J/MNRAS/461/1012    ExoMol line lists for H216O2             (Al-Refaie+, 2016)

ExoMol line lists. XV: A new hot line list for hydrogen peroxide. Al-Refaie A.F., Polyansky O.L., Tennyson J., Yurchenko S.N. <Mon. Not. R. Astron. Soc. 461, 1012 (2016)> =2016MNRAS.461.1012A 2016MNRAS.461.1012A (SIMBAD/NED BibCode)
ADC_Keywords: Atomic physics Keywords: molecular data - opacity - astronomical data bases: miscellaneous - planets and satellites: atmospheres Abstract: A computed line list for hydrogen peroxide, H216O2, applicable to temperatures up to T=1250K is presented. A semi-empirical high accuracy potential energy surface is constructed and used with an ab initio dipole moment surface as input TROVE to compute 7.5 million rotational-vibrational states and around 20 billion transitions with associated Einstein-A coefficients for rotational excitations up to J=85. The result- ing APTY line list is complete for wavenumbers below 6000cm-1 (wavelength <1.67um) and temperatures up to 1250K. Room-temperature spectra are compared with laboratory measurements and data currently available in the HITRAN database and literature. Our rms with line positions from the literature is 0.152cm-1 and our absolute intensities agree better than 10%. Description: The data are in two parts. The first, h2o20-85.dat contains a list of 7,560,352 rovibrational states. Each state is labelled with: six normal mode vibrational quantum numbers the torsional symmetry number (tau) and the vibrational symmetry; three rotational quantum numbers including the total angular momentum J and rotational symmetry; the total symmetry quantum number Gamma and the running number in the same J,Gamma block. In addition there are six local mode vibrational numbers and the largest coefficient used to assign the state in question. 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 60 separate files, each containing all the transitions in a 100cm-1 frequency range. These and their contents are ordered by increasing frequency. The name of the file includes the lowest frequency in the range; thus the a-0500.dat file contains all the transitions in the frequency range 500-600cm-1. The transition files contain three columns: the reference number in the energy file of the upper state; that of the lower state; and the Einstein A coefficient of the transition. The energy file and the transitions files are zipped, and need to be extracted before use. There is a Fortran 90 programme, s_APTY.f90 which may be used to generate synthetic spectra (see s_APTY.txt for details). Using this, it is possible to generate absorption or emission spectra in either 'stick' form or else cross-sections convoluted with a gaussian with the half-width at half maximum being specified by the user, or with a the temperature-dependent doppler half-width. Sample input files s_*.inp for use with s_APTY.f90 are supplied. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file h2o20-85.dat 150 7560352 Labelled rovibrational states (h2o2_0-85.dat) s_apty.f90 172 585 Programme for generating spectra s_sti750.inp 177 76 Illustration of 'stick' input file s_dop296.inp 173 76 Illustration of 'doppl' input file s_gau296.inp 175 76 Illustration of 'gauss' input file s_bin750.inp 175 76 Illustration of 'bin' input file s_pfu296.inp 175 76 Illustration of 'partfunc' input file s_stick296.inp 175 76 Illustration of 'stick' input file s_apty.txt 207 88 Explanation of input structure for s_APTY.f90 trans/* . 60 Individual transition files -------------------------------------------------------------------------------- See also: J/MNRAS/425/34 : ExoMol line lists for BeH, MgH and CaH (Yadin+, 2012) J/MNRAS/434/1469 : ExoMol line lists for SiO (Barton+, 2013) J/MNRAS/437/1828 : ExoMol line list for HCN and HNC (Barber+, 2014) J/MNRAS/440/1649 : ExoMol line lists for CH4 (Yurchenko+, 2014) J/MNRAS/442/1821 : ExoMol line list for KCl (Barton+, 2014) J/MNRAS/445/1383 : ExoMol line list for phosphorus nitride (PN) (Yorke+, 2014) J/MNRAS/446/2337 : ExoMol line lists for phosphine (PH3) (Sousa-Silva+, 2015) J/MNRAS/448/1704 : ExoMol line lists for formaldehyde H2CO (Al-Refaie+, 2015) J/MNRAS/449/3613 : ExoMol line lists for AlO (Patrascu+, 2015) J/MNRAS/451/634 : ExoMol line lists for NaH and NaD (Rivlin+, 2015) J/MNRAS/456/4524 : ExoMol line lists for CaO (Yurchenko+, 2016) Byte-by-byte Description of file: h2o20-85.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 35- 40 I6 --- J [0/85] J-quantum number J$ is the total angular momentum excluding nuclear spin 41- 55 D15.4 s L ?=-1 Lifetime in seconds (1) 58- 62 I5 --- G [1/8] Total symmetry in D2h(M), Gamma = A1g,A1u,B1g,B1u,B2g,B2u,B3g,B3u 64- 66 I3 --- v1 [0/10] normal mode vibrational quantum number 68- 70 I3 --- v2 [0/14] normal mode vibrational quantum number 72- 74 I3 --- v3 [0/14] normal mode vibrational quantum number 76- 78 I3 --- v4 [0/10] torsional excitation quantum number 80- 82 I3 --- v5 [0/10] normal mode vibrational quantum number 84- 86 I3 --- v6 [0/14] normal mode vibrational quantum number 87- 89 I3 --- t [0/10] torsional symmetry number 91- 93 I3 --- Gv [1/8] D2h(M) vi. symmetry Gamma(v) (local mode) 96- 98 I3 --- K [0/70] Projection of J on axis of molec. symmetry 101-103 I3 --- Pr [0/1] Rotational parity 106-110 I5 --- Gr [1/8] D2h(M) rot. symmetry Gamma(v) (local mode) 112-119 I8 --- N(Bl) [1/67238] Reference number in the polyad 123-126 F4.2 --- C2 [0.0/1.00] Square of the largest coefficient 128-130 I3 --- n1 [0/14] Local mode vibrational quantum number 132-134 I3 --- n2 [0/10] Local mode vibrational quantum number 136-138 I3 --- n3 [0/10] Local mode vibrational quantum number 140-142 I3 --- n4 [0/14] Local mode vibrational quantum number 144-146 I3 --- n5 [0/14] Local mode vibrational quantum number 148-150 I3 --- n6 [0/42] Local mode vibrational quantum number -------------------------------------------------------------------------------- Note (1): If less than 0 (i.e. -1) then it is considered infinite or 'inf'. If E (energy) is >6000cm-1 then L is incomplete and should be considered as 'nan'. ------------------------------------------------------------------------------- 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: Ahmed F. Al-Refaie, ahmed.al-refaie.12(at)ucl.ac.uk
(End) Ahmed F. Al-Refaie [UCL], Patricia Vannier [CDS] 06-Jun-2016
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