J/ApJ/795/56     Experimental spectrum of methanol (CH3OH)   (McMillan+, 2014)

The complete, temperature resolved experimental spectrum of methanol (CH3OH) between 214.6 and 265.4 GHz. McMillan J.P., Fortman S.M., Neese C.F., De Lucia F.C. <Astrophys. J., 795, 56 (2014)> =2014ApJ...795...56M 2014ApJ...795...56M (SIMBAD/NED BibCode)
ADC_Keywords: Spectroscopy ; Atomic physics Keywords: astrochemistry - molecular data Abstract: The spectrum of methanol (CH3OH) has been characterized between 214.6 and 265.4 GHz for astrophysically significant temperatures. Four hundred and eighty-six spectra with absolute intensity calibration recorded between 240 and 389 K provided a means for the calculation of the complete experimental spectrum (CES) of methanol as a function of temperature. The CES includes contributions from vt=3 and other higher states that are difficult to model quantum mechanically (QM). It also includes the spectrum of the 13C isotopologue in terrestrial abundance. In general the QM models provide frequencies that are within 1 MHz of their experimental values, but there are several outliers that differ by tens of MHz. As in our recent work on methanol in the 560-654 GHz region, significant intensity differences between our experimental intensities and cataloged values were found. In this work these differences are explored in the context of several QM analyses. The experimental results presented here are analyzed to provide a frequency point-by-point catalog that is well suited for the simulation of crowded and overlapped spectra. Additionally, a catalog in the usual line frequency, line strength, and lower state energy format is provided. Description: In this paper we describe the spectrum of methanol between 214.6 and 265.4 GHz. In this region we observed 589 lines with scaled absorbance cross-sections greater than 0.0037 nm2. For comparison there are 386 lines in a composite catalog above this scaled absorbance cross-section. The spectrometer uses ax24 frequency multiplied probe, a heterodyne receiver, and a temperature controlled 6 m long cell (Fortman et al. 2010ApJ...725.1682F 2010ApJ...725.1682F, 2011ApJ...737...20F 2011ApJ...737...20F). Four hundred eighty-six spectral scans were recorded as the temperature was ramped over a period of 305 minutes from 240 K to 389 K. The spectrum was recorded at 24.4140625 kHz intervals, with an integration time of ∼18 us/bin. The temperatures were determined spectroscopically and are used as a part of the file name. The decontaminated absorbance spectra data are contained in 486 flat text files in this tarball. Each spectrum file contains 2.08 million data bins, starting at 214.6 GHz and incrementing in steps of 24.4140625 kHz. The frequency (in MHz) is provided in "tablefre.dat" and calibration data are provided in "tablecal.dat" File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 100 592 Line catalog tablecal.dat 20 486 Calibration Data tablefre.dat 17 2080000 Frequency in MHz for all scans sp/* . 485 Individual spectra for frequencies listed in tablefre.dat -------------------------------------------------------------------------------- See also: J/ApJ/782/75 : Complete spectrum of methanol (Fortman+, 2014) Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Snippet [0/556] Snippet Index 7- 10 A4 --- Ref Reference Index 12- 20 F9.5 D2 S Line Strength 22- 30 F9.5 D2 e_S Line Strength Uncertainty 32- 40 F9.3 cm-1 E Lower State Energy 42- 50 F9.3 cm-1 e_E Lower State Energy Uncertainty 52- 65 F14.6 MHz nu Frequency 67- 75 F9.6 MHz e_nu Frequency Uncertainty 77- 85 F9.6 MHz LW Lorentzian HWHM @ 300 K 87- 95 F9.6 MHz e_LW Lorentzian HWHM Uncertainty 97-100 I4 --- C13 Line attributed to Carbon-13 -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablecal.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I03 --- Index [0/485] Index of the Scan 6- 11 F6.2 K T Spectroscopic Temperature 12- 20 F9.5 nm-2 N Effective Column Density -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablefre.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 17 F17.10 MHz Freq Frequency -------------------------------------------------------------------------------- Byte-by-byte Description of file: sp/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Abs Napierian Absorbance spectra -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Tiphaine Pouvreau [CDS] 18-May-2017
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