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-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]]
-The files in the [[/classic/entries|Entries section]] contain predictions
-for 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 [JPL
-catalog](http://spec.jpl.nasa.gov/ftp/pub/catalog/catform.html). Herb
-Pickett's programs **SPFIT** and **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) follows below along with
-[remarks on the selection rules and
-assignments](description.html#selection), [comments on the reliability
-of the predictions](description.html#reliable), [remarks on the
-partition function](description.html#partition), and [some useful
-equations](description.html#equations).
-[The structure of the files]{style="color:#f00090"} is described in
-detail in the Letter [THE COLOGNE DATABASE FOR MOLECULAR SPECTROSCOPY,
-CDMS](/classic/pdfs/CDMS_AA.pdf) by H. S. P. Müller, S. Thorwirth, D. A.
-Roth, and G. Winnewisser; *Astron. Astrophys.* **370** (2001) L49 –
-L52.\
-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
-SPECTROSCOPISTS](/classic/pdfs/CDMS_JMSt.pdf), *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 also. We recommend to cite the
-original sources of the data too, which are given in the documentations,
-at least as far as this is feasible. Since the format in the CDMS
-catalog is identical to the one in the JPL catalog information can also
-be found in the article SUBMILLIMETER, MILLIMETER, AND MICROWAVE
-SPECTRAL LINE CATALOG by H. M. Pickett, R. L. Poynter, E. A. Cohen, M.
-L. Delitsky, J. C. Pearson, and H. S. P. Müller; *J. Quant. Spectrosc.
-Radiat. Transfer* **60** (1998) 883 – 890.
-Some catalog entries are available with frequencies in units of cm^–1^.
-This applies mainly to light hydrides and some stable molecules that
-might be of interest as secondary standards in the laboratory or in
-radioastronomical observations.
-[Vibration-rotation transitions]{style="color:#f00090"} in the
-far-infrared region have been included for C~3~. They may be included in
-a greater number in the near future. Vibration-rotation transitions in
-the mid-infrared region are currently not considered to be included in
-the database. If there is a genuine interest for such information to be
-included in our database please use the [comments and
-suggestions]{style="color:#f00090"} option below in order to suggest
-species. Information on background literature is desirable !!
-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]{style="color:#ff9000"}**
-(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.
-----
-Comments and suggestions are very welcome. Please send an email to one of the following persons:
-    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
-    Prof. Dr. Jürgen Stutzki    stutzki(at)ph1(Dot)uni-koeln(Dot)de
-    Prof. Dr. Stephan Schlemmer schlemmer(at)ph1(Dot)uni-koeln(Dot)de
-© 2019 by I.Physik