Catalogs

  • The Collision Database (C. Vastel, 21. March 2025)
  • The aim of this database is to provide the community an up-to-date database on the collisional coefficients to be used with the RADEX radiative transfer modelling. These files are mandatory for the non-LTE modelling within CASSIS. To date there are three updated collision databases:

    The LAMDA database maintained by F. van der Tak at the Leiden University (Netherlands), the Basecol database maintained by M.-L. Dubernet at the Paris observatory (France) and the EMAA database. The LAMDA and EMAA database has the advantage to provide collision files directly used with the RADEX tool. The Basecol database does not generate files directly used with this tool. RADEX is implemented within the CASSIS software and CASSIS needs to address the quantum numbers associated with the molecular/atomic transitions to perform line identification and generate synthetic spectra for example.

    With this project I am trying to gather the most up-to-date collision files provided by LAMDA, BASECOL, and by the scientists feeding the databases (e.g. F. Lique, A. Faure). I then made those files compatible with their associated molecular database (JPL and/or CDMS) so that the quantum numbers, Einstein coefficients, upper energy levels and rest frequencies match. Indeed, some species may have less quantum numbers from database to another.

    Currently the database contains data for 76 molecular species. Several isotopomers and deuterated versions are also available. Work is currently underway to add more datafiles. We encourage comments from the users in order to improve and extend the database. Here is below the proposed collision files to be used in CASSIS. You can also use your own modified collision rates, but be careful to use the underscore symbol between the quantum numbers. Example:
    ! LEVEL + ENERGY(CM-1) + WEIGHT + QUANTUM NOS.
    1 0.0000 3.0 0 0 0
    2 2.1346 9.0 1 0 1
    should be :
    ! LEVEL + ENERGY(CM-1) + WEIGHT + QUANTUM NOS.
    1 0.0000 3.0 0_0_0
    2 2.1346 9.0 1_0_1

    Then, when using the LTE-RADEX modelling within CASSIS, select your file using Ctrl + left click under the "Collision" tab.

    The previous list of the collision files implemented in CASSIS5.0 can be found here.

CASSIS TAGSSpeciesCollision FileCollidersReferencesNotesCaveats
12501CC-H-e-H+-He-o-p-H2.datH, o-H2, p-H2, He, H+, eLaunay & Roueff (1977); Johnson, Burke, & Kingston 1987, JPhysB, 20, 2553; Roueff & Le Bourlot 1990, A&A, 236, 515; Staemmler, V., Flower, D.R. 1991, J. Phys. B, 24, 2343 Schroeder et al. 1991, J. Phys. B, 24, 2487From LAMDA, 13 Mar 2018T=[10-1200] K for o-p-H2
12503C+C+-o-p-H2-H-e.dato-H2, p-H2, H, eWiesenfeld & Goldsmith (2014), Lique et al. (2013), Barinovs et al. 2005, ApJ, 620, 537, Wilson & Bell, 2002, MNRAS, 337, 1027; Launay & Roueff, 1977, JPB, 10, 879; Flower & Launay (1977, JPB, 10, 3673)From LAMDA, 13 Mar 2018T=[10-500] K for o-p-H2
15501NHNH-He-scaled.datHe scaled (*1.3335)Dumouchel et al. (2012), Journal of Chemical Physics, Volume 137, Issue 11Provided by F. Lique (7 dec 2016)T=[5-150] K
15001NHNH-He-scaled.datHe scaled (*1.3335)Dumouchel et al. (2012), Journal of Chemical Physics, Volume 137, Issue 11Provided by F. Lique (7 dec 2016)T=[5-150] K
