diff options
author | Jörg Frings-Fürst <debian@jff-webhosting.net> | 2017-11-25 10:16:00 +0100 |
---|---|---|
committer | Jörg Frings-Fürst <debian@jff-webhosting.net> | 2017-11-25 10:16:00 +0100 |
commit | f6b8e0eae4374f339487a33e3e4fe5462d5816e1 (patch) | |
tree | 5f5f764fd6cda404b2ad6e85762c03fce3a335db /doc/XRGA.html | |
parent | 615ab5513e79c4abc5bbe5c993587785b6a1738b (diff) |
New upstream version 2.0.0upstream/2.0.0
Diffstat (limited to 'doc/XRGA.html')
-rwxr-xr-x[-rw-r--r--] | doc/XRGA.html | 4 |
1 files changed, 4 insertions, 0 deletions
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> |