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!!
-I Read the raw pixels from standard input in CPU byte order with no header. Use
dcraw -E -4 to get the raw pixel values.
Read the dead pixel list from this file instead of ".badpixels". See FILES for a
description of the format.
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.
When shadows appear foggy, you need to raise the darkness level. To measure this,
apply pamsumm -mean to the dark frame generated above.
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 | pam-
The default darkness and saturation are usually correct.
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
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
-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).
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 with the original unscaled pixel values.
-E Same as -D, but masked pixels are not cropped.
-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.
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.
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.
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), pamsumm(1), pnmgamma(1), pnmtotiff(1), pnmtopng(1), gphoto2(1),
Written by David Coffin, dcoffin a cybercom o net
May 14, 2009 dcraw(1)