J/A+A/549/A38     Millimetre and infrared spectrum of DC4H  (Tamassia+, 2013)

Accurate ro-vibrational rest frequencies of DC4H at infrared and millimetre wavelengths. Tamassia F., Bizzocchi L., Degli Esposti C., Dore L., Di Lauro M., Fusina L., Villa M., Cane E. <Astron. Astrophys. 549, A38 (2013)> =2013A&A...549A..38T 2013A&A...549A..38T
ADC_Keywords: Atomic physics Keywords: ISM: molecules - line: identification - molecular data - molecular processes - infrared: ISM Abstract: Diacetylene, C4H2, has been identified in several astronomical environments through its infrared spectrum. In contrast, monodeuterated diacetylene (DC4H) has not been detected in space so far owing to the low isotopic abundance of deuterated species but also to the rather poor laboratory spectroscopic characterisation of this molecule. The aim of this work is to provide accurate spectroscopic parameters for DC4H to achieve reliable predictions for both its spectra at millimetre and infrared wavelengths. We studied the rotational spectrum of DC4H in the range 85-615GHz by millimetre-wave spectroscopy and the infrared spectrum below 1000cm-1 by high-resolution, Fourier-transform spectroscopy. Several pure rotational transitions were recorded in the ground state and in excited vibrational bending states. The three fundamental bands v6, v7, and v8 have been identified and assigned in the infrared spectrum. Description: The table contains the measured and predicted line positions, quantum numbers, estimated 1σ uncertainties, and line strengths for millimetre and infrared transitions of DC4H. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table4.dat 99 2147 Measured and predicted line positions -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 4 I3 --- J' [1/120] Upper level J quantum number 8- 9 I2 --- l' [0/1] Upper level l quantum number 14 A1 --- p' [ef] Upper level e(-)/f(+) parity 18- 19 I2 --- v' [0/9] Upper level v quantum number 21- 23 I3 --- J [0/120] Lower level J quantum number 27- 28 I2 --- l [0/1] Lower level l quantum number 33 A1 --- p [ef] Lower level e(-)/f(+) parity 37- 38 I2 --- v [0/9] Lower level v quantum number 42- 52 F11.4 --- RFmeas ?=- Measured line position (in rest frame) (2) 54- 58 F5.4 --- e_RFmeas ? Assumed uncertainties (2) 61- 73 F13.6 --- RFpred Predicted line position (in rest frame) (2) 77- 83 E7.5 --- e_RFpred Estimated 1σ level error (2) 86- 89 A4 --- x_RF Units for RFmeas, RFunc, RFpred and sigma (2) 91- 99 F9.3 --- S Transition strength -------------------------------------------------------------------------------- Note (2): the line positions are * either wavenumbers expressed in cm-1 (when x_RF="cm-1") * or frequencies expressed in MHz (when x_RF="MHz") ------------------------------------------------------------------------------ Acknowledgements: Filippo Tamassia, filippo.tamassia(at)unibo.it
(End) Patricia Vannier [CDS] 14-Nov-2012
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