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. |
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. |
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. |
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" |