16001OO-o-pH2-H-H+-e-jpl.dato-H2, p-H2, H, H+, eLique et al. (2017), MNRAS 474, 2313Provided by F. Lique (6 nov 2017), adapted by CV for the 2 transitions in JPLT=[10-1000] K for o-p-H2
16502NDND-He-scaled.datHe scaled (*1.3335)ND-He rates from Dumouchel et al. (2012), unpublishedProvided by F. Lique (7 dec 2016), modified by CV 23 Aug 2017T=[5-150] K
17001OHOH-o-p-H2.datortho and para H2OH o-H2 and pH2 from Offer et al. (1994) + Offer priv. comm.Constructed by CV based on LAMDA, 4 Oct 2017T=[15-200] K
17082p-NH3p-NH3-pH2.datpara H2Danby et al 1988, MNRAS 235, 229From LAMDA, 25 Aug 2017T=[15-300] K
17092o-NH3o-NH3-pH2.datpara H2Danby et al 1988, MNRAS 235, 229From LAMDA, 25 Aug 2017T=[15-300] K
18083p-H2Op-H2O-o-p-H2-jpl.datortho and para H2pH2O - pH2 and pH2O - oH2 from Daniel et al. (2011), assuming thermal o/p for H2From LAMDA, 23 Aug 2017T=[5-1500] K
18093o-H2Oo-H2O-o-p-H2-jpl.datortho and para H2oH2O - pH2 and oH2O - oH2 from Daniel et al. (2011), assuming thermal o/p for H2From LAMDA, 23 Aug 2017T=[5-1500] K
18581p-NH2Dp-NH2D-o-p-H2.datortho and para H2oH2 and thermalized pH2 from Daniel et al (2014): oH2 is assumed similar to pH2 (j2 = 2)constructed by CV from LAMDA, 25 Aug 2017T=[5-300] K CV corrects the IDs for o and p H2 in the LAMDA file. Confirmation asked to Floris (and received) on August 25th, 2017
18591o-NH2Do-NH2D-o-p-H2.datortho and para H2oH2 and thermalized pH2 from Daniel et al (2014): oH2 is assumed similar to pH2 (j2 = 2)constructed by CV from LAMDA, 25 Aug 2017T=[5-300] K CV corrects the IDs for o and p H2 in the LAMDA file. Confirmation asked to Floris (and received) on August 25th, 2017
19002HDOHDO-o-p-H2-jpl.datortho and para H2Faure et al. (2012)From LAMDA, 23 Aug 2017T=[5-300] K
20002HFHF-o-p-H2-e-He.datortho and para H2, e and HeGuillon & Stoecklin (2012), Thummel et al. (1991), Reese et al. (2005)From LAMDA, 14 Mar 2018T=[10-300] K for H2
25001CCHC2H-He-scaled-e.datHe scaled (*1.36) and eSpielfiedel et al (2012), scaled by 1.36 from their rates with HeFrom LAMDA, 23 Aug 2017T=[5-100] K
25501CCHC2H-He-scaled-e.datHe scaled (*1.36) and eSpielfiedel et al (2012), scaled by 1.36 from their rates with HeFrom LAMDA, 23 Aug 2017T=[5-100] K
26504CNCN-pH2-cdms.datpara H2Kalugina et al. (2012), MNRAS, 422, 812constructed by CV December 6th, 2017 based on Basecol fileT =[5-100] K
27501HCNHCN-He-scaled-e-cdms.datHe scaled (*1.363) and eDumouchel et al. (2010)constructed by CV based on LAMDA file (April 2018)T=[5-500] and T=[5-800] K no HFS
27501HCNHCN-pH2-cdms.datpara H2Hernandez-Vera et al., J. Chem. Phys. vol140, 22, 2014constructed by CV April 19th, 2017 based on Basecol fileT=[5-100] K no HFS
27501HCNHCN-He-scaled-cdms.datHe scaled (*1.363)Green & Thaddeus (1974) + extrapolationconstructed by CV based on LAMDA, March 14, 2019T=[5-1200] K
27601HCNHCN-hfs-pH2-cdms-1.datpara H2Abdallah et al. MNRAS 419, 2441-2447, 2012constructed by CV April 17th, 2018 based on Basecol fileT=[5-100] K HFS
27601HCNHCN-hfs-pH2-cdms-2.datpara H2Hernandez-Vera et al., MNRAS 468, 1084, 2017constructed by CV April 2nd, 2019 based on LAMDA fileT=[5-30] K HFS
