsight & Photoshop CS6.  
				- 
				
				
				eXcalibrator 
				v4.36 for (g:r) color balancing, using 
				798 stars from the 
				SDSS-DR9 database.  
				- 
				
				CCDStack to 
				calibrate all sub exposures, register, stack and create the RGB image.  
				- 
				
				PixInsight 
				processing includes gradient removal and non-linear stretching 
				with HistogramTransformation.  
				- 
				
				PhotoShop for 
				the final touch up.
				  
			 
			 | 
		
		
			| 
			 
			Comment  | 
			
			 
			North is to the 
			top. 
			
			M35, or NGC 2168, is 
			an open cluster in the constellation Gemini, at a distance of about 
			2800 light years. At only 150 million years old, M35 s a classic 
			example of a young open cluster with very hot young blue stars.  
			 
			To the lower right is the tightly grouped cluster NGC 2158. This 
			cluster is about 2 billion years old. The much older stars of the 
			cluster account for its yellowish color. It is about 9000 light 
			years further away than M35. This greater distance may also slightly 
			contribute to the yellowish color. 
			 
			To the far right–center are the two sparse clusters IC2156 and 2157.  |