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+The directory contains input data for two test cases.
+The first one is computing a spectrum for a 
+Kurucz model, Teff=9750 K, log g = 4, for a short wavelength 
+range between 1400 and 1410 A.
+
+In order to be able to use the script file RSynspec, one needs to
+copy the original Kurucz model file (ap00t9750g40k2.dat), and the
+standard input file (tab.5) to the name with a common core name,
+in this case kurucz9750g40, as it is done in the script file R1.
+The spectrum is computed with atomic lines only.
+
+Without using the script R1, the same model can be run as:
+
+ln -s -f $TLUSTY/data data
+ln -s -f data/linelist.test fort.19
+cp ap00t9750g40k2.dat fort.8
+$TLUSTY/synspec/synspec.exe < tab.5 > kurucz9750g40.log
+cp fort.7 kurucz9750g40.spec
+cp fort.17 kurucz9750g40.cont
+cp fort.12 kurucz9750g40.eqws
+
+One can similarly run a spectrum for a pure continuum (plus
+hydrogen lines), as first copying fort.55.con to fort.55
+
+cp fort.55.con fort.55
+$TLUSTY/synspec/synspec.exe < tab.5 > tmp.log
+
+This is mentioned just for completeness, but is not
+a part of the test case.
+
+
+The second test is computing a spectrum between 2500 and 7500 A
+for a solar-type star, Teff=5500 K, log g = 4.5, taking into
+account three line lists, all in the binary format: gfATO.bin (atomic), 
+gfMOL.bin (diatomic molecules), and gfTiO.bin (TiO).
+The model core name is kur55g45.
+The standard input file, tab.5, is almost identical to cool.5 used
+iun the previous test, but contains the keyword parameter file 
+(tab.nst) that sets generating four output files with interesting 
+parameters pertaining to the equation of state, fort.51 - 54. 
+These files are explained in detail in Paper IV (manual), Sec.3.3.