27502HNCHNC-o-p-H2-cdms.datortho and para H2Dumouchel, Klos & Lique Phys. Chem. Chem. Phys., 2011, 13, 8204-8212constructed by CV April 10th, 2017 based on files given by F. Dumouchel. Valid for CDMS databaseT=[5-100] K
27502HNCHNC-He-scaled-cdms.datHe scaled (*1.363)Dumouchel et al. (2010)From LamdaT=[5-500] K
28001COCO-o-p-H2.datortho and para H2Yang et al. (2010)from LAMDA, Aug 22, 2017T=[2-3000] K
28001COCO-high-J.datortho and para H2from Yang et al (2010) extrapolated by David Neufeld (13dec2010)from LAMDA, Aug 22, 2017T=[2-3000] K For High J transitions (J=80)
28503COCO-o-p-H2.datortho and para H2Yang et al. (2010)from LAMDA, Aug 22, 2017T=[2-3000] K
28503COCO-high-J.datortho and para H2from Yang et al (2010) extrapolated by David Neufeld (13dec2010)from LAMDA, Aug 22, 2017T=[2-3000] K For High J transitions (J=80)
28515HN13CHN13C-He-scaled-cdms.datHe scaled (*1.363)Dumouchel et al. (2010)Constructed by CV May 2nd 2017, using Lamda.T=[5-500] K
28515HN13CHN13C-o-p-H2-cdms.datortho and para H2Dumouchel, Klos & Lique Phys. Chem. Chem. Phys., 2011, 13, 8204-8212Constructed by CV May 3nd 2017, based on HNC files given by F. Dumouchel. Valid for CDMS databaseT=[5-100] K
28501H13CNH13CN-pH2-cdms.datpara H2Hernandez-Vera et al., J. Chem. Phys. vol140, 22, 2014constructed by CV April 26th, 2017 based on HCN fileT=[5-100] K
28506HC15NHC15N-p-H2-cdms.datpara H2Hernandez-Vera et al., J. Chem. Phys. vol140, 22, 2014constructed by CV April 26th, 2017 based on HCN fileT=[5-100] K
28508DNCDNC-o-p-H2-cdms.datortho and para H2Dumouchel, Klos & Lique Phys. Chem. Chem. Phys., 2011, 13, 8204-8212constructed by CV April 19th, 2017 based on HNC files given by F. Dumouchel. Valid for CDMS databaseT=[5-100] K
28508DNCDNC-He-scaled-cdms.datHe scaled (*1.363)Dumouchel et al. (2010)constructed by CV April 19th, 2017 based on HNC fileT=[5-500] K no HFS
28509DCNDCN-p-H2-cdms.datpara H2Hernandez-Vera et al., J. Chem. Phys. vol140, 22, 2014constructed by CV April 26th, 2017 based on HCN fileT=[5-100] K
2900113CO13CO-o-p-H2.datortho and para H2Yang et al. (2010)from LAMDA, Aug 23, 2017T=[2-3000] K
29002HCO+HCO+-H2-jpl.datH2Yazidi et al. MNRAS 441, 664-670 (2014)Given by F. Lique adapted to match the JPL spectroscopyT=[10-490] K
29006C17OC17O-o-p-H2.datortho and para H2Yang et al. (2010)from LAMDA, Aug 23, 2017T=[2-3000] K JPL only, as CDMS has HFS which LAMDA does not have
2950113CO13CO-o-p-H2.datortho and para H2Yang et al. (2010)from LAMDA, Aug 23, 2017T=[2-3000] K
29506N2H+N2H+-H2-cdms.datH2Schoier et al. A&A 432, 369 (2005)from LAMDA, Feb 14, 2018, but adapted by CV for the CDMS spectroscopyT=[10-2000] K
29507HCO+HCO+-H2-cdms.datH2Yazidi et al. MNRAS 441, 664-670 (2014)Given by F. Lique, adapted to match the CDMS spectroscopyT=[10-490] K
29507HCO+HCO+-xpol-H2-cdms.datH2Flower (1999) + extrapolation 10-2000KFrom LamdaT=[10-2000] K The Einstein coeff, frequencies and energy levels are different from JPL or CDMS
29510D13CND13CN-pH2-cdms.datpara H2Hernandez-Vera et al., J. Chem. Phys. vol140, 22, 2014constructed by CV April 26th, 2017 based on HCN fileT=[5-100] K
29511DC15NDC15N-pH2-cdms.datpara H2Hernandez-Vera et al., J. Chem. Phys. vol140, 22, 2014constructed by CV April 26th, 2017 based on HCN fileT=[5-100] K
