Add links to generated API docs

Author: mgreter

docs/iau.ab.md

@@ -6,8 +6,6 @@ IAU.ab(pnat, v, s, bm1)
 
 Apply aberration to transform natural direction into proper
 direction.
-SOFA (Standards of Fundamental Astronomy) software collection.
-
 
 ## Given:
   pnat    double[3]   natural direction to the source (unit vector)
@@ -34,7 +32,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
       0.4 microarcsecond.
 
 2) In almost all cases, the maximum accuracy will be limited by the
-   supplied velocity.  For example, if the SOFA iauEpv00 function is
+   supplied velocity.  For example, if the SOFA [iauEpv00][1] function is
    used, errors of up to 5 microarcseconds could occur.
 
 ## References:
@@ -55,4 +53,6 @@ This revision:   2013 October 9
 
 SOFA release 2018-01-30
 
-Copyright (C) 2018 IAU SOFA Board.
+Copyright (C) 2018 IAU SOFA Board.
+
+[1]: iau.epv00.md

docs/iau.af2a.md

@@ -5,8 +5,6 @@
 ```
 
 Convert degrees, arcminutes, arcseconds to radians.
-SOFA (Standards of Fundamental Astronomy) software collection.
-
 
 ## Given:
 ```

docs/iau.apcg.md

@@ -11,8 +11,6 @@ The Earth ephemeris is supplied by the caller.
 The parameters produced by this function are required in the
 parallax, light deflection and aberration parts of the astrometric
 transformation chain.
-SOFA (Standards of Fundamental Astronomy) software collection.
-
 
 ## Given:
 ```
@@ -24,7 +22,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
 
 ## Returned:
 ```
-   astrom iauASTROM*   star-independent astrometry parameters:
+   astrom ASTROM*   star-independent astrometry parameters:
     pmt    double       PM time interval (SSB, Julian years)
     eb     double[3]    SSB to observer (vector, au)
     eh     double[3]    Sun to observer (unit vector)
@@ -103,7 +101,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
    transformation), and atmospheric refraction.
 
 4) The context structure astrom produced by this function is used by
-   iauAtciq* and iauAticq*.
+   [iauAtciq][13]* and [iauAticq][14]*.
 
 ## Called:
 ```
@@ -114,4 +112,7 @@ This revision:   2013 October 9
 
 SOFA release 2018-01-30
 
-Copyright (C) 2018 IAU SOFA Board.
+Copyright (C) 2018 IAU SOFA Board.
+
+[13]: iau.atciq.md
+[14]: iau.aticq.md

docs/iau.apcg13.md

@@ -12,8 +12,6 @@ the Earth ephemeris.
 The parameters produced by this function are required in the
 parallax, light deflection and aberration parts of the astrometric
 transformation chain.
-SOFA (Standards of Fundamental Astronomy) software collection.
-
 
 ## Given:
 ```
@@ -23,7 +21,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
 
 ## Returned:
 ```
-   astrom iauASTROM* star-independent astrometry parameters:
+   astrom ASTROM* star-independent astrometry parameters:
     pmt    double       PM time interval (SSB, Julian years)
     eb     double[3]    SSB to observer (vector, au)
     eh     double[3]    Sun to observer (unit vector)
@@ -73,7 +71,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
 2) All the vectors are with respect to BCRS axes.
 
 3) In cases where the caller wishes to supply his own Earth
-   ephemeris, the function iauApcg can be used instead of the present
+   ephemeris, the function [iauApcg][1] can be used instead of the present
    function.
 
 4) This is one of several functions that inserts into the astrom
@@ -106,7 +104,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
    transformation), and atmospheric refraction.
 
 5) The context structure astrom produced by this function is used by
-   iauAtciq* and iauAticq*.
+   [iauAtciq][13]* and [iauAticq][14]*.
 
 ## Called:
 ```
@@ -118,4 +116,8 @@ This revision:   2013 October 9
 
 SOFA release 2018-01-30
 
-Copyright (C) 2018 IAU SOFA Board.
+Copyright (C) 2018 IAU SOFA Board.
+
+[1]: iau.apcg.md
+[13]: iau.atciq.md
+[14]: iau.aticq.md

docs/iau.apci.md

@@ -12,8 +12,6 @@ caller.
 The parameters produced by this function are required in the
 parallax, light deflection, aberration, and bias-precession-nutation
 parts of the astrometric transformation chain.
-SOFA (Standards of Fundamental Astronomy) software collection.
-
 
 ## Given:
 ```
@@ -27,7 +25,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
 
 ## Returned:
 ```
-   astrom iauASTROM*   star-independent astrometry parameters:
+   astrom ASTROM*   star-independent astrometry parameters:
     pmt    double       PM time interval (SSB, Julian years)
     eb     double[3]    SSB to observer (vector, au)
     eh     double[3]    Sun to observer (unit vector)
@@ -77,7 +75,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
 2) All the vectors are with respect to BCRS axes.
 
