% @(#)copy_pscr.hlq 17.1.1.1 (ESO-IPG) 01/25/02 17:43:26 %++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ %.COPYRIGHT (c) 1990 European Southern Observatory %.IDENT copy_pscr.hlq %.AUTHOR KB, IPG/ESO %.KEYWORDS MIDAS, help files, COPY/PSCR %.PURPOSE On-line help file for the command: COPY/PSCR %.VERSION 1.0 17-FEB-1997 : Creation, KB %---------------------------------------------------------------- \se SECTION./PSCR \es\co COPY/PSCR 19-SEP-1995 KB \oc\su COPY/PSCR image [PS_file] [options] [prnt_flags] [scales] [LUT_specs] convert MIDAS images (bdf-files) to PostScript format \us\pu Purpose: Convert MIDAS images (bdf-files) to PostScript format. \up\sy Syntax: COPY/PSCR image [PS_file] [options] [prnt_flags] [scales] [LUT_specs] \ys\pa image = name of MIDAS image \ap\pa PS_file = name of Postscript file; \\ defaulted to `image' name with ".ps" appended \ap\pa options = optional string of up to 9 option_flags ("wbneavfNE"); \\ w - add an intensity wedge to the right of each frame \\ b - use a blue background color instead of white \\ v - will list the origin and scale parametrs for each frame \\ n - use a negative ITT instead of a positive ramp \\ e - use an exponential ITT instead of a linear one \\ a - autoscale bdf-file to fit into display area (paper size) \\ f - draw a frame box around the image \\ N - no frame identifier will be included \\ E - create an Encapsulated PostScript file which can be embedded in other documents \ap\pa prnt_flags = page_format,resolution; \\ page_format can be one of the following: \\ A4P, A4L, A3P, A3L, S4P and S4L, \\ the first two letters define the page size as A3/A4 or S4, which is for Slide format being A4 with wider margins, the last letter is P or L for portrait or landscape; \\ resolution specifies the resolution of the printer in pixels per cm, if this parameter is 0 or not given the printer default is used; \\ defaulted to A4P,0 \ap\pa scales = xscales,yscales to specify the scaling of the image as xscale,yscale in world coordinates per cm; \\ by default the image will be scaled to fill the full available area with xscale=yscale \ap\pa LUT_specs = 0, 1, 2 or 3 for simple internally generated LUTs, or name of LUT stored as standard MIDAS table (in current dir!) \ap\sa See also: COPY/DISPLAY, @a outima \as\no Note: The cut values for the pixel intensity is taken from descr. LHCUTS. \\ The PostScript file can be viewed with any viewer (e.g. Ghostscript or xv) and printed out on a PostScript printer with the `lp' command. A color PostScript file requires a color printer to come out correctly. \on\exs Examples: \ex COPY/PSCR galaxy ? wn p6=3 Image `galaxy.bdf' is converted to the color PostScript file `galaxy.ps' using the internal LUT no. 3. A negative ITT is also used and a color wedge is added to the right of the image. \xe\ex COPY/PSCR n2997 n2997.eps En MIDAS image `n2997.bdf' is converted to an Encapsulated PostScript file `n2997.eps' using a negative ITT. The EPS file `n2997.eps' can then be enbedded in other documents. \xe \sxe