~cloos/ghostpdl - Clone of git://git.ghostscript.com/ghostpdl.git.

Age	Commit message (Collapse)	Author	Files	Lines
2011-03-04	Reorganization of threshold code to move all the thresh holding operations ↵	Michael Vrhel	1	-0/+13
	into a new file. git-svn-id: http://svn.ghostscript.com/ghostscript/trunk@12238 a1074d23-0009-0410-80fe-cf8c14f379e6
2011-03-02	Introduction of a member variable in gs_image1_t, which will let us know the ↵	Michael Vrhel	1	-0/+18
	original source type of the image. For example if, the parent source were type3 this spawns two type1 images. One for the mask and one for the image data. The mask is rendered using image render simple. If the image is monochrome or indexed, it is rendered with the renderer in gximono.c . If we are going to a halftone monochrome device, we end up using the fast threshold based renderer which has its interpolation stepping in device space as opposed to source space. This causes very minor differences between the mask and the image data. To avoid this, we use the old rect_fill code for the image type3 data to ensure a more exact spatial match. git-svn-id: http://svn.ghostscript.com/ghostscript/trunk@12227 a1074d23-0009-0410-80fe-cf8c14f379e6
2008-08-29	Split the source tree into two new directories.	Ralph Giles	1	-0/+300
	PSSRC files are now in 'gs/psi'. GLSRC files are now in 'gs/base'. This is to facilitate build modularization and merging in the ghostpdl tree. NOTE: msvc32.mak is now in psi, not src. git-svn-id: http://svn.ghostscript.com/ghostscript/trunk@9048 a1074d23-0009-0410-80fe-cf8c14f379e6