From c0b89ac5bfb90835ef01573267020e42d4fe070c Mon Sep 17 00:00:00 2001 From: =?UTF-8?q?J=C3=B6rg=20Frings-F=C3=BCrst?= Date: Sun, 23 Aug 2015 12:17:05 +0200 Subject: Imported Upstream version 1.8.0 --- doc/3dformat.html | 5 +- doc/ArgyllCMS_arts_tag.html | 0 doc/ArgyllDoc.html | 556 ++++++++++++++++++++- doc/ArgyllFlow.jpg | Bin doc/ArgyllFlowThumb.jpg | Bin doc/CMP_DT_003.jpg | Bin doc/CMP_Digital_Target-4.jpg | Bin doc/CRTspectrum.jpg | Bin doc/ChangesSummary.html | 44 ++ doc/Chroma4.jpg | Bin doc/ColorHug.jpg | Bin doc/ColorManagement.html | 0 doc/ColorMunki.jpg | Bin doc/ColorMunkiCreate.jpg | Bin doc/Compiling.html | 0 doc/CrushedDisplyBlacks.html | 0 doc/DC.jpg | Bin doc/DTP20.jpg | Bin doc/DTP22.jpg | Bin doc/DTP41.jpg | Bin doc/DTP51.jpg | Bin doc/DTP92.jpg | Bin doc/DTP94.jpg | Bin doc/DocLicense.txt | 0 doc/EX1.jpg | Bin 0 -> 24772 bytes doc/Environment.html | 11 + doc/FWA.html | 0 doc/FWA_measure.jpg | Bin doc/File_Formats.html | 2 +- doc/Fluorescent.jpg | Bin doc/HCFR.jpg | 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a/doc/3dformat.html +++ b/doc/3dformat.html @@ -30,7 +30,7 @@     Any web browser supporting javascript and WebGL can be used to display this.

- By default ArgyllCMS tools will output VRML format, but the defaul + By default ArgyllCMS tools will output X3DOM format, but the defaul can be overridden by setting the environment variable
"ARGYLL_3D_DISP_FORMAT" to "VRML", "X3D" or "X3DOM"

@@ -78,8 +78,7 @@ Function Key - - + Reset view r diff --git a/doc/ArgyllCMS_arts_tag.html b/doc/ArgyllCMS_arts_tag.html old mode 100644 new mode 100755 diff --git a/doc/ArgyllDoc.html b/doc/ArgyllDoc.html old mode 100644 new mode 100755 index f7a0141..5f617e0 --- a/doc/ArgyllDoc.html +++ b/doc/ArgyllDoc.html @@ -10,9 +10,9 @@ Argyll Documentation Top -

Argyll CMS documentation index (V1.7.0)
+

Argyll CMS documentation index (V1.8.0)

- Date:   1st May 2015
+ Date:   20th August 2015
Author: Graeme Gill

Introduction

ArgyllCMS is an ICC compatible color management system, available as @@ -34,7 +34,7 @@ provided for each major tool, and a general guide to using the tools for typical color management tasks is also available. A mailing list provides support for more advanced usage.
-

This is Version 1.7.0, a feature and bug fix update to V1.6.3. +

This is Version 1.8.0, a feature and bug fix update to V1.7.0. The first public release of icclib was in November 1998, and of Argyll was in October 2000. Code development commenced in 1995. See Changes Summary for an @@ -47,10 +47,10 @@

Please note that instruments are being driven by ArgyllCMS drivers, and that any problems or queries regarding instrument
- operation should be - directed to the Argyll's author(s) or the Argyll mailing list, - and not to any other - party.

+ operation should + first be directed to the Argyll's author(s) or the Argyll + mailing list, and not to any other party.

An Introduction to Color Management

@@ -93,6 +93,10 @@ + + + + @@ -169,6 +173,64 @@ + + + + + + + + + + + + + + + + + + + + + + + + + + - Tele-Spectro-Radiometer
+
+ Image Engineering:
+
+     EX1                                               + + + + + + + + + + + + + + + + + + + + + + + + + + + + @@ -211,6 +273,10 @@ + + + + @@ -306,6 +372,10 @@ + + + + @@ -395,6 +465,10 @@ + + + + @@ -483,6 +557,10 @@ + + + + @@ -573,6 +651,10 @@ + + + + @@ -661,6 +743,10 @@ + + + + @@ -749,6 +835,10 @@ + + + + @@ -898,6 +988,10 @@ + + + + @@ -987,6 +1081,10 @@ + + + + @@ -1085,6 +1183,10 @@ + + + + @@ -1175,6 +1277,10 @@ + + + + @@ -1270,6 +1376,10 @@ + + + + @@ -1297,7 +1407,11 @@
Other:
    Colorimètre HCFR                          + href="instruments.html#HCFR">Colorimètre HCFR                         + + + + @@ -1451,6 +1565,10 @@ + + + + @@ -1458,6 +1576,10 @@ - display colorimeter
+     SwatchMate + Cube                         + + - reflective colorimeter

See Operation of particular instruments for more instrument specific detail.
@@ -1510,6 +1632,10 @@ + + + + GNU license prohibits extending these tools @@ -1647,6 +1773,10 @@ + + + + @@ -1733,6 +1863,10 @@ + + + + @@ -1902,6 +2036,10 @@ calibration + + + + @@ -1998,6 +2136,10 @@ href="http://www.google.com/search?hl=en&source=hp&q=argyllcms+GUI&a + + + + @@ -2101,6 +2243,10 @@ href="http://www.google.com/search?hl=en&source=hp&q=argyllcms+GUI&a + + + + @@ -2190,6 +2336,10 @@ href="http://www.google.com/search?hl=en&source=hp&q=argyllcms+GUI&a + + + + @@ -2279,6 +2429,10 @@ href="http://www.google.com/search?hl=en&source=hp&q=argyllcms+GUI&a + + + + @@ -2371,6 +2525,10 @@ href="http://www.google.com/search?hl=en&source=hp&q=argyllcms+GUI&a + + + + @@ -2460,6 +2618,10 @@ href="http://www.google.com/search?hl=en&source=hp&q=argyllcms+GUI&a + + + + @@ -2558,7 +2720,7 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> converting color spaces of raster files.

Although it is is a couple of years old now, this tutorial + href="http://www.argyllcms.com/doc2/FCMS2010_ArgyllTute.pdf">tutorial may also be of interest.
 

Topical @@ -2700,6 +2862,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -2790,6 +2956,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -2880,6 +3050,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -2972,6 +3146,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -3063,6 +3241,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -3153,6 +3335,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -3243,6 +3429,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -3338,6 +3528,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -3432,6 +3626,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -3523,6 +3721,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -3613,6 +3815,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -3642,6 +3848,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -3732,6 +3942,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -3757,6 +3971,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + or Merge two or more measurement data files, or average patches within a single file.
@@ -3843,6 +4061,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -3932,6 +4154,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -4022,6 +4248,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -4113,6 +4343,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -4205,6 +4439,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -4295,6 +4533,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -4384,6 +4626,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -4474,6 +4720,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -4564,6 +4814,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -4654,6 +4908,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -4752,6 +5010,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -4841,6 +5103,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -4931,6 +5197,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -5023,6 +5293,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -5112,6 +5386,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -5201,6 +5479,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -5289,6 +5571,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -5382,6 +5668,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -5470,6 +5760,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -5502,6 +5796,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -5591,6 +5889,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -5681,6 +5983,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -5773,6 +6079,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -5868,6 +6178,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -5964,6 +6278,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -6054,6 +6372,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -6146,6 +6468,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -6235,6 +6561,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -6325,6 +6655,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -6415,6 +6749,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -6504,6 +6842,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -6595,6 +6937,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -6684,6 +7030,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -6774,6 +7124,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -6864,6 +7218,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -6957,6 +7315,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -7047,6 +7409,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -7138,6 +7504,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -7232,6 +7602,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -7322,6 +7696,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -7411,6 +7789,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -7500,6 +7882,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -7589,6 +7975,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -7679,6 +8069,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -7768,6 +8162,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -7857,6 +8255,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -7946,6 +8348,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -8039,6 +8445,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -8130,6 +8540,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -8220,6 +8634,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -8309,6 +8727,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -8399,6 +8821,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -8493,6 +8919,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -8582,6 +9012,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -8672,6 +9106,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -8767,6 +9205,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -8857,6 +9299,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -8948,6 +9394,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -9039,6 +9489,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -9127,6 +9581,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -9216,6 +9674,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -9305,6 +9767,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -9395,6 +9861,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -9484,6 +9954,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -9574,6 +10048,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -9668,6 +10146,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -9759,6 +10241,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -9849,6 +10335,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -9966,6 +10456,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -10054,6 +10548,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -10142,6 +10640,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -10234,6 +10736,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -10323,6 +10829,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -10411,6 +10921,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -10507,6 +11021,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -10595,6 +11113,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -10683,6 +11205,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -10771,6 +11297,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -10859,6 +11389,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + @@ -10952,6 +11486,10 @@ href="http://www.google.com/search?hl=en&q=windows+command+prompt+tutorial"> + + + + diff --git a/doc/ArgyllFlow.jpg b/doc/ArgyllFlow.jpg old mode 100644 new mode 100755 diff --git a/doc/ArgyllFlowThumb.jpg b/doc/ArgyllFlowThumb.jpg old mode 100644 new mode 100755 diff --git a/doc/CMP_DT_003.jpg b/doc/CMP_DT_003.jpg old mode 100644 new mode 100755 diff --git a/doc/CMP_Digital_Target-4.jpg b/doc/CMP_Digital_Target-4.jpg old mode 100644 new mode 100755 diff --git a/doc/CRTspectrum.jpg b/doc/CRTspectrum.jpg old mode 100644 new mode 100755 diff --git a/doc/ChangesSummary.html b/doc/ChangesSummary.html old mode 100644 new mode 100755 index d0eee96..559f521 --- a/doc/ChangesSummary.html +++ b/doc/ChangesSummary.html @@ -16,6 +16,48 @@

Summary of Argyll CMS Changes since last release

For a complete and more detailed list of changes, please see the log.txt file.

