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OpenSolaris 2009.06 - man page for dcraw (opensolaris section 1)

dcraw(1)										 dcraw(1)

       dcraw - command-line decoder for raw digital photos

       dcraw [OPTION]... [FILE]...

       dcraw decodes raw photos, displays metadata, and extracts thumbnails.

       -v     Print verbose messages, not just warnings and errors.

       -c     Write decoded images or thumbnails to standard output.

       -e     Extract  the  camera-generated  thumbnail,  not the raw image.  You'll get either a
	      JPEG or a PPM file, depending on the camera.

       -z     Change the access and modification times of an AVI, JPEG, TIFF or raw file to  when
	      the photo was taken, assuming that the camera clock was set to Universal Time.

       -i     Identify	files  but  don't  decode them.  Exit status is 0 if dcraw can decode the
	      last file, 1 if it can't.  -i -v shows metadata.

	      dcraw cannot decode JPEG files!!

       For dead pixel removal, see FILES.

       -k black
	      Set the black level.  Default depends on the camera.

       -K darkframe.pgm
	      Subtract a dark frame from the raw data.	To generate a dark  frame,  shoot  a  raw
	      photo with no light and do dcraw -D -4 -j -t 0.

       -n noise_threshold
	      Use  wavelets  to  erase	noise  while  preserving real detail.  The best threshold
	      should be somewhere between 100 and 1000.

       -C red_mag blue_mag
	      Enlarge the raw red and blue layers by the given factors, typically 0.999 to 1.001,
	      to correct chromatic aberration.

       -H 0   Clip all highlights to solid white (default).

       -H 1   Leave highlights unclipped in various shades of pink.

       -H 2   Blend clipped and unclipped values together for a gradual fade to white.

       -H 3+  Reconstruct  highlights.	Low numbers favor whites; high numbers favor colors.  Try
	      -H 5 as a compromise.  If that's not good enough, do -H 9, cut  out  the	non-white
	      highlights, and paste them into an image generated with -H 3.

       By  default,  dcraw  uses  a fixed white balance based on a color chart illuminated with a
       standard D65 lamp.

       -w     Use the white balance specified by the camera.  If this is not found, print a warn-
	      ing and use another method.

       -a     Calculate the white balance by averaging the entire image.

       -A left top width height
	      Calculate   the	white	balance  by  averaging	a  rectangular	area.	First  do
	      dcraw -j -t 0 and select an area of neutral grey color.

       -r mul0 mul1 mul2 mul3
	      Specify your own raw white balance.  These multipliers can be cut and  pasted  from
	      the output of dcraw -v.

       +M or -M
	      Use (or don't use) any color matrix from the camera metadata.  The default is +M if
	      -w is set, -M otherwise.	This option only affects Olympus,  Leaf,  and  Phase  One

       -o [0-5]
	      Select the output colorspace when the -p option is not used:

		   0   Raw color (unique to each camera)
		   1   sRGB D65 (default)
		   2   Adobe RGB (1998) D65
		   3   Wide Gamut RGB D65
		   4   Kodak ProPhoto RGB D65
		   5   XYZ

       -p camera.icm [ -o output.icm ]
	      Use  ICC profiles to define the camera's raw colorspace and the desired output col-
	      orspace (sRGB by default).

       -p embed
	      Use the ICC profile embedded in the raw photo.

       -d     Show the raw data as a grayscale image with no interpolation.  Good for photograph-
	      ing black-and-white documents.

       -D     Same as -d, but totally raw (no color scaling).

       -h     Output a half-size color image.  Twice as fast as -q 0.

       -q 0   Use high-speed, low-quality bilinear interpolation.

       -q 1   Use Variable Number of Gradients (VNG) interpolation.

       -q 2   Use Patterned Pixel Grouping (PPG) interpolation.

       -q 3   Use Adaptive Homogeneity-Directed (AHD) interpolation.

       -f     Interpolate RGB as four colors.  Use this if the output shows false 2x2 meshes with
	      VNG or mazes with AHD.

       -m number_of_passes
	      After interpolation, clean up color artifacts by repeatedly applying a  3x3  median
	      filter to the R-G and B-G channels.

       By  default,  dcraw  writes  PGM/PPM/PAM  with 8-bit samples, a BT.709 gamma curve, a his-
       togram-based white level, and no metadata.

       -W     Use a fixed white level, ignoring the image histogram.

       -b brightness
	      Divide the white level by this number, 1.0 by default.

       -4     Write 16-bit linear samples (fixed white level, no gamma).

       -T     Write TIFF with metadata instead of PGM/PPM/PAM.

       -t [0-7,90,180,270]
	      Flip the output image.  By default, dcraw applies the flip specified by the camera.
	      -t 0 disables all flipping.

       -j     For  Fuji Super CCD  cameras,  show  the image tilted 45 degrees.  For cameras with
	      non-square pixels, do not stretch the image to its correct aspect  ratio.   In  any
	      case, this option guarantees that each output pixel corresponds to one raw pixel.

       -s [0..N-1] or -s all
	      If  a  file  contains  N	raw  images, choose one or "all" to decode.  For example,
	      Fuji Super CCD SR cameras generate a second image underexposed four stops  to  show
	      detail in the highlights.

       ./.badpixels, ../.badpixels, ../../.badpixels, ...
	      List of your camera's dead pixels, so that dcraw can interpolate around them.  Each
	      line specifies the column, row, and UNIX time of death for one pixel.  For example:

	       962   91 1028350000  # died between August 1 and 4, 2002
	      1285 1067 0	    # don't know when this pixel died

	      These coordinates are before any cropping or rotation, so use  dcraw  -j	-t  0  to
	      locate dead pixels.

       pgm(5),	ppm(5),  pam(5),  pnmgamma(1),	pnmtotiff(1),  pnmtopng(1), gphoto2(1), cjpeg(1),

       Written by David Coffin, dcoffin a cybercom o net

					November 28, 2007				 dcraw(1)

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