The Cologne Database for Molecular Spectroscopy, CDMS: a useful tool for astronomers and spectroscopists

By H. S. P. Müller, F. Schlöder, J. Stutzki, G. Winnewisser. 2005

1,481 citations recorded by the source corpus.

Subfields: Atmospheric Science, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/beee127206f3b1e2ffdff9dfa14ff1ab6743c574

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Atmospheric Science

In Spectroscopy

Citations in the corpus

ALMA OBSERVATIONS OF CIRCUMSTELLAR DISKS IN THE UPPER SCORPIUS OB ASSOCIATION (2016, background): “Aul is the Einstein A coefficient and Eu is the energy of the upper level of the transition (Aul = 2.497× 10−6 s−1 and Euk = 33.19 K for 12CO J = 3−2, Müller et al. 2001, 2005).”
The GEISA spectroscopic database: Current and future archive for Earth and planetary atmosphere studies (2008, neutral): “doc), and the CDMS database [96,97] (http://www.”
Increased complexity in interstellar chemistry: detection and chemical modeling of ethyl formate and n-propyl cyanide in Sagittarius B2(N) (2009, methodology): “The predictions used for the current analysis will be made available in the CDMS (Müller et al. 2001, 2005, see footnote 4).”
Astrochemistry and compositions of planetary systems (2020, background): “Yet data-bases are far from complete, especially for isotopologues of common interstellar molecules (Müller et al. 2005).”
MARVEL: Measured active rotational–vibrational energy levels. II. Algorithmic improvements☆ (2012, background): “The emphasis of the present paper is on the accumulation, validation, handling, visualization, and distribution of the increasing amount of such spectroscopic information on molecular systems [19–28].”
The Galactic Center: The Largest Oxygen-bearing Organic Molecule Repository (2007, methodology): “They were obtained from the Cologne Database for Molecular Spectroscopy (Müller et al. 2001, 2005), the Jet Propulsion Laboratory catalog (Pickett et al. 1998), and Hollis et al. (2004b).”
The 2009 edition of the GEISA spectroscopic database (2011, methodology): “H2CO (molecule 21) Formaldehyde has been completely revised in the microwave and far infrared using the line list of positions and intensities from the CDMS database [18,19] for the three isotopologues present in GEISA, namely H2(12)C(16)O, H2(12)C(18)O, and H2(13)C(16)O.”
Complex organic molecules in the interstellar medium: IRAM 30 m line survey of Sagittarius B2(N) and (M) (2013, methodology): “…are taken from our line catalog which contains all entri s from the catalog of the Cologne Database for Molecular Spectroscopy (CDMS4, see Müller et al. 2001, 2005) and most entries from the molecular spectroscopic database of the Jet Propulsi n Laboratory (JPL5, see Pickett et al.…”
Astronomical identification of CN^-, the smallest observed molecular anion (2010, background): “The only plausible molecule with a transition within 2 MHz of the observed frequency, according to the line catalogs of J. Cernicharo, CDMS (Müller et al., 2005), and JPL (Pickett et al., 1998), is13CCH, whoseNJ,F1,F = 47/2,4,7/2-37/2,4,7/2 transition lies at 336775.7 MHz.”
Our astrochemical heritage (2012, methodology): “ in the following databases: { Spectroscopic databases: + JPL Molecular spectroscopy database ([348]): http://spec.jpl.nasa.gov/home.html + Cologne Database for Molecular Spectroscopy database (CDMS, [308]): http://www.astro.uni-koeln.de/cdms/ + Splatalogue database for astronomical spectroscopy (SP”
The 2015 edition of the GEISA spectroscopic database (2016, methodology): “As commented in the GEISA-2011 [11] SO2 update description, “It is worthwhile mentioning that the CDMS catalog [18,19] provides an entry for ν2 which is based on extensive rotational transitions in its v2=0 and 1 states [175] along with previous IR data”, this entry has been, consequently, taken as ”
Interstellar OH+, H2O+ and H3O+ along the sight-line to G10.6–0.4 (2010, methodology): “Müller et al (2005) have published a global fit using these data which is available in the Cologne Data base for Molecular Spectroscopy (CDMS).”
Molecules with ALMA at Planet-forming Scales (MAPS). I. Program Overview and Highlights (2021, neutral): “…F=3–2 265.886434 −3.1292 7.0 25.5 CDMS Y Y Y Y Y J=3–2, F=3–3 265.884891 −4.0322 7.0 25.5 CDMS Y Y Y Y Y J=3–2, F=2–2 265.888522 −3.8861 5.0 25.5 CDMS Y Y Y Y Y 1 Spectroscopic data are compiled from the CDMS (Müller et al. 2001, 2005; Endres et al. 2016); JPL (Pickett et al. 1998); and LAMBDA…”
PGOPHER: A program for simulating rotational, vibrational and electronic spectra (2017, methodology): “MHz/(molecule nm(2)) as used by the JPL catalogue[29] and the CDMS database[30] is also an option (IntensityUnits = nm2MHzperMolecule).”