+

[V1.7.0 -> V1.8.0] 20th August 2015

+
    +
  • Added support for the Image Engineering EX1 spectroradiometer.
    • +
  • Added support for the SwatchMate Cube reflective colorimeter, + with improved accuracy.
    • +
  • Added Added Television Lighting Consistency Index (EBU + TLCI-2012 Qa)  to spotread and specplot output.
    • +
  • Added R9 value to CRI value in spotread and specplot output.
    • +
  • Added support for "EMISINPUT" type .ti3 file.
    • +
  • Build using OpenSSL rather than axTLS if it is built on Linux.
    • +
  • Fixed stack space problem in OS X UI programs by expanding + main thread proxy to have 8MB instead of the default 512K.
    • +
  • Updated built in libtiff to V4.0.4beta.
    • +
  • Changed CGATS format to not emit unknown keyword declaration + ("KEYWORD") by default.
    • +
  • Added inst_calc_cond_mask to inst.h to allow for flags in + calibration conditions. A consequence of this is that calc needs + to be masked with this when comparing against a specific + condition, and the inst_calc_optional_flag should be cleared if + it is set, before callint inst->calibrate() if the user wants + to proceed with a particular calibration.
    • +
  • Fixed bug with dispcal -e N
    • +
  • Fixed bug in xicclu -fg and -kp
    • +
  • Added dispcal -x x option to allow reading a chart and + manually entering the XYZ values.
    • +
  • Fix spyder4 & 5 bug where some display types were set as + refresh when they shouldn't be.
    • +
  • Fix collink "Warning :- RGB black hack trigger more than + once!" when -b is used with input video encoding (-e).
    • +
  • Changed colprof so that the default ICC description is the + base filename rather than the whole file path.
    • +
  • Fix technology type and display type selector + "uniqueification" bug  that shows up in "ccxxmake -??".
    • +
  • Add OEM field to ccmx and ccss files to mark files that have + been installed from OEM disk, so that custom ccmx & ccss + files can be given suggested selector letter priority (+ + ref/CRT.ccss).
    • +
  • Tweak CGATS write format to avoid scientific notation until + the numbers are bigger and smaller (i.e until e6 and e-6 are + needed).
    +
    • +

[V1.6.3 -> V1.7.0] 1st May 2015

  • Improved gamut mapping to reduce unnecessary changes to less @@ -922,6 +964,7 @@ + for systems with > 3Gig Ram.
    • @@ -958,6 +1001,7 @@ + and memory usage issues. diff --git a/doc/Chroma4.jpg b/doc/Chroma4.jpg old mode 100644 new mode 100755 diff --git a/doc/ColorHug.jpg b/doc/ColorHug.jpg old mode 100644 new mode 100755 diff --git a/doc/ColorManagement.html b/doc/ColorManagement.html old mode 100644 new mode 100755 diff --git a/doc/ColorMunki.jpg b/doc/ColorMunki.jpg old mode 100644 new mode 100755 diff --git a/doc/ColorMunkiCreate.jpg b/doc/ColorMunkiCreate.jpg old mode 100644 new mode 100755 diff --git a/doc/Compiling.html b/doc/Compiling.html old mode 100644 new mode 100755 diff --git a/doc/CrushedDisplyBlacks.html b/doc/CrushedDisplyBlacks.html old mode 100644 new mode 100755 diff --git a/doc/DC.jpg b/doc/DC.jpg old mode 100644 new mode 100755 diff --git a/doc/DTP20.jpg b/doc/DTP20.jpg old mode 100644 new mode 100755 diff --git a/doc/DTP22.jpg b/doc/DTP22.jpg old mode 100644 new mode 100755 diff --git a/doc/DTP41.jpg b/doc/DTP41.jpg old mode 100644 new mode 100755 diff --git a/doc/DTP51.jpg b/doc/DTP51.jpg old mode 100644 new mode 100755 diff --git a/doc/DTP92.jpg b/doc/DTP92.jpg old mode 100644 new mode 100755 diff --git a/doc/DTP94.jpg b/doc/DTP94.jpg old mode 100644 new mode 100755 diff --git a/doc/DocLicense.txt b/doc/DocLicense.txt old mode 100644 new mode 100755 diff --git a/doc/EX1.jpg b/doc/EX1.jpg new file mode 100755 index 0000000..0192ba8 Binary files /dev/null and b/doc/EX1.jpg differ diff --git a/doc/Environment.html b/doc/Environment.html old mode 100644 new mode 100755 index d02bf6c..b4cd9ca --- a/doc/Environment.html +++ b/doc/Environment.html @@ -41,6 +41,12 @@     Note that while a reading is being made, a character input can abort the reading, just as with normal interactive mode.
    +
    +     Note that on MSWin systems, the character and + return or line fee characters must be written to stdin in a single + operation (i.e. testing ARGYLL_NOT_INTERACTIVE  + mode manually will probably fail, because the character and + return get split up.)

    ARGYLL_3D_DISP_FORMAT
    @@ -51,11 +57,13 @@ +     or X3DOM, which will result in .wrl, .x3d and .x3d.html files respectively. See 3d + Viewing Format.

    @@ -88,6 +96,7 @@ a + delay of 200 msec is allowed between changing a patch color in software, and that change appearing in the displayed color itself. For some instuments (ie. i1d3, i1pro, ColorMunki, Klein K10-A) @@ -106,6 +115,7 @@ environment + variable, ie. ARGYLL_MIN_DISPLAY_UPDATE_DELAY_MS=400 would set a 400 msec minimum delay.