29511DC15NDC15N-He-scaled-cdms.datHe scaled (*1.363)Dumouchel et al. (2010)constructed by EMT=[5-500] K
30001C18OC18O-o-p-H2.datortho and para H2Yang et al. (2010)from LAMDA, Aug 23, 2017T=[2-3000] K
30008NONO-He-scaled-jpl.datHe scaled (*1.4)Lique et al. (2009), A&A 493, 557constructed by CV December 5th, 2017 based on Lamda fileT=[10-300] K
30517NONO-He-scaled-cdms.datHe scaled (*1.4)Lique et al. (2009), A&A 493, 557from LAMDA, Dec 13, 2017, but adapted by CV for the CDMS spectroscopyT=[10-300] K
30502C18OC18O-o-p-H2.datortho and para H2Yang et al. (2010)from LAMDA, Aug 23, 2017T=[2-3000] K
30504H13CO+H13CO+-H2-cdms.datH2Yazidi et al. MNRAS 441, 664-670 (2014)constructed by CV April 26th, 2017 based on HCO+ fileT=[10-490] K
30504H13CO+H13CO+-xpol-H2-cdms.datH2Flower (1999) + extrapolation 10-2000Kconstructed by CV April 26th, 2017 based on HCO+ fileT=[10-2000] K
30505HC17O+HC17O+-H2-cdms.datH2Flower (1999) + extrapolation 10-2000Kfrom LAMDA, Aug 23, 2017T=[10-2000] K
30510DCO+DCO+-H2-cdms.datH2Flower (1999) + extrapolation 10-2000Kfrom LAMDA, Aug 23, 2017T=[10-2000] K
30581p-H2COp-H2CO-o-p-H2-cdms.datortho and para H2Wiesenfeld & Faure MNRAS (2013)from LAMDA, Aug 24, 2017T=[10-300] K
30591o-H2COo-H2CO-o-p-H2-cdms.datortho and para H2Wiesenfeld & Faure MNRAS (2013)from LAMDA, Aug 24, 2017T=[10-300] K
31506HC18O+HC18O+-H2-cdms.datH2Flower (1999) + extrapolation 10-2000Kfrom LAMDA, Aug 23, 2017T=[10-2000] K
31508D13CO+D13CO+-H2-cdms.datH2Flower (1999) + extrapolation 10-2000Kconstructed by CV Aug 23 2017 based on HCO+ fileT=[10-2000] K
32001O2O2-H2-jpl.datH2Lique et al. 2014Provided by F. Lique (7 dec 2016)T=[5-150] K
32083e-CH3OHe-CH3OH-pH2.datpara H2Rabli & Flower (2010)constructed by CV from LAMDA, Aug 24, 2017T=[10-200] K
32093a-CH3OHa-CH3OH-pH2.datpara H2Rabli & Flower (2010)constructed by CV from LAMDA, Aug 24, 2017T=[10-200] K
32584e-CH3OHe-CH3OH-col.datpara H2Rabli & Flower (2010)from EMAA, April 18, 2024T=[10-200] K
32594a-CH3OHa-CH3OH-col.datpara H2Rabli & Flower (2010) from EMAA, April 18, 2024T=[10-200] K
32508O2O2-H2-cdms.datH2Lique et al. 2014Provided by F. Lique (7 dec 2016)T=[5-150] K
34082p-H2Sp-H2S-o-p-H2.datortho and para H2p-H2S - oH2 and pH2 scaled from H2O-H2 (Daniel/Dubernet et al 2012)from LAMDA, Aug 23, 2017T=[5-1500] K
34092o-H2So-H2S-o-p-H2.datortho and para H2oH2O - pH2 from Dubernet et al (2009) and oH2O - oH2 from Daniel et al. (2011), assuming thermal o/p for H2, scaled to oH2Sfrom LAMDA, Aug 23, 2017T=[5-1500] K
34582p-H2Sp-H2S-o-p-H2-cdms.datortho and para H2Paul J. Dagdigian, accepted in MNRAS (2020)given by Paul, Avril 17th 2020T=[5-1500] K
34592o-H2So-H2S-o-p-H2-cdms.datortho and para H2Paul J. Dagdigian, accepted in MNRAS (2020)given by Paul, Avril 17th 2020T=[5-1500] K
36001HClHCl-o-p-H2.datortho and para H2Lanza et al. 2014constructed by CV from LAMDA, Mar 13, 2018T=[10-300]
38082p-c-C3H2p-c-C3H2-H2-jpl.datH2Chandra & Kegel (2000)from LAMDA, Aug 23, 2017T=[30-120] The Einstein A coefficients have been re-scaled using a dipole moment of 3.27 D
38092o-c-C3H2o-c-C3H2-H2-jpl.datH2Chandra & Kegel (2000)from LAMDA, Aug 23, 2017T=[30-120] The Einstein A coefficients have been re-scaled using a dipole moment of 3.27 D
