> --- Ursprüngliche Nachricht --- > Von: Jan-Peter Homann <homann@xxxxxxxxxxxxxxxxxx> > Sometimes the compensation of optical brightners in > Profilemaker or PrintOpen helps. > > ** > Is there a comparable function in Argyll ? > ** Yes there is, if spectral measurements are available. See the options -f of the "profile" command. See also Graeme's paper http://www.imaging.org/store/epub.cfm?abstrid=22190 which describes the principles of the implemented algorithm. (Actually I'm wondering, whether the other professional profilers are probably based on Graeme's algorithm as well?) In addition to the measured spectral radiance factors, the algorithm requires the spectrum of the instrument's light source as input paramter (for instuments with a filter in the illumination path, of course the filtered light spectrum hitting the paper needs to be used). My understanding is, the algorithm eventually attempts to predict the spectral radiance factors of the patches, as if the paper were illuminated by the actual desired viewing illuminant (e.g. D50). Argyll currently assumes an illuminant A light source for virtually all instruments, which is probably a reasonable approximation for instruments with tungsten lamps, but which if of course not correct, if an UV filter is used, or if e.g. a Spectrolino is equipped with a D65 filter. Graeme was also so kind to add on my request Spectrocam's Xenon flash spectrum to spectro/inst.c and xicc/xspect.c, which can be selected for FWA compensation by setting TARGET_INSTRUMENT to "Spectrocam" in the .ti3 file. Regards, Gerhard -- 5 GB Mailbox, 50 FreeSMS http://www.gmx.net/de/go/promail +++ GMX - die erste Adresse f�r Mail, Message, More +++