    @@ -246,6 +256,7 @@ Base + Directory Specification, and uses the XDG_CACHE_HOME environment variable to place per instrument calibration information, and diff --git a/doc/FWA.html b/doc/FWA.html old mode 100644 new mode 100755 diff --git a/doc/FWA_measure.jpg b/doc/FWA_measure.jpg old mode 100644 new mode 100755 diff --git a/doc/File_Formats.html b/doc/File_Formats.html old mode 100644 new mode 100755 index 1741701..70a196a --- a/doc/File_Formats.html +++ b/doc/File_Formats.html @@ -117,7 +117,7 @@ href="File_Formats.html#CGATS">CGATS, Argyll specific format, used to hold a set of display spectral samples. For Colorimeters that have known sensor spectral sensitivity information (such as the - i1d3 and Spyder4), this allows a calibration to be created that is + i1d3 and Spyder4 & Spyder5), this allows a calibration to be created that is tuned for a particular display. The file contains a description of the display, the display technology type, the type of spectrometer used for taking the readings. See oeminst diff --git a/doc/Fluorescent.jpg b/doc/Fluorescent.jpg old mode 100644 new mode 100755 diff --git a/doc/HCFR.jpg b/doc/HCFR.jpg old mode 100644 new mode 100755 diff --git a/doc/HCT.jpg b/doc/HCT.jpg old mode 100644 new mode 100755 diff --git a/doc/HiResLaser.jpg b/doc/HiResLaser.jpg old mode 100644 new mode 100755 diff --git a/doc/Huey.jpg b/doc/Huey.jpg old mode 100644 new mode 100755 diff --git a/doc/Installing.html b/doc/Installing.html old mode 100644 new mode 100755 diff --git a/doc/Installing_Linux.html b/doc/Installing_Linux.html old mode 100644 new mode 100755 diff --git a/doc/Installing_MSWindows.html b/doc/Installing_MSWindows.html old mode 100644 new mode 100755 index 40dcd2c..bb610cd --- a/doc/Installing_MSWindows.html +++ b/doc/Installing_MSWindows.html @@ -61,9 +61,9 @@
     So if the current value of PATH is "%SystemRoot%\system32;%SystemRoot%" and you unpacked Argyll version - 1.7.0 in d:\bin\, then you + 1.8.0 in d:\bin\, then you would modify PATH to be - "%SystemRoot%\system32;%SystemRoot%;d:\bin\Argyll_V1.7.0\bin", - + "%SystemRoot%\system32;%SystemRoot%;d:\bin\Argyll_V1.8.0\bin", - i.e. you append the path to the Argyll binaries to your PATH, separated by the ';' character. The change will take effect when you start a new command shell, which you start from Start diff --git a/doc/Installing_OSX.html b/doc/Installing_OSX.html old mode 100644 new mode 100755 diff --git a/doc/JETI_1211.jpg b/doc/JETI_1211.jpg old mode 100644 new mode 100755 diff --git a/doc/K10A.jpg b/doc/K10A.jpg old mode 100644 new mode 100755 diff --git a/doc/Kgraph1.jpg b/doc/Kgraph1.jpg old mode 100644 new mode 100755 diff --git a/doc/Kgraph2.jpg b/doc/Kgraph2.jpg old mode 100644 new mode 100755 diff --git a/doc/Kgraph3.jpg b/doc/Kgraph3.jpg old mode 100644 new mode 100755 diff --git a/doc/Kgraph4.jpg b/doc/Kgraph4.jpg old mode 100644 new mode 100755 diff --git a/doc/Kgraph5.jpg b/doc/Kgraph5.jpg old mode 100644 new mode 100755 diff --git a/doc/Kgraph6.jpg b/doc/Kgraph6.jpg old mode 100644 new mode 100755 diff --git a/doc/Kgraph7.jpg b/doc/Kgraph7.jpg old mode 100644 new mode 100755 diff --git a/doc/Kgraph8.jpg b/doc/Kgraph8.jpg old mode 100644 new mode 100755 diff --git a/doc/Kparams.jpg b/doc/Kparams.jpg old mode 100644 new mode 100755 diff --git a/doc/LSDC.jpg b/doc/LSDC.jpg old mode 100644 new mode 100755 diff --git a/doc/LabSteps.jpg b/doc/LabSteps.jpg old mode 100644 new mode 100755 diff --git a/doc/License.txt b/doc/License.txt old mode 100644 new mode 100755 diff --git a/doc/License2.txt b/doc/License2.txt old mode 100644 new mode 100755 diff --git a/doc/License3.txt b/doc/License3.txt old mode 100644 new mode 100755 diff --git a/doc/Limitations.html b/doc/Limitations.html old mode 100644 new mode 100755 diff --git a/doc/MinorTools.html b/doc/MinorTools.html old mode 100644 new mode 100755 diff --git a/doc/Organisation.html b/doc/Organisation.html old mode 100644 new mode 100755 diff --git a/doc/Overview.html b/doc/Overview.html old mode 100644 new mode 100755 diff --git a/doc/Performance.html b/doc/Performance.html old mode 100644 new mode 100755 diff --git a/doc/Q60.jpg b/doc/Q60.jpg old mode 100644 new mode 100755 diff --git a/doc/QPcard201.jpg b/doc/QPcard201.jpg old mode 100644 new mode 100755 diff --git a/doc/QPcard202.jpg b/doc/QPcard202.jpg old mode 100644 new mode 100755 diff --git a/doc/SG.jpg b/doc/SG.jpg old mode 100644 new mode 100755 diff --git a/doc/SG_footer.txt b/doc/SG_footer.txt old mode 100644 new mode 100755 diff --git a/doc/SG_header.txt b/doc/SG_header.txt old mode 100644 new mode 100755 diff --git a/doc/SMCube.jpg b/doc/SMCube.jpg new file mode 100755 index 0000000..e38d23a Binary files /dev/null and b/doc/SMCube.jpg differ diff --git a/doc/Scenarios.html b/doc/Scenarios.html old mode 100644 new mode 100755 index 7b5899f..8cd45c9 --- a/doc/Scenarios.html +++ b/doc/Scenarios.html @@ -178,6 +178,7 @@ + @@ -256,6 +257,7 @@ + @@ -638,6 +640,7 @@ + @@ -708,6 +711,7 @@ + @@ -876,6 +880,7 @@ + @@ -944,6 +949,7 @@ + @@ -1017,6 +1023,7 @@ + @@ -1081,6 +1088,7 @@ + @@ -1133,6 +1141,7 @@ href="http://www.qpcard.com/en_b2c/color-reference-cards/instant-camera-raw-prof + @@ -1193,7 +1202,7 @@ href="http://www.qpcard.com/en_b2c/color-reference-cards/instant-camera-raw-prof create your own reference file using an instrument and chartread, making use of the chart reference file ref/ColorChecker.ti2:
    -    chartread -n -a +    chartread -n ColorChecker.ti2
    Note that due to the small number of patches, a profile created from such a chart is not likely to be very detailed.
    @@ -1269,6 +1278,7 @@ href="http://www.xrite.com/documents/apps/public/digital_colorchecker_sg_l_a_b.t + @@ -1298,7 +1308,7 @@ href="http://www.xrite.com/documents/apps/public/digital_colorchecker_sg_l_a_b.t instrument (usually the Eye-One Pro). This can be done using chartread,  making use of the chart reference file ref/i1_RGB_Scan_1.4.ti2:
    -     chartread -n -a +     chartread -n i1_RGB_Scan_1.4
    and then rename the resulting i1_RGB_Scan_1.4.ti3 file to i1_RGB_Scan_1.4.cie
    @@ -1401,6 +1411,7 @@ href="http://www.xrite.com/documents/apps/public/digital_colorchecker_sg_l_a_b.t + @@ -1854,6 +1865,7 @@ href="http://www.xrite.com/documents/apps/public/digital_colorchecker_sg_l_a_b.t + @@ -2003,6 +2015,7 @@ then + @@ -2135,6 +2148,7 @@ then + @@ -2600,6 +2614,7 @@ chart, + @@ -2666,6 +2681,7 @@ an + @@ -2724,6 +2740,7 @@ an + @@ -2790,6 +2807,7 @@ a + @@ -3134,6 +3152,7 @@ a MadVR rather than Argyll, start madTPG and then use the option "-d + madvr" in dispcal, dispread and dispwin. Leave the MadTPG "VideoLUT" and "3dluts" buttons in their default  (enabled) @@ -3195,6 +3214,7 @@ a + interactive adjustment mode can be used to set the white point. Note that while adjusting the neutral axis for neutrality may @@ -3228,6 +3248,7 @@ a + of where to apply display per channel calibration curves.
  • Choose one of the Absolute Colorimetric intents in collink @@ -3718,6 +3739,7 @@ a + @@ -3743,6 +3765,7 @@ a + @@ -3775,6 +3798,7 @@ a + @@ -3800,6 +3824,7 @@ a + diff --git a/doc/Smile.jpg b/doc/Smile.jpg old mode 100644 new mode 100755 diff --git a/doc/Source.html b/doc/Source.html old mode 100644 new mode 100755 diff --git a/doc/Spyd2.jpg b/doc/Spyd2.jpg old mode 100644 new mode 100755 diff --git a/doc/Spyd3.jpg b/doc/Spyd3.jpg old mode 100644 new mode 100755 diff --git a/doc/Spyd3x.jpg b/doc/Spyd3x.jpg old mode 100644 new mode 100755 diff --git a/doc/Spyd4.jpg b/doc/Spyd4.jpg old mode 100644 new mode 100755 diff --git a/doc/Spyd5.jpg b/doc/Spyd5.jpg new file mode 100755 index 0000000..86b4be2 Binary files /dev/null and b/doc/Spyd5.jpg differ diff --git a/doc/SpyderChecker.jpg b/doc/SpyderChecker.jpg old mode 100644 new mode 100755 diff --git a/doc/VideoEOTFs.html b/doc/VideoEOTFs.html old mode 100644 new mode 100755 diff --git a/doc/WideGamutColmters.html b/doc/WideGamutColmters.html old mode 100644 new mode 100755 diff --git a/doc/YellowGreen.jpg b/doc/YellowGreen.jpg old mode 100644 new mode 100755 diff --git a/doc/afiles b/doc/afiles old mode 100644 new mode 100755 index db6632f..88f7406 --- a/doc/afiles +++ b/doc/afiles @@ -39,6 +39,7 @@ Spyd2.jpg Spyd3.jpg Spyd3x.jpg Spyd4.jpg +Spyd5.jpg i1d.jpg i1d3_1.jpg i1d3_2.jpg @@ -48,6 +49,8 @@ sl.jpg ss.jpg JETI_1211.jpg ColorHug.jpg +EX1.jpg +SMCube.jpg mox.jpg moxxr.jpg Chroma4.jpg diff --git a/doc/applycal.html b/doc/applycal.html old mode 100644 new mode 100755 diff --git a/doc/average.html b/doc/average.html old mode 100644 new mode 100755 diff --git a/doc/cal_format.html b/doc/cal_format.html old mode 100644 new mode 100755 diff --git a/doc/calvschar.html b/doc/calvschar.html old mode 100644 new mode 100755 diff --git a/doc/cb2ti3.html b/doc/cb2ti3.html old mode 100644 new mode 100755 diff --git a/doc/ccmxs.html b/doc/ccmxs.html old mode 100644 new mode 100755 diff --git a/doc/ccmxs/DTP-94_1964_10_Dell_2408W.ccmx b/doc/ccmxs/DTP-94_1964_10_Dell_2408W.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/DTP-94_1997_Shaw_Dell_2408W.ccmx b/doc/ccmxs/DTP-94_1997_Shaw_Dell_2408W.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/DTP-94_Dell_2408W.ccmx b/doc/ccmxs/DTP-94_Dell_2408W.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/DTP-94_Dell_U2410.ccmx b/doc/ccmxs/DTP-94_Dell_U2410.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/EyeOne_Display_1_NEC1990SXi.ccmx b/doc/ccmxs/EyeOne_Display_1_NEC1990SXi.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/EyeOne_Display_2_EIZO_S2233W.ccmx b/doc/ccmxs/EyeOne_Display_2_EIZO_S2233W.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/EyeOne_Display_2_NEC1990SXi.ccmx b/doc/ccmxs/EyeOne_Display_2_NEC1990SXi.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/EyeOne_Display_LT_U2410_Standard_1931.ccmx b/doc/ccmxs/EyeOne_Display_LT_U2410_Standard_1931.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/EyeOne_Display_LT_U2410_Standard_1964.ccmx b/doc/ccmxs/EyeOne_Display_LT_U2410_Standard_1964.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/EyeOne_Display_LT_U2410_sRGB_1931.ccmx b/doc/ccmxs/EyeOne_Display_LT_U2410_sRGB_1931.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/EyeOne_Display_LT_U2410_sRGB_1964.ccmx b/doc/ccmxs/EyeOne_Display_LT_U2410_sRGB_1964.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/Huey_Acer_al2016w.ccmx b/doc/ccmxs/Huey_Acer_al2016w.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/Huey_Eizo_CG243.ccmx b/doc/ccmxs/Huey_Eizo_CG243.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/Huey_HP_compaq_6730s.ccmx b/doc/ccmxs/Huey_HP_compaq_6730s.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/Huey_HP_lp2475w.ccmx b/doc/ccmxs/Huey_HP_lp2475w.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/Huey_NEC1990SXi.ccmx b/doc/ccmxs/Huey_NEC1990SXi.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/Huey_NEC_Spectraview_241.ccmx b/doc/ccmxs/Huey_NEC_Spectraview_241.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/NEC_EyeOne_Display_2_NEC2690WUXi2.ccmx b/doc/ccmxs/NEC_EyeOne_Display_2_NEC2690WUXi2.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/Spyder2_EIZO_S2433W_standard_1931.ccmx b/doc/ccmxs/Spyder2_EIZO_S2433W_standard_1931.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/Spyder2_EIZO_S2433W_standard_1964.ccmx b/doc/ccmxs/Spyder2_EIZO_S2433W_standard_1964.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/Spyder3_EIZO_S2233_standard_1964.ccmx b/doc/ccmxs/Spyder3_EIZO_S2233_standard_1964.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/Spyder3_EIZO_S2243W_standard_1931.ccmx b/doc/ccmxs/Spyder3_EIZO_S2243W_standard_1931.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/Spyder3_HP_LP2475w.ccmx b/doc/ccmxs/Spyder3_HP_LP2475w.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/Spyder3_NEC2690WUXi2.ccmx b/doc/ccmxs/Spyder3_NEC2690WUXi2.ccmx old mode 100644 new mode 100755 diff --git a/doc/ccmxs/Spyder3_NEC_PA301W.ccmx b/doc/ccmxs/Spyder3_NEC_PA301W.ccmx old mode 100644 new mode 100755 diff --git a/doc/cctiff.html b/doc/cctiff.html old mode 100644 new mode 100755 index c19d5c5..5a9ca82 --- a/doc/cctiff.html +++ b/doc/cctiff.html @@ -3,7 +3,7 @@ cctiff + charset=windows-1252"> @@ -22,6 +22,7 @@ style="font-style: italic;">profile.icm | [-d dir] calibration.cal ...} infile.tif + outfile.tif
    @@ -33,12 +34,14 @@ style="font-family: monospace;">                +    Verbose
     -c                +    Combine linearisation curves into one transform
                     +    Use slow precise floating point conversion, rather than fast integer routines.
    @@ -54,6 +58,7 @@ style="font-family: monospace;">                +    Check fast result against precise, and report differences.
       -f [T|J]             + Set output format to Tiff or Jpeg (Default is same as input)
     -q quality           + Set JPEG quality 1..100 (Default 80)
     -a-I                   Ignore + any file or profile colorspace mismatches
     -D                   Don't + append or set the output TIFF description
    +  -N                   + Output uncompressed TIFF (default LZW)


    @@ -100,12 +111,14 @@ Don't TIFF or JPEG file.
                              +     This may be an ICC file or TIFF or JPEG file with embedded profile.

                          Then + for each profile in the linked sequence:
                        +     s = saturation, a = absolute colorimetric
      -o order
    @@ -143,10 +158,12 @@ r                         (May + be embedded profile in TIFF or JPEG file)
                          or + each calibration file in sequence:
           + A calibration file.
             A TIFF - or JPEG Raster file that - will be the input raster to be transformed.
    or JPEG + Raster file that will be the input raster to be transformed.
     outfile.tifThe -D flag stops the description tag being set or appended to by cctiff.

