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DJAMEL BOUDJAADAR, Laboratoire de Recherche sur la Physico-Chimie des Surfaces et Interfaces, Université de Skikda, BP 26, Skikda 21000, Algeria; JEAN-YVES MANDIN, VICTOR DANA, Laboratoire de Physique Moléculaire et Applications, CNRS, case courrier 76, Université Pierre-et-Marie-Curie, 75252 Paris Cedex 05, France; LAURENCE RÉGALIA-JARLOT, XAVIER THOMAS, PIERRE VON DER HEYDEN, Groupe de Spectrométrie Moléculaire et Atmosphérique, CNRS, UMR 6089, Université de Reims-Champagne-Ardenne, Faculté des Sciences, BP 1039, 51687 Reims Cedex 2, France; GUY GUELACHVILI AND NATHALIE PICQUÉ, Laboratoire de Photophysique Moléculaire, Unité Propre du C.N.R.S., Bâtiment 350, Université de Paris-Sud, 91405 Orsay, France, email: nathalie.picque@ppm.u-psud.fr .
Using Fourier transform spectra (FTS) and a multispectrum fitting procedure, 395 absolute line intensities of 12C16O2 have been measured between 6035 and 6950 cm-1, for the 4 cold bands 30014-00001, 30013-00001, 30012-00001, and 30011-00001, and for the 3 hot bands 31113-01101, 31112-01101, and 01131-01101. Vibrational transition dipole moments and Herman-Wallis coefficients are reported for each band. Comparisons are made with previous experimental results and with data available in the HITRAN database and the Carbon Dioxide Spectroscopic Databank (CDSD).
Comparisons with experimental line intensities recently obtained from FTS for the 2 bands 30013-00001 and 30012-00001 are also performed. They show a very good line by line agreement: (0.3 \pm 0.6) % on the mean for a hundred of lines, with a maximum discrepancy 1.6 %. Thus, the accuracy of these sets of individual line intensities, which was originally estimated about 3 % on the average in both works, is likely better than 1%. This is close to what is needed by some atmospheric experiments, as OCO.