8 Feb 1994 This directory contains revised versions of source code files from the Guide Star Survey Sampler CD-ROM. All files can be copied in ascii mode. These changes have three purposes: (1) They repair several problems that have been encountered using the software on VMS systems. With the changes we believe the programs will work around some problems with the "VFS MOUNT" software that is sometimes used to read CD-ROMs on VAXes, and the output FITS and hhh/hhd format files should be compatible with any other software. (The MODIFY program used with earlier versions is no longer needed.) (2) They include a modification that allows the programs to read the CD-ROM files correctly on Unix systems that cause the files to appear with uppercase names instead of lowercase names. This happens on at least some Decstations running Ultrix. If you have this problem, edit makefile and remove the comment symbol ('#') from the line at the beginning of the file that says #MORECFLAGS = -DULTRIX (3) They provide an entirely new capability to smooth the decompressed images by adjusting the H-transform coefficients. The effect is that the "blockiness" that appears in highly compressed images is removed. The smoothing adapts to the structure in the images; for example, it does not blur star images. The smoothing has little effect on images at the lowest compression ratio, but produces images that appear noticeably more natural on the highest compression images. The changes are most dramatic for images that include some extended emission (nebulosity or large galaxies). To build the program, copy these new files and compile the programs again using the "make" command for Unix or "@make" for VMS. Run the programs as before, but optionally add the switch "-s" to the command line to specify that the extracted images should be smoothed. For example, to run IMEXTRCT, the program that extracts an image at a specified RA and Dec, do imextract.csh -s high (Unix) @imextrct -s high (VMS) to extract a smoothed image from the high compression version of the plates. As before, if the compression ratio (low, medium, or high) is omitted the low compression plates are used; if the smoothing switch is omitted then the images are not smoothed. Copyright (c) 1993 Association of Universities for Research in Astronomy. All rights reserved. Produced under National Aeronautics and Space Administration Contract No. NAS5-26555. gscdist@stsci.edu (Internet) SCIVAX::GSCDIST (SPAN), or GSCDIST@STSCI (BITNET), or (410) 338-5090 FAX, or paper mail to GSC Distribution Office SCARS Division Space Telescope Science Institute 3700 San Martin Drive Baltimore, MD 21218 U.S.A.