    + By default any TIFF output file will be LZW + compressed, but the -N flag + will cause any TIFF file to be saved uncompressed.
    +
    The -e profile.[icm | tiff | jpg] option allows an ICC profile to be embedded in the destination TIFF or JPEG diff --git a/doc/ccxxmake.html b/doc/ccxxmake.html old mode 100644 new mode 100755 index f83afc8..a2a9080 --- a/doc/ccxxmake.html +++ b/doc/ccxxmake.html @@ -32,9 +32,10 @@ information built into them  (ie. the X-Rite i1d3, and - DataColor Spyder4), ccxxmake allows a creation of a - calibration spectral sample (ccss) + DataColor Spyder4 & Spyder5), + + ccxxmake allows a creation + of a calibration spectral sample (ccss) for a particular Display, by making use a reference Spectrometer instrument. This can then be used to improve the accuracy of @@ -73,6 +74,8 @@ + +       Verbose mode
      -S                                         Create @@ -96,8 +99,10 @@ rather + + than CCMX
    -   -f file1.ti3[,file2.ti3] +   -f ref.ti3[,targ.ti3]                Create from @@ -122,6 +127,8 @@ two + + .ti3 files rather than measure.
     -display @@ -143,6 +150,8 @@ two + + displayname  [X11 only] Choose X11 display name

     -d @@ -197,6 +208,8 @@ m + + n                  Choose the @@ -223,6 +236,8 @@ list + + (default 1)
     -dweb[:port]          @@ -244,6 +259,8 @@ list + + @@ -262,10 +279,14 @@ list + + [MSWin] Display via MadVR Video Renderer
     -dcc[:n]              + + Display via n'th ChromeCast (default 1, ? for list)
     
      -y X @@ -311,11 +334,17 @@ list + + Display type - instrument specific list to choose from. (CCMX)
     -z disptype           + + Different display type for spectrometer (see -y)
      -P ho,vo,ss[,vs]      + + Position test window and scale it
                           @@ -344,6 +373,8 @@ center, + + 1.0 = right/bottom etc.
                           ss: @@ -371,6 +402,8 @@ normal, + + 2.0 = double etc.
                           @@ -385,6 +418,8 @@ normal, + + ss,vs: = optional horizontal, vertical scale.
     
       -N                    @@ -459,6 +498,8 @@ on + + Disable initial calibration of instrument if possible
     
    @@ -504,6 +547,8 @@ on + + "command"          Invoke shell "command" each time a color is set
     -o @@ -539,6 +584,8 @@ sequence + + combination steps (default 3)
         -W @@ -560,6 +607,8 @@ sequence + + n|h|x              Override serial @@ -586,6 +635,8 @@ n + + none, h = HW, x = Xon/Xoff
     -D [level] @@ -615,6 +666,8 @@ overall + + description
     -I "displayname"      -t + + dtech              Set display technology type
    @@ -631,26 +686,36 @@ overall c                   + + CRT
        m                   + + Plasma
        l                   + + LCD
        1                   + + LCD CCFL
        2               + +         LCD CCFL IPS
    @@ -658,6 +723,8 @@ overall 3               + +         LCD CCFL VPA
    @@ -665,6 +732,8 @@ overall 4               + +         LCD CCFL TFT
    @@ -672,6 +741,8 @@ overall L               + +         LCD CCFL Wide Gamut
    @@ -679,6 +750,8 @@ overall 5               + +         LCD CCFL Wide Gamut IPS
    @@ -686,6 +759,8 @@ overall 6               + +         LCD CCFL Wide Gamut VPA
    @@ -693,6 +768,8 @@ overall 7               + +         LCD CCFL Wide Gamut TFT
    @@ -700,6 +777,8 @@ overall e               + +         LCD White LED
    @@ -707,6 +786,8 @@ overall 8               + +         LCD White LED IPS
    @@ -714,6 +795,8 @@ overall 9               + +         LCD White LED VPA
    @@ -721,6 +804,8 @@ overall a               + +         LCD White LED TFT
    @@ -728,6 +813,8 @@ overall b               + +         LCD RGB LED
    @@ -735,6 +822,8 @@ overall b               + +         LCD RGB LED IPS
    @@ -742,6 +831,8 @@ overall c               + +         LCD RGB LED VPA
    @@ -749,6 +840,8 @@ overall d               + +         LCD RGB LED TFT
    @@ -756,6 +849,8 @@ overall h               + +         LCD RG Phosphor
    @@ -763,6 +858,8 @@ overall e               + +         LCD RG Phosphor IPS
    @@ -770,6 +867,8 @@ overall f               + +         LCD RG Phosphor VPA
    @@ -777,6 +876,8 @@ overall g               + +         LCD RG Phosphor TFT
    @@ -784,6 +885,8 @@ overall o               + +         LED OLED
    @@ -791,6 +894,8 @@ overall a               + +         LED AMOLED
    @@ -798,6 +903,8 @@ overall p               + +         DLP Projector
    @@ -805,6 +912,8 @@ overall h               + +         DLP Projector RGB Filter Wheel
    @@ -812,6 +921,8 @@ overall i               + +         DPL Projector RGBW Filter Wheel
    @@ -819,6 +930,8 @@ overall j               + +         DLP Projector RGBCMY Filter Wheel
    @@ -826,6 +939,8 @@ overall u               + +         Unknown
      -U c                  @@ -835,6 +950,8 @@ overall + + Set UI selection character(s)
     -Y @@ -853,12 +970,16 @@ overall + +      Override refresh, non-refresh display mode
         -Y R:rate             + + Override measured refresh rate with rate Hz
     -YA
    -f file1.ti3[,file2.ti3] - By default ref.ti3[,targ.ti3]     By + default ccxxmake creates a CCMX file by displaying test patches on the screen, and then prompting you to measure them @@ -964,6 +1085,8 @@ overall + + 1,2 . Some experimentation may be needed using dispwin on such systems, to discover what screen has access to the VideoLUT hardware, and which screens the @@ -990,10 +1113,11 @@ overall
    -dmadvr [MSWin only] causes test patches to be displayed using the MadVR - video renderer. Note that you may have to start the video playback - software and load a video clip in pause for this to work. MadVR - rendering does not need or support VideoLUT access. Test patch - colors will be processed by the MadVR 3dLut.
    + video renderer. Note that will have to start MadTPG before + running ccxxmake, and that while you can adjust the "Test Pattern + Configuration" controls, you should not normally alter the + "Existing Calibration" controls, as ccxxmake will set these + appropriately.

    -dcc or -dcc:no causes test patches to be displayed using and available for more details. This may give better accuracy for display measurements.

    @@ -1213,6 +1339,8 @@ overall + + -Y n options overrides the refresh display mode set by the     -y display type selection, with -Y r forcing refresh display mode, diff --git a/doc/chartread.html b/doc/chartread.html old mode 100644 new mode 100755 index 18d0144..4d5b005 --- a/doc/chartread.html +++ b/doc/chartread.html @@ -3,7 +3,7 @@ chartread + charset=windows-1252"> @@ -26,6 +26,7 @@ Verbose + mode
     -c listno      -d
    @@ -58,6 +61,7 @@ measurement               + Display type - instrument specific list to choose from.
     -e  -p
      -x [lx]            Take -external -values, - - - either L*a*b* (-xl) or XYZ (-xx).
    + manually entered + values, either L*a*b* (-xl) or XYZ (-xx).
     -n             @@ -96,6 +99,7 @@ values, Don't + save spectral information (default saves spectral)
     -l  -I file.cal        Override @@ -121,26 +126,31 @@ partly monospace;">-F filter          + Set filter configuration:
      n                  + None
      p                  + Polarising filter
      6                  + D65
      u                  + U.V. Cut
     
         -X file.ccss          @@ -176,6 +187,7 @@ Samples + for calibration
     -Q observ1931_2 (def.)      -S                 @@ -209,12 +223,14 @@ wrong strip + & unexpected value warnings
     -W n|h|x           Override + serial port flow control: n = none, h = HW, x = Xon/Xoff
             +  Base name for input[.ti2]/output[
    The -x - flag causes chartread to expect values to be entered for each - reading, rather than using an instrument to do the + flag causes chartread to expect values to be manually entered for + each reading, rather than using an instrument to do the measurements.  This mode is ideal if your instrument is not supported by Argyll. Either XYZ or L*a*b* values can be entered, depending on what option follows chartread + -I parameter allows overriding the .ti2 calibration curves placed in the resulting .ti3 file with the actual calibration that was used for that particular print.
    @@ -424,13 +442,11 @@ Override colorimeter instruments calibration. This will only work with colorimeters that rely on sensor spectral sensitivity calibration information (ie. the X-Rite i1d3, - or the DataColor Spyder4).This -can -improve -a - - - colorimeters accuracy for a particular type of display.
    + or the DataColor Spyder4 & + Spyder 5).This + can + improve + a colorimeters accuracy for a particular type of display.

    The -T ratio argument modifies the patch consistency tolerance threshold for some diff --git a/doc/cht_format.html b/doc/cht_format.html old mode 100644 new mode 100755 diff --git a/doc/collink.html b/doc/collink.html old mode 100644 new mode 100755 index edd58b1..0bb3e77 --- a/doc/collink.html +++ b/doc/collink.html @@ -58,6 +58,7 @@ + Verbose
    @@ -121,6 +122,7 @@ existing + profile, rather than link (Debug option)

    @@ -209,6 +212,7 @@ preserve + device curves in result
     
    @@ -381,6 +388,7 @@ Gamut + Mapping Mode using inverse outprofile A2B [optional source @@ -430,6 +438,7 @@ s + = saturation, a = absolute colorimetric

    @@ -564,6 +575,7 @@ aw + Absolute Colorimetric (in Jab) with scaling to fit white point

    @@ -643,6 +656,7 @@ r + White Point Matched Appearance [ICC Relative Colorimetric]


    @@ -841,6 +859,7 @@ s + Enhanced Saturation [ICC Saturation]
    @@ -913,6 +933,7 @@ al + rl - White Point Matched Colorimetric (Lab)  
    @@ -1060,6 +1084,7 @@ either +   pe - Print evaluation environment (CIE 116-1995)
    @@ -1099,6 +1124,7 @@ either +   pc - Critical print evaluation environment (ISO-3664 P1)


    @@ -1363,6 +1394,7 @@ Adaptatation + luminance in cd.m^2 (default 50.0)
    @@ -1917,6 +1962,7 @@ destination + eeColor .txt file
    @@ -1939,6 +1985,7 @@ destination + MadVR .3dlut   file
         -I B               @@ -1948,6 +1995,7 @@ destination + Use BT.1886 source EOTF with technical gamma 2.4
     -I b:g.g           Use @@ -1992,6 +2040,7 @@ destination + Video encode input as:
    @@ -2023,6 +2072,7 @@ destination + Video encode output as:          t                @@ -2069,11 +2120,13 @@ destination + RGB (16-235)/255 "TV" levels
         + T                @@ -2094,6 +2147,7 @@ destination + RGB (16-235)/255 "TV" levels, clip WTW [Input Only]
         6                @@ -2115,6 +2169,7 @@ destination + Rec601 YCbCr SD (16-235,240)/255 "TV" levels
         7                @@ -2136,6 +2191,7 @@ destination + Rec709 1125/60Hz YCbCr HD (16-235,240)/255 "TV" levels
         5                @@ -2157,6 +2213,7 @@ destination + Rec709 1250/50Hz YCbCr HD (16-235,240)/255 "TV" levels
         2                @@ -2178,6 +2235,7 @@ destination + Rec2020 YCbCr UHD (16-235,240)/255 "TV" levels
         C                @@ -2199,6 +2257,7 @@ destination + Rec2020 Constant Luminance YCbCr UHD (16-235,240)/255 "TV" levels
         @@ -2221,6 +2280,7 @@ destination + xvYCC Rec601 YCbCr Rec709 Prims. SD (16-235,240)/255 "TV" levels
         @@ -2243,6 +2303,7 @@ destination + xvYCC Rec709 YCbCr Rec709 Prims. HD (16-235,240)/255 "TV" levels
          
    @@ -2327,6 +2389,7 @@ ICC + profile. A TIFF @@ -2363,6 +2426,7 @@ ICC + or JPEG file with embedded profile may be used here.
    A -q
    @@ -2699,6 +2765,7 @@ ICC +  p = perceptual, r = relative colorimetric,
    @@ -2836,9 +2903,11 @@ ICC The -b flag forces RGB source 0,0,0 to map to RGB destination 0,0,0. This may be useful for Video proofing/calibration purposes, where the source is a standard - colorspace such as Rec709, and the display device is well behaved - with black at 0,0,0. By forcing the black mapping, any slight - raising of the black due to display profile tolerances is avoided.
    + colorspace such as Rec709, and the display device is well + behaved with black at 0,0,0, and forcing the black mapping + avoids any slight raising of the black due to display profile + tolerances. On the other hand, any "dead zone" above zero device + input, won't be corrected.

