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                    °Þ²       ÄÄGAMMAÄRAYÄBURSTÄÄ       ²Ý°                  
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            ß  P  R  O  U  D  L  Y      P  R  E  S  E  N  T  S    ß            
                                                                            
                                                                             
                MEDIA.CYBERNETICS.AUTOQUANT.X.V2.1.3_X86-GRB                                                                     
                                                                              
    _  __  ___  ____  _____  ______  _______  ____________________________     



                       DATE.......: 07/02/2009  
                       SUPPLIER...: GRB            
                       CRACKER....: GRB         
                       PACKER.....: GRB                
                       TYPE.......: Crack                
                       PROTECTION.: HASP                               
                       SIZE.......: 18x.5.00MB                       
                       URL........: http://www.mediacy.com/index.aspx?page=AutoDeblurVisualize
                      
                                                 
                  Ü  Ü                                   Ü  Ü                
                   ßßÜ                                   Üßß                 
                    °Þ²         RELEASE NOTES           ²Ý°                  
                    ÜÛß                                 ßÛÜ                  
               ÜÜÜÛßß                                     ßßÛÜÜÜ             
            ÜÛÛßß                                             ßßÛÛÜ          
           Þ²Ýß                                                 ßÞ²Ý         
            ß                                                     ß            
                                                                            
                  All microscopes are limited by the laws of   
                    physics, and these laws state that when    
                   light passes through a medium, that light   
                   will bend. This is one of the most common   
                     causes of haze and blur in microscopy     
                    images. Deconvolution can correct this     
                    problem, not only removing the haze and    
                blur, but restoring vital detail to datasets.  
                                                               
                     AutoDeblur® offers the most powerful      
                    deconvolution tools available for life     
                    science research.  Retrieve better data    
                   from your images using the most complete    
                   suite of 2D and 3D algorithms available.    
                   It offers an advanced Blind Deconvolution   
                     algorithm which is both iterative and     
                                 constrained.                  
                     Unlike other deconvolution products,      
                    AutoDeblur does not require the manual     
                   calibration and measurement of the point    
                      spread function (PSF).  Instead, it      
                     constructs the PSF directly from the      
                   collected data set. AutoDeblur works with   
                       widefield epi-fluorescence, DIC,        
                    transmitted-light brightfield and most     
                   Confocal microscopes including two-Photon   
                              and spinning disk.               
                     In addition to the full complement of     
                  algorithms, AutoDeblur offers several other  
                     advantages as well.  It is based on a     
                     multiDimensional platform, capable of     
                  handling 3D time-series datasets.  Instead   
                   of loading each time point one at a time,   
                      and processing them through a batch      
                   process, they can be loaded and processed   
                             as a single dataset.              
                    Another advantage of AutoDeblur is the     
                   ability to load a nearly limitless number   
                       of channels, freeing you from the       
                  constraints of the world of RGB.  You also   
                  have full control over the display of each   
                   channel - choose from the lists of custom   
                  colors, wavelengths, dyes, or color mapping  
                        to best display your dataset.          
                   Let AutoDeblur show you what you 've been   
                  missing in your images, because better data  
                             means better science.             
                 
                  Ü  Ü                                   Ü  Ü                
                   ßßÜ                                   Üßß                 
                    °Þ²         RELEASE INFOS           ²Ý°                  
                    ÜÛß                                 ßÛÜ                  
               ÜÜÜÛßß                                     ßßÛÜÜÜ             
            ÜÛÛßß                                             ßßÛÛÜ          
           Þ²Ýß                                                 ßÞ²Ý         
            ß                                                     ß            
                                                                            
                                  1. extract                   
                                  2. install                   
                          3. replace in program files          
                            *:\Program Files\Media             
                           Cybernetics\AutoQuant X2            
                        4. Gamma Ray Burst is Shining.         


                  Ü  Ü                                   Ü  Ü                
                   ßßÜ                                   Üßß                 
                    °Þ²            GROUP INFO           ²Ý°                  
                    ÜÛß                                 ßÛÜ                  
               ÜÜÜÛßß                                     ßßÛÜÜÜ             
            ÜÛÛßß                                             ßßÛÛÜ          
           Þ²Ýß                                                 ßÞ²Ý         
            ß                                                     ß            
                                                                            
                                                       
     Gamma-ray bursts (GRBs) are the most luminous electromagnetic events 
               occurring in the universe since the Big Bang.                                                        
     Since GRBs in metal-rich galaxies like the Milky Way are rare, mass 
       extinctions due to GRBs may only happen once per billion years.
                  Dedicated To Quality And Not To Quantity

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                               J O I N - W A N T E D
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                            Take a look at the Milky Way
 
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                    !DZr                                  01.01.2K9!