# dcraw

Section: User Commands (1)
Updated: May 14, 2009
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## NAME

dcraw - command-line decoder for raw digital photos

## SYNOPSIS

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

## DESCRIPTION

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

## GENERAL OPTIONS

-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!!

## REPAIR OPTIONS

-P deadpixels.txt
  Read the dead pixel list from this file instead of ".badpixels". See FILES for a description of the format.
-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.
-k darkness
  When shadows appear foggy, you need to raise the darkness level. To measure this, apply pamsumm -mean to the dark frame generated above.
-S saturation
  When highlights appear pink, you need to lower the saturation level. To measure this, take a picture of something shiny and do dcraw -D -4 -j -c photo.raw | pamsumm -max
  The default darkness and saturation are usually correct.
-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.

## COLOR OPTIONS

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 warning 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 cameras.
-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 colorspace (sRGB by default).
-p embed
  Use the ICC profile embedded in the raw photo.

## INTERPOLATION OPTIONS

-d
  Show the raw data as a grayscale image with no interpolation. Good for photographing 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.

## OUTPUT OPTIONS

By default, dcraw writes PGM/PPM/PAM with 8-bit samples, a BT.709 gamma curve, a histogram-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.
-g power toe_slope
  Set the gamma curve, by default BT.709 (-g 2.222 4.5). If you prefer sRGB gamma, use -g 2.4 12.92. For a simple power curve, set the toe slope to zero.
-6
  Write sixteen bits per sample instead of eight.
-4
  Linear 16-bit, same as -6 -W -g 1 1.
-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.

## FILES

:./.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.

## SEE ALSO

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

## AUTHOR

Written by David Coffin, dcoffin a cybercom o net

## Index

NAME
SYNOPSIS
DESCRIPTION
GENERAL OPTIONS
REPAIR OPTIONS
COLOR OPTIONS
INTERPOLATION OPTIONS
OUTPUT OPTIONS
FILES
SEE ALSO
AUTHOR

This document was created by man2html, using the manual pages.
Time: 21:25:23 GMT, July 04, 2009