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authorJörg Frings-Fürst <debian@jff-webhosting.net>2017-12-03 20:38:41 +0100
committerJörg Frings-Fürst <debian@jff-webhosting.net>2017-12-03 20:38:41 +0100
commitba627dd9ecb578e9852c7b9cce67ec63199d1acf (patch)
tree27c4258311ca8c8ed7ff67a8a0bc7280e8fcae79 /doc/XRGA.html
parent69aec3b712232e93600ecd741269fed1f90b412a (diff)
parent3abb40d43649adb3807180692d8579c405524675 (diff)
Merge branch 'release/2.0.0+repack-1'2.0.0+repack-1
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diff --git a/doc/XRGA.html b/doc/XRGA.html
index 295d7b2..778b8bd 100644..100755
--- a/doc/XRGA.html
+++ b/doc/XRGA.html
@@ -27,6 +27,7 @@
href="https://www.xrite.com/documents/literature/en/L7-462_XRGA_WhitePaper_en.pdf">conversion
+
is possible</a> between these different standards. While such a
conversion is not perfect, it reduces the discontinuities between
old instrument families and current X-Rite instruments.<br>
@@ -133,5 +134,8 @@ href="https://www.xrite.com/documents/literature/en/L7-462_XRGA_WhitePaper_en.pd
(The DTP51 returns only colorimetric data, while the conversion
requires spectral data.)<br>
<br>
+ You can also convert from one standard to the other using <a
+ href="spec2cie.html#A">spec2cie</a>.<br>
+ <br>
</body>
</html>