    The -c and -d options allow specification of the viewing conditions for the source @@ -2955,6 +3024,7 @@ ICC +    _______  enle
    @@ -2994,6 +3064,7 @@ ICC +    /
    @@ -3033,6 +3104,7 @@ ICC +   /
    @@ -3072,6 +3144,7 @@ ICC +  /
    @@ -3111,6 +3184,7 @@ ICC + /
    @@ -3156,6 +3230,7 @@ White            &nb + Black
    @@ -3355,6 +3430,7 @@ White            &nb + Full output offset with effective gamma of 2.2
    -I B                  @@ -3364,6 +3440,7 @@ White            &nb + Full input offset (BT.1886 like) with technical gamma of 2.4. This exactly implements the BT.1886 specification.
    -I G                  @@ -3374,6 +3451,7 @@ White            &nb + Full output offset with technical gamma of 2.2

    -I b:2.3             @@ -3384,6 +3462,7 @@ White            &nb + Full input offset (BT.1886 like) with effective gamma of 2.3
    -I g:2.3             @@ -3394,6 +3473,7 @@ White            &nb + Full output offset with effective gamma of 2.3
     -I B:2.35           @@ -3403,6 +3483,7 @@ White            &nb + Full input offset (BT.1886 like) with technical gamma of 2.35
    -I G:2.35           @@ -3412,6 +3493,7 @@ White            &nb + Full output offset with technical gamma of 2.35

    -I b:0.4:2.3        @@ -3424,6 +3506,7 @@ White            &nb + Same as above.
     -I B:0.4:2.35      60% input offset, 40% output offset with technical gamma of 2.35
    @@ -3441,6 +3524,7 @@ White            &nb style="font-family: monospace;">     + T                @@ -3461,10 +3545,12 @@ White            &nb + RGB (16-235)/255 "TV" levels, clip WTW [Input Only]
         + x                @@ -3484,6 +3570,7 @@ White            &nb + xvYCC Rec601 YCbCr Rec709 Prims. SD (16-235,240)/255 "TV" levels
         @@ -3506,6 +3593,7 @@ White            &nb + xvYCC Rec709 YCbCr Rec709 Prims. HD (16-235,240)/255 "TV" levels

    @@ -3550,6 +3638,7 @@ White            &nb + normal RGB 0..1 full range levels (default)
         t                @@ -3571,6 +3660,7 @@ White            &nb + RGB (16-235)/255 "TV" levels
    @@ -3578,6 +3668,7 @@ White            &nb style="font-family: monospace;">     + 6                @@ -3597,6 +3688,7 @@ White            &nb + Rec601 YCbCr SD (16-235,240)/255 "TV" levels
         7                @@ -3618,6 +3710,7 @@ White            &nb + Rec709 1125/60Hz YCbCr HD (16-235,240)/255 "TV" levels
         5                @@ -3639,6 +3732,7 @@ White            &nb + Rec709 1250/50Hz YCbCr HD (16-235,240)/255 "TV" levels
         2                @@ -3660,6 +3754,7 @@ White            &nb + Rec2020 YCbCr UHD (16-235,240)/255 "TV" levels
         C                @@ -3681,6 +3776,7 @@ White            &nb + Rec2020 Constant Luminance YCbCr UHD (16-235,240)/255 "TV" levels
    page.
    diff --git a/doc/colorchecker.jpg b/doc/colorchecker.jpg old mode 100644 new mode 100755 diff --git a/doc/colprof.html b/doc/colprof.html old mode 100644 new mode 100755 diff --git a/doc/colverify.html b/doc/colverify.html old mode 100644 new mode 100755 diff --git a/doc/cube.jpg b/doc/cube.jpg old mode 100644 new mode 100755 diff --git a/doc/dispcal.html b/doc/dispcal.html old mode 100644 new mode 100755 index 993124d..ff96ff2 --- a/doc/dispcal.html +++ b/doc/dispcal.html @@ -65,6 +65,8 @@ + + @@ -130,6 +132,8 @@ for + + @@ -186,6 +190,8 @@ list + + @@ -232,6 +238,8 @@ list + + @@ -263,6 +271,8 @@ list + + @@ -276,6 +286,8 @@ list + +     Display via n'th ChromeCast (default 1, ? for list)
    @@ -325,6 +337,8 @@ list + + @@ -401,6 +415,8 @@ list + + @@ -456,6 +472,8 @@ ICC + + @@ -507,6 +525,8 @@ ICC + + @@ -543,6 +563,8 @@ ICC + + @@ -592,6 +614,8 @@ ICC + + @@ -651,6 +675,8 @@ in + + @@ -708,6 +734,8 @@ temperaturee + + @@ -758,6 +786,8 @@ temperaturee + + @@ -808,6 +838,8 @@ temperaturee + + @@ -858,6 +890,8 @@ temperaturee + + @@ -906,6 +940,8 @@ temperaturee + + @@ -954,6 +990,8 @@ temperaturee + + @@ -1009,6 +1047,8 @@ use + + @@ -1056,6 +1096,8 @@ use + + @@ -1104,6 +1146,8 @@ use + + @@ -1143,6 +1187,8 @@ use + + @@ -1203,6 +1249,8 @@ output + + @@ -1250,6 +1298,8 @@ output + + @@ -1270,6 +1320,8 @@ output + + Use forced black point hack
    -dmadvr [MSWin only] causes test patches to be displayed using the MadVR - video renderer. Note that you may have to start the video playback - software and load a video clip in pause for this to work. MadVR - rendering does not need or support VideoLUT access, but be aware - that the state of the Graphics Card VideoLUTs may affect the - results, and therefore may have to be set appropriately using - dispwin. Test patch colors will not be processed by the - MadVR 3dLut by default.
    + video renderer. Note that will have to start MadTPG before + running dispcal, and that while you can adjust the "Test Pattern + Configuration" controls, you should not normally alter the + "Existing Calibration" controls, as dispcal will set these + appropriately.

    -dcc or -dcc:no causes test patches to be displayed using and available installation + + instructions for your platform).

    @@ -2617,6 +2709,8 @@ Set + + @@ -2671,6 +2765,8 @@ the + + @@ -2776,6 +2872,8 @@ As + + @@ -2915,6 +3013,8 @@ If + + @@ -2942,10 +3042,10 @@ If to destination 0,0,0. This may be useful with displays that have a very dark black point, and with an instrument is unable to measure it precisely, and where it is known in some other way that the - display is very well behaved from black (i.e. that it has no "dead - zone" above zero device input). Using this option with a display - that is not well behaved, may result in a loss of shadow detail. - This will override any -k factor.
    + display is very well behaved from black (i.e. that it has no + "dead zone" above zero device input). Using this option with a + display that is not well behaved, may result in a loss of + shadow detail. This will override any -k factor.

    -B  Set the target brightness of black in cd/m^2 (i.e. the absolute Y @@ -3076,56 +3176,9 @@ If colorimeter instruments calibration. This will only work with colorimeters that rely on sensor spectral sensitivity calibration information (ie. the X-Rite i1d3, - or the DataColor Spyder4).This -can -improve -a - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - colorimeters accuracy for a particular type of display.
    + or the DataColor Spyder4 & + Spyder 5).This can improve a colorimeters accuracy for a + particular type of display.

    The -Q flag allows specifying a tristimulus observer, and is used to compute PCS (Profile Connection Space) diff --git a/doc/dispprofloc.html b/doc/dispprofloc.html old mode 100644 new mode 100755 diff --git a/doc/dispread.html b/doc/dispread.html old mode 100644 new mode 100755 index a30ab25..f7fe551 --- a/doc/dispread.html +++ b/doc/dispread.html @@ -45,6 +45,10 @@ + + + + @@ -93,6 +97,10 @@ m + + + + @@ -133,6 +141,10 @@ list + + + + @@ -167,6 +179,10 @@ list + + + + @@ -192,12 +208,20 @@ list + + + + [MSWin] Display via MadVR Video Renderer
     -dcc[:n]             + + + + Display via n'th ChromeCast (default 1, ? for list)
     -s              @@ -381,6 +425,10 @@ Apply + + + + @@ -424,6 +472,10 @@ center, + + + + @@ -463,6 +515,10 @@ normal, + + + + @@ -488,6 +544,10 @@ normal, + + + + @@ -522,6 +582,10 @@ normal, + + + + @@ -546,6 +610,10 @@ normal, + + + +     Video encode output as (16-235)/255 "TV" levels
    @@ -566,6 +634,10 @@ normal, + + + + Quantize test @@ -582,6 +654,10 @@ fit + + + + in nbits
     rate             @@ -905,6 +1017,10 @@ Both: + + + + Override measured refresh rate with rate Hz
         -M "command"         Invoke shell "command" each time a color is measured
    +   -x x                 +Take + manually entered + XYZ values
     -W n|h|x             Override @@ -984,6 +1109,10 @@ n + + + + @@ -1019,6 +1148,10 @@ n + + + + @@ -1116,6 +1249,10 @@ n + + + + @@ -1160,14 +1297,12 @@ n
    -dmadvr [MSWin only] causes test patches to be displayed using the MadVR - video renderer. Note that you may have to start the video playback - software and load a video clip in pause for this to work. MadVR - rendering does not need or support VideoLUT access, so the -K option should be used to read calibrated values. - Be aware that the state of the Graphics Card VideoLUTs may affect - the results, and therefore may have to be set appropriately using - dispwin. By default the test patch colors will not be - processed by the MadVR 3dLut (see the -V flag).
    + video renderer. Note that will have to start MadTPG before + running dispread, and that while you can adjust the "Test Pattern + Configuration" controls, you should not normally alter the + "Existing Calibration" controls, as dispread will set these + appropriately. See also -V flag.

    -dcc or -dcc:no causes test patches to be displayed using and available installation + falls back to the Default receiver (see installation + + + + instructions for your platform).

    -c: The @@ -1388,41 +1527,9 @@ n colorimeter instruments calibration. This will only work with colorimeters that rely on sensor spectral sensitivity calibration information (ie. the X-Rite i1d3, - or the DataColor Spyder4).This -can -improve -a - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - colorimeters accuracy for a particular type of display.
    + or the DataColor Spyder4 & + Spyder 5).This can improve a colorimeters accuracy for a + particular type of display.

