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 atoms and molecules of astrophysical and atmospheric interest as well as some documentation on which data have atoms and molecules of astrophysical and atmospheric interest as well as some documentation on which data have
 been used for the predictions. At present, the aim of of this page is to supplement data bases such as the been used for the predictions. At present, the aim of of this page is to supplement data bases such as the
-[JPL catalog](http://spec.jpl.nasa.gov/ftp/pub/catalog/catform.html). Herb Pickett's programs **SPFIT** and+[[http://spec.jpl.nasa.gov/ftp/pub/catalog/catform.html|JPL catalog]]. Herb Pickett's programs **SPFIT** and
 **SPCAT** have been used for the most part to generate the predictions. **SPCAT** have been used for the most part to generate the predictions.
  
-After some general remark, a [brief description of the format of the catalog entries](description.html#description) +After some general remark, a brief description of the format of the catalog entries 
-follows below along with [remarks on the selection rules and assignments](description.html#selection), +follows below along with remarks on the selection rules and assignments, 
-[comments on the reliability of the predictions](description.html#reliable), +comments on the reliability of the predictions, 
-[remarks on the partition function](description.html#partition), and +remarks on the partition function, and 
-[some useful equations](description.html#equations).+some useful equations.
  
-[The structure of the files]{style="color:#f00090"} is described in detail in the Letter +**The structure of the files** is described in detail in the Letter 
-[THE COLOGNE DATABASE FOR MOLECULAR SPECTROSCOPY, CDMS](/classic/pdfs/CDMS_AA.pdf) by H. S. P. Müller,+[[https://cdms.astro.uni-koeln.de/classic/predictions/pdfs/CDMS_AA.pdf|THE COLOGNE DATABASE FOR MOLECULAR SPECTROSCOPY, CDMS]] 
 +by H. S. P. Müller,
 S. Thorwirth, D. A. Roth, and G. Winnewisser; *Astron. Astrophys.* **370** (2001) S. Thorwirth, D. A. Roth, and G. Winnewisser; *Astron. Astrophys.* **370** (2001)
 L49 – L52.\\ L49 – L52.\\
 An update on the CDMS appeared somewhat later: H. S. P. Müller, F. Schlöder, J. Stutzki, and G. Winnewisser, An update on the CDMS appeared somewhat later: H. S. P. Müller, F. Schlöder, J. Stutzki, and G. Winnewisser,
-[THE COLOGNE DATABASE FOR MOLECULAR SPECTROSCOPY, CDMS: A USEFUL TOOL FOR ASTRONOMERS AND +[[https://cdms.astro.uni-koeln.de/classic/predictions/pdfs/CDMS_JMSt.pdf|THE COLOGNE DATABASE FOR MOLECULAR SPECTROSCOPY, CDMS: A USEFUL TOOL FOR ASTRONOMERS AND 
-SPECTROSCOPISTS](/classic/pdfs/CDMS_JMSt.pdf), *J. Mol. Struct.* **742**, 215–227 (2005).+SPECTROSCOPISTS]], *J. Mol. Struct.* **742**, 215–227 (2005).
  
 Please acknowledge use of the CDMS by citing these articles. You are very welcome to state the web address Please acknowledge use of the CDMS by citing these articles. You are very welcome to state the web address
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 Information on background literature is desirable !! Information on background literature is desirable !!
  
-As in the JPL catalog, the species are sorted according to their molecular weight in atomic mass units, +As in the JPL catalog, the species are sorted according to their molecular weight in atomic mass units, which also constitutes the first three digits of the six digit **molecule tag** (with leading zeros frequently omitted), the fourth digit is a 5 (to avoid any conflict with the JPL numbering scheme), and the last two digits are used to number entries with the same molecular weight.
-which also constitutes the first three digits of the six digit +
-**molecule tag** (with leading zeros frequently omitted), the fourth digit is a +
-5 (to avoid any conflict with the JPL numbering scheme), and the last two digits are used to number entries +
-with the same molecular weight. +
- +
-> C. P. Endres, S. Schlemmer, P. Schilke, J. Stutzki, and H. S. P. Müller, **The Cologne Database for Molecular Spectroscopy, CDMS, in the Virtual Atomic and Molecular Data Centre, VAMDC** [J. Mol. Spectrosc. 327, 95–104 (2016)](http://dx.doi.org/10.1016/j.jms.2016.03.005) [Please visit also the VAMDC-compatible version of the CDMS](https://cdms.ph1.uni-koeln.de/cdms/portal/) +
- +
-> H. S. P. Müller, F. Schlöder, J. Stutzki, and G. Winnewisser, [*J. Mol. Struct.* **742**, 215–227 (2005)](http://dx.doi.org/10.1016/j.molstruc.2005.01.027) +
- +
-> H. S. P. Müller, S. Thorwirth, D. A. Roth, and G. Winnewisser, [*Astronomy and Astrophysics* **370,** L49–L52 (2001)](http://www.edpsciences.org/articles/aa/pdf/2001/18/aadb051.pdf) [[http://example.com|External Link]]+
  
 +<alert type="info">
 +  * C. P. Endres, S. Schlemmer, P. Schilke, J. Stutzki, and H. S. P. Müller, **The Cologne Database for Molecular Spectroscopy, CDMS, in the Virtual Atomic and Molecular Data Centre, VAMDC** [[https://doi.org/10.1016/j.jms.2016.03.005|J. Mol. Spectrosc. 327, 95–104 (2016)]]
 +  * H. S. P. Müller, F. Schlöder, J. Stutzki, and G. Winnewisser, [[https://doi.org/10.1016/j.molstruc.2005.01.027|J. Mol. Struct. 742, 215–227 (2005)]]
 +  * H. S. P. Müller, S. Thorwirth, D. A. Roth, and G. Winnewisser, [[https://doi.org/10.1051/0004-6361:20010367|Astronomy and Astrophysics 370, L49–L52 (2001)]]
 +</alert>
 ---- ----
  
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     Dr. Holger S. P. Müller     hspm(at)ph1(Dot)uni-koeln(Dot)de     Dr. Holger S. P. Müller     hspm(at)ph1(Dot)uni-koeln(Dot)de
-    Dr. Christian P. Endres     endres(at)ph1(Dot)uni-koeln(Dot)de +    Dr. Christian P. Endres     cendres(at)mpe(Dot)mpg(Dot)de 
-    Prof. Dr. Jürgen Stutzki    stutzki(at)ph1(Dot)uni-koeln(Dot)de+    Prof. Dr. Peter Schilke     schilke(at)ph1(Dot)uni-koeln(Dot)de
     Prof. Dr. Stephan Schlemmer schlemmer(at)ph1(Dot)uni-koeln(Dot)de     Prof. Dr. Stephan Schlemmer schlemmer(at)ph1(Dot)uni-koeln(Dot)de
  
 © 2019 by I.Physik © 2019 by I.Physik
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