 3) In cases where the caller does not wish to provide the Earth
-   ephemeris and CIP/CIO, the function iauApci13 can be used instead
+   ephemeris and CIP/CIO, the function [iauApci13][1] can be used instead
    of the present function.  This computes the required quantities
    using other SOFA functions.
 
@@ -111,7 +109,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
    transformation), and atmospheric refraction.
 
 5) The context structure astrom produced by this function is used by
-   iauAtciq* and iauAticq*.
+   [iauAtciq][13]* and [iauAticq][14]*.
 
 ## Called:
 ```
@@ -123,4 +121,8 @@ This revision:   2013 September 25
 
 SOFA release 2018-01-30
 
-Copyright (C) 2018 IAU SOFA Board.
+Copyright (C) 2018 IAU SOFA Board.
+
+[1]: iau.apci13.md
+[13]: iau.atciq.md
+[14]: iau.aticq.md

docs/iau.apci13.md

@@ -12,8 +12,6 @@ to predict the Earth ephemeris and CIP/CIO.
 The parameters produced by this function are required in the
 parallax, light deflection, aberration, and bias-precession-nutation
 parts of the astrometric transformation chain.
-SOFA (Standards of Fundamental Astronomy) software collection.
-
 
 ## Given:
 ```
@@ -23,7 +21,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
 
 ## Returned:
 ```
-   astrom iauASTROM*  star-independent astrometry parameters:
+   astrom ASTROM*  star-independent astrometry parameters:
     pmt    double       PM time interval (SSB, Julian years)
     eb     double[3]    SSB to observer (vector, au)
     eh     double[3]    Sun to observer (unit vector)
@@ -74,7 +72,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
 2) All the vectors are with respect to BCRS axes.
 
 3) In cases where the caller wishes to supply his own Earth
-   ephemeris and CIP/CIO, the function iauApci can be used instead
+   ephemeris and CIP/CIO, the function [iauApci][1] can be used instead
    of the present function.
 
 4) This is one of several functions that inserts into the astrom
@@ -107,7 +105,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
    transformation), and atmospheric refraction.
 
 5) The context structure astrom produced by this function is used by
-   iauAtciq* and iauAticq*.
+   [iauAtciq][13]* and [iauAticq][14]*.
 
 ## Called:
 ```
@@ -123,4 +121,8 @@ This revision:   2013 October 9
 
 SOFA release 2018-01-30
 
-Copyright (C) 2018 IAU SOFA Board.
+Copyright (C) 2018 IAU SOFA Board.
+
+[1]: iau.apci.md
+[13]: iau.atciq.md
+[14]: iau.aticq.md

docs/iau.apco.md

@@ -9,8 +9,6 @@ parameters for transformations between ICRS and observed
 coordinates.  The caller supplies the Earth ephemeris, the Earth
 rotation information and the refraction constants as well as the
 site coordinates.
-SOFA (Standards of Fundamental Astronomy) software collection.
-
 
 ## Given:
 ```
@@ -32,7 +30,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
 
 ## Returned:
 ```
-   astrom iauASTROM*   star-independent astrometry parameters:
+   astrom ASTROM*   star-independent astrometry parameters:
     pmt    double       PM time interval (SSB, Julian years)
     eb     double[3]    SSB to observer (vector, au)
     eh     double[3]    Sun to observer (unit vector)
@@ -110,7 +108,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
 
 7) In cases where the caller does not wish to provide the Earth
    Ephemeris, the Earth rotation information and refraction
-   constants, the function iauApco13 can be used instead of the
+   constants, the function [iauApco13][1] can be used instead of the
    present function.  This starts from UTC and weather readings etc.
    and computes suitable values using other SOFA functions.
 
@@ -144,7 +142,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
    transformation), and atmospheric refraction.
 
 9) The context structure astrom produced by this function is used by
-   iauAtioq, iauAtoiq, iauAtciq* and iauAticq*.
+   [iauAtioq][13], [iauAtoiq][14], [iauAtciq][15]* and [iauAticq][16]*.
 