    The -Q flag allows specifying a tristimulus observer, and is used to compute PCS (Profile Connection Space) @@ -1515,6 +1622,14 @@ a will abort. Note that a test window will also be created on the system running dispread.

    + The -x flag causes dispread to expect + values to be manually entered for each reading, rather than using an + instrument to do the measurements.  This mode is ideal if your + instrument is not supported by Argyll. XYZ values should be entered. + It is possible to navigate about the test values being measured, so + as to do them in any order, as well as re-do values, in case of any + mistakes.
    +
    The -W n|h|x parameter overrides the default serial communications flow control setting. The value n turns diff --git a/doc/dispwin.html b/doc/dispwin.html old mode 100644 new mode 100755 index 6036e76..05db989 --- a/doc/dispwin.html +++ b/doc/dispwin.html @@ -50,6 +50,7 @@ Verbose + mode
     
     
         -dcc[:n]             + Display via n'th ChromeCast (default 1, ? for list)
    @@ -147,6 +152,7 @@ ho,vi: + = left/top, 0.5 = center, 1.0 = right/bottom etc.
    @@ -167,6 +173,7 @@ ss: + = half, 1.0 = normal, 2.0 = double etc.
                          @@ -180,6 +187,7 @@ ss: + ss,vs: = optional horizontal, vertical scale.
          Video encode output as (16-235)/255 "TV" levels
    -s filename.cal      @@ -287,6 +299,7 @@ the + currently loaded Video LUT to 'filename'

    @@ -330,6 +344,7 @@ that + calfile/profile cal. is currently loaded in LUT
    Install profile for display and use it's calibration
    @@ -369,6 +385,7 @@ that +     Un-install profile for display
    @@ -389,6 +406,7 @@ the + install/uninstall scope for OS X [nlu] or Vista [lu]
                          @@ -408,6 +426,7 @@ is + one of: n = network, l = local system, u = user (default)
    Load installed profiles cal. into Video LUT
    @@ -448,6 +468,7 @@ is + [X11 only] Run in daemon loader mode for given X11 server
    @@ -470,6 +491,7 @@ debug + diagnostics to stderr    .cal or .icm) into LUT, and exit. -dmadvr [MSWin only] causes test patches to be displayed using the MadVR - video renderer. Note that you may have to start the video playback - software and load a video clip in pause for this to work. MadVR - rendering does not need or support VideoLUT access, but be aware - that the state of the Graphics Card VideoLUTs may affect the results - (check this using dispwin). Test patch colors will be - processed by the MadVR 3dLut by default (see -n - flag).
    + video renderer. Note that will have to start MadTPG before + running dispread, and that while you can adjust the "Test Pattern + Configuration" controls, you should not normally alter the + "Existing Calibration" controls, as dispread will set these + appropriately. See -n flag.

    -dcc or -dcc:no causes test patches to be displayed using and available installation + falls back to the Default receiver (see installation + instructions for your platform).

    The -P diff --git a/doc/evalInputTargets.html b/doc/evalInputTargets.html old mode 100644 new mode 100755 diff --git a/doc/extracticc.html b/doc/extracticc.html old mode 100644 new mode 100755 diff --git a/doc/extractttag.html b/doc/extractttag.html old mode 100644 new mode 100755 diff --git a/doc/fakeCMY.html b/doc/fakeCMY.html old mode 100644 new mode 100755 diff --git a/doc/fakeread.html b/doc/fakeread.html old mode 100644 new mode 100755 diff --git a/doc/filmread.html b/doc/filmread.html old mode 100644 new mode 100755 diff --git a/doc/filmtarg.html b/doc/filmtarg.html old mode 100644 new mode 100755 diff --git a/doc/gamma.html b/doc/gamma.html old mode 100644 new mode 100755 diff --git a/doc/gamutmapping1.jpg b/doc/gamutmapping1.jpg old mode 100644 new mode 100755 diff --git a/doc/greytiff.html b/doc/greytiff.html old mode 100644 new mode 100755 diff --git a/doc/i1d.jpg b/doc/i1d.jpg old mode 100644 new mode 100755 diff --git a/doc/i1d3_1.jpg b/doc/i1d3_1.jpg old mode 100644 new mode 100755 diff --git a/doc/i1d3_2.jpg b/doc/i1d3_2.jpg old mode 100644 new mode 100755 diff --git a/doc/i1m.jpg b/doc/i1m.jpg old mode 100644 new mode 100755 diff --git a/doc/i1p.jpg b/doc/i1p.jpg old mode 100644 new mode 100755 diff --git a/doc/i1pro2.jpg b/doc/i1pro2.jpg old mode 100644 new mode 100755 diff --git a/doc/i1proDriver.html b/doc/i1proDriver.html old mode 100644 new mode 100755 diff --git a/doc/i1proDriver.xls b/doc/i1proDriver.xls old mode 100644 new mode 100755 diff --git a/doc/i1proHiRes.html b/doc/i1proHiRes.html old mode 100644 new mode 100755 diff --git a/doc/i1proHiRes.jpg b/doc/i1proHiRes.jpg old mode 100644 new mode 100755 diff --git a/doc/i1proHiRes.zip b/doc/i1proHiRes.zip old mode 100644 new mode 100755 diff --git a/doc/i1scan14.jpg b/doc/i1scan14.jpg old mode 100644 new mode 100755 diff --git a/doc/iccdump.html b/doc/iccdump.html old mode 100644 new mode 100755 diff --git a/doc/iccgamut.html b/doc/iccgamut.html old mode 100644 new mode 100755 diff --git a/doc/iccgamutmapping.html b/doc/iccgamutmapping.html old mode 100644 new mode 100755 diff --git a/doc/icclu.html b/doc/icclu.html old mode 100644 new mode 100755 diff --git a/doc/illumread.html b/doc/illumread.html old mode 100644 new mode 100755 diff --git a/doc/illumread_1.jpg b/doc/illumread_1.jpg old mode 100644 new mode 100755 diff --git a/doc/illumread_2.jpg b/doc/illumread_2.jpg old mode 100644 new mode 100755 diff --git a/doc/illumread_3.jpg b/doc/illumread_3.jpg old mode 100644 new mode 100755 diff --git a/doc/illumread_4.jpg b/doc/illumread_4.jpg old mode 100644 new mode 100755 diff --git a/doc/illumread_5.jpg b/doc/illumread_5.jpg old mode 100644 new mode 100755 diff --git a/doc/illumread_6.jpg b/doc/illumread_6.jpg old mode 100644 new mode 100755 diff --git a/doc/instruments.html b/doc/instruments.html old mode 100644 new mode 100755 index f5897d5..2a970bd --- a/doc/instruments.html +++ b/doc/instruments.html @@ -25,6 +25,66 @@
        specbos 1211 & 1201                    + + + + + + + + + + + + + + + + + + + + + + - Tele-Spectro-Radiometer
    +
    + Image Engineering:
    +
    +     EX1                                               + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + @@ -90,6 +150,10 @@ + + + + @@ -132,6 +196,10 @@ + + + + @@ -174,6 +242,10 @@ + + + + @@ -218,6 +290,10 @@ + + + + @@ -260,6 +336,10 @@ + + + + @@ -302,6 +382,10 @@ + + + + @@ -344,6 +428,10 @@ + + + + @@ -386,6 +474,10 @@ + + + + @@ -482,6 +574,10 @@ + + + + @@ -525,6 +621,10 @@ + + + + @@ -577,6 +677,10 @@ + + + + @@ -621,6 +725,10 @@ + + + + @@ -670,6 +778,10 @@ + + + + @@ -696,7 +808,11 @@
    Other:
        Colorimètre - HCFR                          + HCFR                        + + + + @@ -764,14 +880,23 @@ + + + + - - display colorimeter
    -
    + - display colorimeter
    +     SwatchMate Cube                         + + + + - reflective colorimeter
    +
    Other instruments can be supported indirectly, since patch result files created by other packages can be imported into Argyll.

    @@ -1077,6 +1202,10 @@ + + + + @@ -1211,14 +1340,32 @@     Availability:

    The specbos 1211 and 1201from     and 1201 from JETI  are currently available instruments. These are reference grade instruments capable of emissive and ambient measurements, and are often used for monitor, projector and cinema calibration & - characterization, and colorimeter calibration, amongst many other - uses.
    + characterization, lighting measurement and colorimeter + calibration, amongst many other uses.

    +
    +

    Image Engineering EX1
    +

    + Image Engineering EX1
    +
    + Availability:
    +
    +     The Image + + + + Engineering EX1 is a currently available instruments. This is + a high resolution spectrometer intended for the measurement of light + sources. +


    @@ -1235,6 +1382,10 @@ + + + + Klein Instruments  @@ -1242,6 +1393,10 @@ + + + + is a currently available instrument. It is noted for it's speed, high precision, and ability to measure to very low light @@ -1548,6 +1703,10 @@ + + + + @@ -1610,6 +1769,10 @@ + + + + @@ -1653,6 +1816,10 @@ + + + + @@ -1712,6 +1879,10 @@ Gretag + + + + @@ -1957,6 +2128,10 @@ Gretag + + + + @@ -1987,6 +2162,10 @@ Gretag + + + + @@ -2034,6 +2213,10 @@ Gretag + + + + @@ -2077,6 +2260,10 @@ Gretag + + + + @@ -2144,6 +2331,10 @@ href="http://www8.hp.com/us/en/products/oas/product-detail.html?oid=5225568">HP + + + + DreamColor instruments are also reported to work. They will appear as a be a the same as the i1Display Pro.
    @@ -2253,6 +2444,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + @@ -2300,6 +2495,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + @@ -2343,6 +2542,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + @@ -2411,6 +2614,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + @@ -2454,6 +2661,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + @@ -2530,6 +2741,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + @@ -2573,6 +2788,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + @@ -2739,6 +2958,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + @@ -2791,6 +3014,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + @@ -2838,6 +3065,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + @@ -2874,7 +3105,11 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey     Operation:

    These instruments are capable of using using CCSS (Colorimeter + href="file:///D:/src/argyll/doc/File_Formats.html#ccss">Colorimeter + + + + Calibration Spectral Sample) files, and this also gives the instrument the capability of using a non-default standard observer. CCSS files can be created using the Huey + + + + @@ -3007,6 +3246,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + @@ -3054,6 +3297,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + @@ -3111,6 +3358,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + @@ -3172,6 +3423,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + @@ -3215,6 +3470,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + @@ -3239,14 +3498,17 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey is a low cost display colorimeter instrument from Hughski.
    + ArgyllCMS will also work with the ColorHug2.

    Operation:

    Due to the nature of its sensor, the ColorHug accuracy is quite - dependent on the instrument calibration matrix. A custom .CCMX will - greatly assist it's accuracy, although a workaround is to calibrate - your display using its native white point, rather than aiming for - some absolute white point such as D65.
    + dependent on the instrument calibration matrix. (The ColorHug2 + is much more forgiving though). A custom .CCMX will greatly assist + it's accuracy, although a workaround is to calibrate your display + using its native white point, rather than aiming for some absolute + white point such as D65.

