J/MNRAS/490/4638    ExoMol molecular line lists. XXXV. NH3        (Coles+, 2019)

ExoMol molecular line lists. XXXV: A rotation-vibration line list for hot ammonia. Coles P.A., Yurchenko S.N., Tennyson J. <Mon. Not. R. Astron. Soc. 490, 4638 (2019)> =2019MNRAS.490.4638C 2019MNRAS.490.4638C (SIMBAD/NED BibCode)
ADC_Keywords: Atomic physics Keywords: molecular data - opacity - astronomical data bases: miscellaneous - planets and satellites: atmospheres - brown dwarfs - stars: low-mass Abstract: A new hot line list for 14NH3 is presented. The line list CoYuTe was constructed using an accurate, empirically refined potential energy surface and a CCSD(T)/aug-cc-pVQZ ab initio dipole moment surface of ammonia, previously reported. The line list is an improvement of the ammonia line list BYTe (Yurchenko et al., 2011MNRAS.413.1828Y 2011MNRAS.413.1828Y, Cat. VI/133). The CoYuTe line list covers wavenumbers up to 20000cm-1, i.e. wavelengths above 0.5 um for temperatures up to 1500K. Comparisons with the high temperature experimental data from the literature show excellent agreement for wavenubmers below 6000cm-1. The CoYuTe line list contains 16.9 billion transitions. Description: The states file st-nh3.dat (14N-1H3CoYoTe.states) contains a list of rovibrational states. Each state is labelled with normal as well TROVE local mode vibrational quantum numbers and the vibrational symmetry; three rotational quantum numbers including the total angular momentum J and rotational symmetry; the total symmetry quantum number Gamma. Each rovibrational state has a unique number, which is the number of the row in which it appears in the file. This number is the means by which the state is related to the second part of the data system, the transitions files. The total degeneracy is also given to facilitate the intensity calculations. Because of their size, the transitions are listed in 200 separate files, each containing all the transitions in a 100cm-1 frequency range. These transition files 14N-1H3CoYoTe*.trans contain the Ammonia lines consisting of three columns: the reference number in the energy file of the upper state, that of the lower state, the Einstein A coefficient of the transition and the transition wavenumber. These entries are ordered by increasing frequency. The name of the file includes the lowest frequency in the range; thus the 14N-1H3CoYuTe00500-00600.trans file contains all the transitions in the frequency range 500-600cm-1. The energy file and the transitions files are bzipped, and need to be extracted before use. A programme ExoCross to generate synthetic spectra from these line lists can be obtained at www.exomol.com. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file st-14nh3.dat 156 5095730 Labelled ro-vibrational states for 14NH3 pf-nh3.dat 24 2000 Partition function for NH3 trans/* . 200 Transition files for 14NH3 -------------------------------------------------------------------------------- See also: VI/133 : A variationally computed hot NH3 line list - BYTe (Yurchenko+, 2011) Byte-by-byte Description of file: st-14nh3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 I12 --- i State ID, non-negative integer index, starting at 1 14- 25 F12.6 cm-1 E State energy term value in cm-1 27- 32 I6 --- g Total state degeneracy 34- 40 I7 --- J [0/43] J-quantum number J$ is the total angular momentum excluding nuclear spin 42 A1 --- p [-/+] Total inversion parity of the state 45 I1 --- G [1/6] Total symmetry in D3h(M), Gamma=1,2,3,4,5,6=A1',A2',E',A1",A2",E" 49- 56 I8 --- NN Counting number in the (J,Gamma) block 60- 63 I4 --- n1a Symmetric stretch quantum number (normal mode) 64- 67 I4 --- n2a Symmetric bend quantum number (normal mode) 68- 71 I4 --- n3a Asymmetric stretch quantum number (normal mode) 72- 75 I4 --- n4a Asymmetric bend quantum number (normal mode) 78- 81 I4 --- n5a Asymmetric stretch vibrarional angular momentum QN (normal mode) 83- 85 I3 --- n6a Asymmetric bend vibrarional angular momentum QN (normal mode) 89- 90 I2 --- n7a Inversion parity (0 or 1) 95- 97 I3 --- J2 Total angular momentum 99-101 I3 --- K Projection of $J$ on molecular symmetry axis 103-105 I3 --- Pr Rotational parity (0 or 1) 110-112 I3 --- n1b Local mode stretching QN 113-116 I4 --- n2b Local mode stretching QN 117-120 I4 --- n3b Local mode stretching QN 121-124 I4 --- n4b Local mode asymetric bending QN 125-128 I4 --- n5b Local mode asymetric bending QN 129-132 I4 --- n6b Local mode torsional QN 137-138 I2 --- Gv Vibrational symmetry (local mode) 145-156 F12.6 cm-1 ET TROVE energy term value if subsituted with MARVEL otherwise -1.000000 -------------------------------------------------------------------------------- Byte-by-byte Description of file: pf-nh3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 F8.1 K T Temperature in Kelvin 10- 24 F15.4 --- Q Parition function -------------------------------------------------------------------------------- Byte-by-byte Description of file: trans/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 I12 --- i" Upper state ID 14- 25 I12 --- i' Lower state ID 27- 36 E10.4 s-1 A Einstein A-coefficient of the transition ------------------------------------------------------------------------------- Acknowledgements: S.N. Yurchenko, s.yurchenko(at)ucl.ac.uk J. Tennyson, j.tennyson(at)ucl.ac.uk
(End) Patricia Vannier [CDS] 03-Nov-2019
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line