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Comparing ray/doc/man/man1/pvalue.1 (file contents):
Revision 1.8 by greg, Thu Dec 16 21:34:41 2010 UTC vs.
Revision 1.12 by greg, Fri Feb 4 20:11:48 2022 UTC

# Line 42 | Line 42 | these files.
42   .TP 10n
43   .BR \-u
44   Print only unique values in the output, skipping runs of equal pixels.
45 + For reverse conversions, the
46 + .I \-u
47 + option writes uncompressed output rather than the standard run-length RGBE
48 + encoding.
49   Specifying
50   .I \+u
51   turns this option off, which is the default.
# Line 49 | Line 53 | turns this option off, which is the default.
53   .BR \-o
54   Print original values, before exposure compensation.
55   If the input file is in XYZE format, the Y (green) channel
56 < will correspond to units of candelas/meter^2.
57 < Otherwise, the RGB values should be in spectral watts/steradian/meter^2.
56 > will correspond to units of candelas/meter^2, unless
57 > .I \-O
58 > is specified, when watts/sr/meter^2 are always reported.
59   Specifying
60   .I \+o
61   uses final exposed values, which is the default.
# Line 76 | Line 81 | causes the resolution string to be printed, which is t
81   Skip the specified number of bytes on the input header.
82   This option is useful for skipping unintelligible headers in
83   foreign file formats.
79 (Does not work when reading from standard input.)
84   .TP
85   .BI \-e \ exposure
86   Adjust the exposure by the amount specified.
# Line 239 | Line 243 | pflip \-v flipped.hdr > final.hdr
243   .SH AUTHOR
244   Greg Ward
245   .SH BUGS
246 < The
243 < .I \-r
244 < option does not work with the
245 < .I \-u
246 < option.
247 < Also, input pixel locations are ignored during a reverse
246 > Input pixel locations are ignored during a reverse
247   conversion, so this information is not used in determining
248   the scanline ordering or picture size.
249   .SH "SEE ALSO"

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