    The Display Selections for this instrument are:

    @@ -3260,6 +3522,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + LCD, CCFL Backlight [Default]
       c                  @@ -3273,6 +3539,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + CRT display
       p                  @@ -3286,6 +3556,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + Projector
       e                  @@ -3298,6 +3572,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + LCD, White LED Backlight
       F                  @@ -3311,6 +3589,10 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + Factory matrix (For Calibration) [CB1]
       R                 @@ -3324,9 +3606,104 @@ href="http://www.pantone.com/pages/products/product.aspx?pid=562&ca=2">Huey + + + + Raw Reading (For Factory matrix Calibration) [CB2]

    +

    + SwatchMate + Cube
    +
    + SwatchMate Cube
    +
    +     Availability:
    +
    +     The Cube from SwatchMate + is a currently available entry level Colorimeter, with somewhat + limited accuracy. The ArgyllCMS driver provides two + alternative calibrations that noticably improve + this accuracy.
    +
    + The Calibration Selections for this instrument are:
    +
    +    m +                 + + + + Matt surfaces [Default]
    +    g                  + + + + + + + + + + + + + + + + Gloss surfaces
    +    N +                 + + + + Native Calibration
    +
    + Operation:
    +
    + The Cube must be connected via USB for operation with ArgyllCMS, and + can be connected either by USB or using Bluetooth LE when used with + ArgyllPRO ColorMeter on + capable Android devices.
    +
    + The Cube goes to sleep fairly rapidly and must be woken up by + pressing the top of it before connecting via USB to be recognized by + ArgyllCMS, although once connected, and with an ArgyllCMS utility + running, it should stay awake.
    +
    + When connecting via Bluetooth to ColorMeter, the foreground + application will be the one that connects to it.
    +
    + The ability to measure values into its own memory and recover them + later is not supported, since it is not possible to use the + ArgyllCMS calibrations with this feature.
    +
    + Calibration:
    +
    + As well as the normal white calibration step, the ArgyllCMS driver + offers two option supplemental calibration steps that can improve + accuracy, but both require appropriate calibration conditions. You + can use spotread with the 'k' command + to trigger this calibration.
    +
    + The black calibration requires a light trap, and the easiest + way of providing this is to place the Cube in a location that is + dark (i.e. not illuminated directly by any light) and some distance + from any surface. A practical approach I have used is to place the + measuring end in a thick black sock, and hide it from direct + illumination while this calibration step is done.
    +
    + The gloss calibration requires a black glossy surface. I + have used a paint catalog gloss paint black sample square for this, + but some other completely black glossy surface of sufficient size + such as a glossy black plastic item or a smooth surface painted in + gloss black paint should also work.
    +
    +
    +



    diff --git a/doc/invprofcheck.html b/doc/invprofcheck.html old mode 100644 new mode 100755 index bd611b3..65502ee --- a/doc/invprofcheck.html +++ b/doc/invprofcheck.html @@ -1,133 +1,168 @@ - - invprofcheck - - - - -

    profile/invprofcheck

    -

    Summary

    -Check ICC forward against reverse -lookup. -
    -

    Usage Summary

    -usage: invprofcheck -[-options] profile.icm
    - -v [level]   -verbosity level (default 1), 2 to print each DE
    - -l -limit     set total ink -limit (estimate by default)
    -     -L -klimit    set black channel ink -limit (estimate by default)
    - -h           -high res test (27)
    - -u           -Ultra high res test (61)
    - -R res       Specific grid -resolution
    -     -c           -Show CIE94 delta E values
    - -k           -Show CIEDE2000 delta E values
    - -w           -create X3DOM visualisation (profile.x3d.html)
    - -x           -Use X3DOM axes
    - -e           -Color vectors acording to delta E
    - profile.icm  -Profile to check     -
    -

    Usage Details and Discussion

    -invprofcheck provides a way of checking how well an ICC profile inverse transform inverts -the forward transform. For devices with more than 4 channels, a total -ink limit is assumed, and (if no -l -parameter is given) a reasonable number is deduced from the reverse -table. A grid of device values is created, and the transform from -PCS->device, and then device->PCS is computed in L*a*b* space. -The average, maximum and RMS error delta E values are computed and -displayed in the chosen delta E metric. A X3DOM plot of the error vectors can -be created. invprofcheck tries -to only test in-gamut color values. Note that because it scans a device -grid, for a CMYK device, the density of test points will be -progressively higher in the dark regions, and the average and RMS -values will be distorted by the denser sampling.
    -
    -The -v flag prints out extra information during the checking. A -value greater than 1 will print the color values of each test point.
    -
    -The -l flag allows setting a total ink limit (TAC) for printing -devices. If a device has a total ink limit, and hasn't been -characterised with device values above this limit, then plotting the -gamut in these areas will almost certainly be misleading. The ink limit -will be in final calibrated device values if the profile includes -calibration information.
    -
    -The -L flag allows setting a black channel ink limit for -printing -devices. If a device has a black ink limit, and hasn't been -characterised with device values above this limit, then plotting the -gamut in these areas will almost certainly be misleading. The black ink -limit -will be final calibrated device values if the profile -includes calibration information.
    -
    -The default device grid is relativy low, and 11 (ie. 11 x 11 x 11 for -an RGB device, 11 x 11 x 11 x 11 for a CMYK device etc.).
    -
    -The -h flag selects a higher -device grid resolution of 27.
    -
    -The -u flag selects an -extremely high device grid resolution of 61. This will probably take a -long time to run.
    -
    -The -G res option allows a -specific grid resolution to be used.
    -
    -The -c option causes the error differences to be -displayed -in CIE94 delta E, rather than plain L*a*b* delta E. CIE94 delta E has a -closer -correspondence with perceived color differences than the default CIE76 -delta E values.
    -
    -The -k option causes the error differences to be -displayed -in CIEDE2000 delta E, rather than plain L*a*b* delta E. CIEDE2000 delta -E has a -closer -correspondence with perceived color differences than either CIE76 or -CIE94 delta E values.
    -
    -The -w creates a X3DOM 3D -visualization -of the differences between the test points and the profiles prediction -of -the resulting colors.
    -
    -The -x flag adds Lab axes to the X3DOM output.
    -
    -The -e flag causes the error -vectors in the X3DOM output to be color coded according to their -lengths, from longest to shortest: yellow, red, magenta, blue, cyan and -green.
    -
    -
    -
    - + + invprofcheck + + + + +

    profile/invprofcheck

    +

    Summary

    + Check ICC forward against + reverse + lookup. +
    +

    Usage Summary

    + usage: invprofcheck + [-options] profile.icm
    +  -v [level]   + verbosity level (default 1), 2 to print each DE
    +  -l + limit     set total ink + limit (estimate by default)
    +      -L +klimit +    set black channel ink + limit (estimate by default)
    +  -h           +high + res test (27)
    +  -u           +Ultra + high res test (61)
    +  -R res       Specific grid + resolution
    +  -I           + Do bwd to fwd check
    +      -c           +Show + CIE94 delta E values
    +  -k           +Show + CIEDE2000 delta E values
    +  -w           +create + X3DOM visualisation (profile.x3d.html)
    +  -x           +Use + X3DOM axes
    +  -e           +Color + vectors acording to delta E
    +  profile.icm  + Profile to check     +
    +

    Usage Details and Discussion

    + invprofcheck provides a way of checking how well an ICC profile inverse transform + inverts + the forward transform. For devices with more than 4 channels, a + total + ink limit is assumed, and (if no -l + parameter is given) a reasonable number is deduced from the reverse + table. A grid of device values is created, and the transform from + PCS->device, and then device->PCS is computed in L*a*b* space. + The average, maximum and RMS error delta E values are computed and + displayed in the chosen delta E metric. A X3DOM plot of the error vectors + can + be created. invprofcheck + tries + to only test in-gamut color values. Note that because it scans a + device + grid, for a CMYK device, the density of test points will be + progressively higher in the dark regions, and the average and RMS + values will be distorted by the denser sampling.
    +
    + The -v flag prints out extra information during the + checking. A + value greater than 1 will print the color values of each test point.
    +
    + The -l flag allows setting a total ink limit (TAC) for + printing + devices. If a device has a total ink limit, and hasn't been + characterised with device values above this limit, then plotting the + gamut in these areas will almost certainly be misleading. The ink + limit + will be in final calibrated device values if the profile includes + calibration information.
    +
    + The -L flag allows setting a black channel ink limit for + printing + devices. If a device has a black ink limit, and hasn't been + characterised with device values above this limit, then plotting the + gamut in these areas will almost certainly be misleading. The black + ink + limit + will be final calibrated device values if the profile + includes calibration information.
    +
    + The default device grid is relativy low, and 11 (ie. 11 x 11 x 11 + for + an RGB device, 11 x 11 x 11 x 11 for a CMYK device etc.).
    +
    + The -h flag selects a + higher + device grid resolution of 27.
    +
    + The -u flag selects an + extremely high device grid resolution of 61. This will probably take + a + long time to run.
    +
    + The -G res option allows a + specific grid resolution to be used.
    +
    + If the -I option is used, then the grid is in L*a*b* space, + so out of gamut clipping behavior can be examined. Delta E's will be + high due to the clipping.
    +
    + The -c option causes the error differences to be + displayed + in CIE94 delta E, rather than plain L*a*b* delta E. CIE94 delta E + has a + closer + correspondence with perceived color differences than the default + CIE76 + delta E values.
    +
    + The -k option causes the error differences to be + displayed + in CIEDE2000 delta E, rather than plain L*a*b* delta E. CIEDE2000 + delta + E has a + closer + correspondence with perceived color differences than either CIE76 or + CIE94 delta E values.
    +
    + The -w creates a X3DOM + 3D + visualization + of the differences between the test points and the profiles + prediction + of + the resulting colors.
    +
    + The -x flag adds Lab axes to the X3DOM output.
    +
    + The -e flag causes the + error + vectors in the X3DOM output to be color coded according to their + lengths, from longest to shortest: yellow, red, magenta, blue, cyan + and + green.
    +
    +
    +
    + diff --git a/doc/kodak2ti3.html b/doc/kodak2ti3.html old mode 100644 new mode 100755 diff --git a/doc/monitorcontrols.html b/doc/monitorcontrols.html old mode 100644 new mode 100755 diff --git a/doc/mox.jpg b/doc/mox.jpg old mode 100644 new mode 100755 diff --git a/doc/moxxr.jpg b/doc/moxxr.jpg old mode 100644 new mode 100755 diff --git a/doc/mppcheck.html b/doc/mppcheck.html old mode 100644 new mode 100755 diff --git a/doc/mpplu.html b/doc/mpplu.html old mode 100644 new mode 100755 diff --git a/doc/mppprof.html b/doc/mppprof.html old mode 100644 new mode 100755 diff --git a/doc/oeminst.html b/doc/oeminst.html old mode 100644 new mode 100755 diff --git a/doc/printcal.html b/doc/printcal.html old mode 100644 new mode 100755 diff --git a/doc/printtarg.html b/doc/printtarg.html old mode 100644 new mode 100755 diff --git a/doc/profcheck.html b/doc/profcheck.html old mode 100644 new mode 100755 diff --git a/doc/refine.html b/doc/refine.html old mode 100644 new mode 100755 diff --git a/doc/revfix.html b/doc/revfix.html old mode 100644 new mode 100755 diff --git a/doc/scanin.html b/doc/scanin.html old mode 100644 new mode 100755 diff --git a/doc/sl.jpg b/doc/sl.jpg old mode 100644 new mode 100755 diff --git a/doc/spec2cie.html b/doc/spec2cie.html old mode 100644 new mode 100755 index d25b0a0..7911948 --- a/doc/spec2cie.html +++ b/doc/spec2cie.html @@ -16,6 +16,7 @@ spec2cie [options] input.ti3 + output.ti3
         -v            @@ -23,6 +24,7 @@  -I illum   +    Override actual instrument illuminant in .ti3 file:
               @@ -31,6 +33,7 @@                 + (only used in conjunction with -f)
       -o observ  +    Choose CIE Observer for spectral data:
                     + 1931_2     (def.), - 1964_10, S&B 1955_2, shaw, J&V 1978_2
    + 1964_10, S&B 1955_2, shaw, J&V 1978_2 or file.cmf
     -n             Don't output + spectral values
     -p             @@ -73,10 +80,12 @@ output Measurement + file
     output.ti3     + Converted measurement file