38582p-c-C3H2p-c-C3H2-H2-cdmsH2Chandra & Kegel (2000)from LAMDA, Aug 23, 2017T=[30-120] The Einstein A coefficients have been re-scaled using a dipole moment of 3.27 D
38592o-c-C3H2o-c-C3H2-H2-cdms.datH2Chandra & Kegel (2000)from LAMDA, Aug 23, 2017T=[30-120] The Einstein A coefficients have been re-scaled using a dipole moment of 3.27 D
41001CH3CNCH3CN-H2-jpl.datH2S. Green 1986, ApJ 309, 331constructed by CV from LAMDA, Aug 24, 2017T=[20-500] K
41505CH3CNCH3CN-H2-cdms.datH2S. Green 1986, ApJ 309, 331constructed by CV from LAMDA, Aug 24, 2017T=[20-500] K to be tested with the new database. Update on nov 2016 with 3 quantum number instead of 2
43511HNCOHNCO-H2-o-pH2.datH2 (from Helium), para H2 and ortho H2Green, S. 1986, NASA Technical Memorandum 87791; Sahnoun, et al. 2018, Journal of Physical Chemistry A   Volume: 122   Issue: 11   Special Issue: SI   Pages: 3004-3012constructed by CV April 17th, 2018, based on a file given by L. Wiesenfeld (22 January 2018)T=[20-320], [7-300], [7-300] K
44001CSCS-He-scaled-jpl.datHe scaled (*1.363)Lique et al (2006)from LAMDA, Aug 23, 2017T=[10-300] K
44001CSCS-o-p-H2-jpl.datortho and para H2Denis-Alpizar et al. (2013)constructed by CV May 2nd 2018, based on file given by Otoniel Denis-AlpizarT=[5-305] K
44501CSCS-He-scaled-cdms.datHe scaled (*1.363)Lique et al (2006)constructed by CV on Aug 23, 2017, based on LAMDA fileT=[10-300] K
44501CSCS-o-p-H2-cdms.datortho and para H2Denis-Alpizar et al. (2013)constructed by CV May 2nd 2018, based on file given by Otoniel Denis-AlpizarT=[5-305] K
44505SiOSiO-He-scaled.datHe scaled (*1.38)Dayou & Balanca (2006) + extrapolationconstructed by CV from LAMDA, Aug 24, 2017T=[10-2000] K
4550113CS13CS-He-scaled-cdms.datHe scaled (*1.363)Lique et al (2006)constructed by CV on Mar 13, 2018 based on LAMDA CST=[10-300] K
4550429SiO29SiO-He-scaled.datHe scaled (*1.38)Dayou & Balanca (2006) + extrapolationconstructed by CV from LAMDA, Aug 24, 2017T=[10-2000] K
45506HCS+HCS+-H2.datH2adopting HCO+ - H2 from Flower (1999) + extrapolationfrom LAMDA, Aug 24, 2017T=[10-2000] K
46501C34SC34S-He-scaled-cdms.datHe scaled (*1.363)Lique et al (2006)constructed by CV on Mar 13, 2018 based on LAMDA CST=[10-300] K
46515NSNS-He-scaled-cdms.datHe scaled (*1.4)Lique and Klos 2016constructed by CV April 17th, 2018 based on collisions given by F. Lique (January 25th, 2018)T=[5-30] K
48001SOSO-He-scaled.datHe scaled (*1.363)Lique et al (2006)from LAMDA, Aug 23, 2017T=[60-300] K
48001SOSO-pH2.datpara H2Lique et al (2007)constructed by CV from BASECOL, Aug 23, 2017T=[5-50] K
48501SOSO-He-scaled.datHe scaled (*1.363)Lique et al (2006)from LAMDA, Aug 23, 2017T=[60-300] K
48501SOSO-pH2.datpara H2Lique et al (2007)constructed by CV from BASECOL, Aug 23, 2017T=[5-50] K
51501HC3NHC3N-o-p-H2-cdms.datortho and para H2Faure et al. 2016 MNRAS 460 2103Given by A. FaureT=[10-300] K
60001OCSOCS-H2.datH2Green & Chapman 1978 + extrapolationfrom LAMDA, Aug 23, 2017T=[10-500] K
60503OCSOCS-H2.datH2Green & Chapman 1978 + extrapolationfrom LAMDA, Aug 23, 2017T=[10-500] K
64502SO2SO2-He-scaled.datHe scaled (*1.39)Green 1995 + extrapolation from Schoier al. (2005)from LAMDA, Aug 23, 2017T=[10-375] K
64502SO2SO2-o-p-H2.datortho and para H2Cernicharo et al. 2011constructed by CV from BASECOL, Aug 23, 2017T=[5-30] K