Image Processing from the Cutting Edge
Imagers from as far away as Chile were treated to presentations by a host of expert astrophotographers. Many of the talks focused around the debate of what is "true color" in astrophotography. Don Goldman summed up the camps of color image processing as falling into two groups: the histogrammers those who predominately use Photoshop's "histogram" functions to monitor changes made during various processing steps, and the G2Vers imagers who calibrate color data based on the color of a Sun-like G2V star.
From the histogrammer camp, imaging mavericks such as Ron Wodaski, who's book The New CCD Astronomy has become the standard text introduction to image processing, demonstrated his "zone system" technique, by dissecting the histogram data. Sky & Telescope contributing photographer Tony Hallas (who recently moved to the digital medium) gave tips on artistic image composition and color balance. G2Vers John Smith and Stan Moore both presented an analytical approach to image acquisition and calibration.
Sponsors Santa Barbara Instrument Group (SBIG), Software Bisque, and RC Optical Systems all used the opportunity to announce new products and to give attendees a window into the future of CCD imaging. SBIG showcased products such as the ST-402, a new deep space spectrograph, and tentative plans for two CCD cameras based on new Kodak chips. Software Bisque unleashed the Software Bisque Observatory Suite (SBOS), software integration that ties together all parts of the user's observatory into one manageable package, and the Telescope Control System (TCS), which retrofits the legendary Paramount technology to other manufacturers' mounts. RC Optical announced a new field flattener for its Ritchey-Chrétien reflectors to accommodate the growing size of CCD chips.
Other manufacturers present were Bob Denny of DC3-Dreams, who demonstrated his ACP observatory control software, and CCDWare which announced the release of PEMPro, a program that learns your mount's periodic error and take it into account, to create perfectly tracked subexposures without the need of an autoguider.