    Comments

    This program takes the (usually reflective) spectral data in a .ti3 @@ -129,6 +138,7 @@ Measurement computation illuminant used for FWA (see -i below). See + colprof -f for a fuller explanation.

    The -i parameter allows specifying a @@ -185,6 +195,8 @@ Measurement   shaw selects the Shaw and Fairchild 1997 2 degree observer

    + or a .cmf file can be provided as an argument.
    +
    Note that if an observer other than 1931 2 degree is chosen, the resulting ICC profile will not be standard, and cannot be freely interchanged with other profiles that that us the standard 1931 2 diff --git a/doc/specplot.html b/doc/specplot.html old mode 100644 new mode 100755 index 05b260b..45c9f72 --- a/doc/specplot.html +++ b/doc/specplot.html @@ -3,36 +3,42 @@ specplot + charset=windows-1252">

    xicc/specplot

    Summary

    A simple tool to plot spectrum files (.sp, .cmf, .ccss etc.), and - compute the  CCT and VCT, CRI, XYZ, x,y and L*a*b* values.
    + compute the  CCT and VCT, CRI, TLCI, XYZ, x,y and L*a*b* + values.

    Usage summary

    specplot [infile1.sp, infile2.sp, ...]
     -v               + verbose
     -c               + combine multiple files into one plot
     -z               don't + make range cover zero
     -u level         plot effect of adding estimated UV level
     -U               + plot effect of adding range of estimated UV level
     [infile.sp ...]  spectrum files to plot
                      + default is all built in illuminants

    Usage Details and Discussion

    diff --git a/doc/splitti3.html b/doc/splitti3.html old mode 100644 new mode 100755 diff --git a/doc/spotread.html b/doc/spotread.html old mode 100644 new mode 100755 index f3964f5..3fe030f --- a/doc/spotread.html +++ b/doc/spotread.html @@ -44,6 +44,7 @@ +       Verbose mode

    @@ -205,6 +210,7 @@ + Use display white brightness relative measurement mode
    @@ -220,6 +226,7 @@ + Use display white point relative chromatically adjusted mode
     -p @@ -278,6 +286,7 @@ + Use projectorprojector @@ -370,6 +381,7 @@ + Use ambient flash measurement mode (absolute results)
    @@ -399,6 +411,7 @@ + Display type - instrument specific list to choose from.
    @@ -428,6 +441,7 @@ M0, + M1, M2, A, D50 (def.), D50M2, D65, F5, F8, F10 or file.sp

     -N                    @@ -795,6 +820,7 @@ D50 + Disable initial calibration of instrument if possible
    @@ -824,6 +850,7 @@ D50 + Do one cal. or measure and exit
    @@ -858,6 +885,7 @@ D50 + Apply Colorimeter Correction Matrix
    @@ -891,6 +919,7 @@ Samples + for calibration
    @@ -915,6 +944,7 @@ Samples +      Override refresh, non-refresh display mode
     -Y R:rate             @@ -927,6 +957,7 @@ Samples + Override measured refresh rate with rate Hz
     -Y A
    @@ -1000,6 +1032,7 @@ none, + Optional file to save reading results
    colprof + -f for a fuller explanation.

    The -i parameter allows specifying a @@ -1263,12 +1299,12 @@ none, CIEDE2000 error to the measured color. The last is the daylight color that has a minimum CIEDE2000 error to the measured color. The delta E between the closest temperature and the measured color is - also shown for each. The Color Rendering Index (CRI Ra) is also - computed if the instrument is capable of spectral measurement. If - the notation (Invalid) is - displayed after the CRI, then this means that the the spectrum white - point is to far from the black body and Daylight locus to be - meaningful.
    + also shown for each. The Color Rendering Index (CRI Ra) including + the R9 value, plus the TLCI (Qa) is also computed if the instrument + is capable of spectral measurement. If the notation (Invalid) is displayed after the + CRI or TLCI, then this means that the the spectrum white point is to + far from the black body and Daylight locus to be meaningful.

    -N Any instrument that requires regular calibration will ask for @@ -1306,35 +1342,11 @@ none, colorimeter instruments calibration. This will only work with colorimeters that rely on sensor spectral sensitivity calibration information (ie. the X-Rite i1d3, - or the DataColor Spyder4).This -can -improve -a - - - - - - - - - - - - - - - - - - - - - - - - - colorimeters accuracy for a particular type of display.
    + or the DataColor Spyder4 & + Spyder5).This + can + improve + a colorimeters accuracy for a particular type of display.

    The -Y r and @@ -1354,6 +1366,7 @@ a + -Y n options overrides the refresh display mode set by the -y display type selection, with -Y r forcing refresh display mode, diff --git a/doc/srgbplot.gif b/doc/srgbplot.gif old mode 100644 new mode 100755 diff --git a/doc/ss.jpg b/doc/ss.jpg old mode 100644 new mode 100755 diff --git a/doc/surface.jpg b/doc/surface.jpg old mode 100644 new mode 100755 diff --git a/doc/synthcal.html b/doc/synthcal.html old mode 100644 new mode 100755 diff --git a/doc/synthread.html b/doc/synthread.html old mode 100644 new mode 100755 diff --git a/doc/targen.html b/doc/targen.html old mode 100644 new mode 100755 diff --git a/doc/ti3_format.html b/doc/ti3_format.html old mode 100644 new mode 100755 index c42a124..38a1eb7 --- a/doc/ti3_format.html +++ b/doc/ti3_format.html @@ -3,7 +3,7 @@ Target Information 3 Format File (.ti3) + charset=windows-1252"> @@ -55,10 +55,16 @@ There shall be a DEVICE_CLASS keyword that has a value of "OUTPUT", - "DISPLAY" or "INPUT".
    + + + "DISPLAY",  "INPUT" or "EMISINPUT".
    This indicates to the profile program what type of device the color - information is from.
    + information is from. (An OUTPUT device is typically a printer. An + INPUT device is typically a Scanner or Camera with data from a + reflective reference chart. An EMISINPUT is a camera with emissive + reference data. ).

    An "OUTPUT" type device may have a TOTAL_INK_LIMIT @@ -73,6 +79,8 @@ keyword that contains the absolute XYZ value of white in candelas per meter squared, e.g. "112.334770 + + 119.657745 121.474236".

    A display device may also have a
    -         "Xrite DTP22"
    -         "Xrite DTP41"
    -         "Xrite DTP51"
    -         "Xrite DTP92"
    -         "Xrite DTP94"
    -        "GretagMacbeth Spectrolino"
    -         "GretagMacbeth SpectroScan"
    -         "GretagMacbeth SpectroScanT"
    -         "Spectrocam"
    -         "GretagMacbeth i1 Display 1"
    -         "GretagMacbeth i1 Display 2"
    -         "Xrite i1 DisplayPro, ColorMunki Display"
    -         "GretagMacbeth i1 Monitor"
    -         "GretagMacbeth i1 Pro"
    -         "X-Rite i1 Pro 2"
    -         "X-Rite ColorMunki"
    -         "Colorimtre HCFR"
    -         "ColorVision Spyder2"
    -         "Datacolor Spyder3"
    -         "Datacolor Spyder4"
    -         "GretagMacbeth Huey"
    -         "ColorMunki Smile"
    -         "Hughski ColorHug"
    -
    +
    "X-Rite DTP20"
    + "X-Rite DTP22"
    + "X-Rite DTP41"
    + "X-Rite DTP51"
    + "X-Rite DTP92"
    + "X-Rite DTP94"
    + "GretagMacbeth Spectrolino"
    + "GretagMacbeth SpectroScan"
    + "GretagMacbeth SpectroScanT"
    + "Spectrocam"
    + "GretagMacbeth i1 Display 1"
    + "GretagMacbeth i1 Display 2"
    + "X-Rite i1 DisplayPro, ColorMunki Display"
    + "GretagMacbeth i1 Monitor"
    + "GretagMacbeth i1 Pro"
    + "X-Rite i1 Pro 2"
    + "X-Rite ColorMunki"
    + "Colorimtre HCFR"
    + "ColorVision Spyder1"
    + "ColorVision Spyder2"
    + "Datacolor Spyder3"
    + "Datacolor Spyder4"
    + "Datacolor Spyder5"
    + "GretagMacbeth Huey"
    + "ColorMunki Smile"
    + "JETI specbos 1201"
    + "JETI specbos"
    + "Klein K-10"
    + "Image Engineering EX1"
    +
    All instruments except the Spectrocam are assumed to have an "A" type illuminant (incandescent lamp of  2850 degrees Kelvin.)

    @@ -157,35 +169,51 @@     Cyan + +                         + + C
        Magenta                     M
        Yellow                       + + Y
        Black                         + + K
        Orange                      + + O
        Red                           + + R
        Green                        + + G
        Blue                           + + B
        White                @@ -193,18 +221,26 @@ Cyan     Light Cyan                  + + c
        Light Magenta             + + m
        Light Yellow               + + y
        Light Black                 + + k
        Medium Cyan             2c
    diff --git a/doc/tiffgamut.html b/doc/tiffgamut.html old mode 100644 new mode 100755 diff --git a/doc/timage.html b/doc/timage.html old mode 100644 new mode 100755 diff --git a/doc/txt2ti3.html b/doc/txt2ti3.html old mode 100644 new mode 100755 diff --git a/doc/ucmm.html b/doc/ucmm.html old mode 100644 new mode 100755 diff --git a/doc/viewgam.html b/doc/viewgam.html old mode 100644 new mode 100755 diff --git a/doc/xicclu.html b/doc/xicclu.html old mode 100644 new mode 100755 -- cgit v1.2.3