 ## Called:
 ```
@@ -160,4 +158,10 @@ This revision:   2013 October 9
 
 SOFA release 2018-01-30
 
-Copyright (C) 2018 IAU SOFA Board.
+Copyright (C) 2018 IAU SOFA Board.
+
+[1]: iau.apco13.md
+[13]: iau.atioq.md
+[14]: iau.atoiq.md
+[15]: iau.atciq.md
+[16]: iau.aticq.md

docs/iau.apco13.md

@@ -13,8 +13,6 @@ obtain the Earth ephemeris, CIP/CIO and refraction constants.
 The parameters produced by this function are required in the
 parallax, light deflection, aberration, and bias-precession-nutation
 parts of the ICRS/CIRS transformations.
-SOFA (Standards of Fundamental Astronomy) software collection.
-
 
 ## Given:
 ```
@@ -33,7 +31,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
 
 ## Returned:
 ```
-   astrom iauASTROM* star-independent astrometry parameters:
+   astrom ASTROM* star-independent astrometry parameters:
     pmt    double       PM time interval (SSB, Julian years)
     eb     double[3]    SSB to observer (vector, au)
     eh     double[3]    Sun to observer (unit vector)
@@ -71,14 +69,14 @@ SOFA (Standards of Fundamental Astronomy) software collection.
     present function is that the JD day represents UTC days whether
     the length is 86399, 86400 or 86401 SI seconds.
 
-    Applications should use the function iauDtf2d to convert from
+    Applications should use the function [iauDtf2d][1] to convert from
     calendar date and time of day into 2-part quasi Julian Date, as
     it implements the leap-second-ambiguity convention just
     described.
 
 2)  The warning status "dubious year" flags UTCs that predate the
     introduction of the time scale or that are too far in the
-    future to be trusted.  See iauDat for further details.
+    future to be trusted.  See [iauDat][2] for further details.
 
 3)  UT1-UTC is tabulated in IERS bulletins.  It increases by exactly
     one second at the end of each positive UTC leap second,
@@ -132,7 +130,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
 
 9)  In cases where the caller wishes to supply his own Earth
     ephemeris, Earth rotation information and refraction constants,
-    the function iauApco can be used instead of the present function.
+    the function [iauApco][3] can be used instead of the present function.
 
 10) This is one of several functions that inserts into the astrom
     structure star-independent parameters needed for the chain of
@@ -164,7 +162,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
 ```
 
 11) The context structure astrom produced by this function is used
-    by iauAtioq, iauAtoiq, iauAtciq* and iauAticq*.
+    by [iauAtioq][15], [iauAtoiq][16], [iauAtciq][17]* and [iauAticq][18]*.
 
 ## Called:
 ```
@@ -186,4 +184,12 @@ This revision:   2013 December 5
 
 SOFA release 2018-01-30
 
-Copyright (C) 2018 IAU SOFA Board.
+Copyright (C) 2018 IAU SOFA Board.
+
+[1]: iau.dtf2d.md
+[2]: iau.dat.md
+[3]: iau.apco.md
+[15]: iau.atioq.md
+[16]: iau.atoiq.md
+[17]: iau.atciq.md
+[18]: iau.aticq.md

docs/iau.apcs.md

@@ -12,8 +12,6 @@ caller.
 The parameters produced by this function are required in the space
 motion, parallax, light deflection and aberration parts of the
 astrometric transformation chain.
-SOFA (Standards of Fundamental Astronomy) software collection.
-
 
 ## Given:
 ```
@@ -26,7 +24,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
 
 ## Returned:
 ```
-   astrom iauASTROM*   star-independent astrometry parameters:
+   astrom ASTROM*   star-independent astrometry parameters:
     pmt    double       PM time interval (SSB, Julian years)
     eb     double[3]    SSB to observer (vector, au)
     eh     double[3]    Sun to observer (unit vector)
@@ -88,9 +86,9 @@ SOFA (Standards of Fundamental Astronomy) software collection.
 ```
 
 4) In cases where the caller does not wish to provide the Earth
-   ephemeris, the function iauApcs13 can be used instead of the
+   ephemeris, the function [iauApcs13][1] can be used instead of the
    present function.  This computes the Earth ephemeris using the
-   SOFA function iauEpv00.
+   SOFA function [iauEpv00][2].
 
 5) This is one of several functions that inserts into the astrom
    structure star-independent parameters needed for the chain of
@@ -122,7 +120,7 @@ SOFA (Standards of Fundamental Astronomy) software collection.
    transformation), and atmospheric refraction.
 
 6) The context structure astrom produced by this function is used by
-   iauAtciq* and iauAticq*.
+   [iauAtciq][14]* and [iauAticq][15]*.
 
 ## Called:
 ```
@@ -136,4 +134,9 @@ This revision:   2017 March 16
 
 SOFA release 2018-01-30
 
-Copyright (C) 2018 IAU SOFA Board.
+Copyright (C) 2018 IAU SOFA Board.
+
+[1]: iau.apcs13.md
+[2]: iau.epv00.md
+[14]: iau.atciq.md
+[15]: iau.aticq.md