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apidoc/html/index.html

@@ -292,7 +292,7 @@ <h3><a class="anchor" id="autotoc_md48"></a>
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 <td class="markdownTableBodyNone">Fixed Earth System   </td><td class="markdownTableBodyNone">WGS84   </td><td class="markdownTableBodyNone">International Terrestrial Reference System (ITRS)   </td></tr>
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-<p>See the various enums and constants defined in <code><a class="el" href="novas_8h.html">novas.h</a></code>, as well as the descriptions on the various NOVAS routines on how they are appropriate for the old and new methodologies respectively.</p>
+<p>See the various enums and constants defined in <code><a class="el" href="novas_8h.html">novas.h</a></code>, as well as the descriptions on the various NOVAS routines on how they are appropriate for the old and new methodologies respectively. Figure 1 also shows the relation of the various old and new coordinate systems and the (Super)NOVAS functions for converting among them.</p>
 <p>In NOVAS, the barycentric BCRS and the geocentric GCRS systems are effectively synonymous to ICRS. The origin for positions and for velocities, in any reference system, is determined by the <code>observer</code> location.</p>
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doc/README.md

@@ -373,7 +373,8 @@ terms differently:
  
  
 See the various enums and constants defined in `novas.h`, as well as the descriptions on the various NOVAS routines
-on how they are appropriate for the old and new methodologies respectively.
+on how they are appropriate for the old and new methodologies respectively. Figure 1 also shows the relation of the
+various old and new coordinate systems and the (Super)NOVAS functions for converting among them.
 
 In NOVAS, the barycentric BCRS and the geocentric GCRS systems are effectively synonymous to ICRS. The origin for
 positions and for velocities, in any reference system, is determined by the `observer` location.