The room temperature spectrum of carbon monoxide in natural isotopic abundance is recorded by Cavity Ring Down Spectroscopy between 8094 and 8317 cm−1. The investigated range covers the low frequency region of the third overtone band centered at 8414 cm−1. The achieved sensitivity of the recordings corresponds to a noise equivalent absorption, αmin~5×10–12 cm−1. 94 transitions are measured with intensity ranging between 3×10–27 and 1×10–30 cm/molecule. They include the first observation of (i) high J lines of the P branch of the 4-0 band of 12C16O, (ii) the 4-0 band of 13C16O and 12C18O present in natural abundance in the sample (35 and 38 transitions, respectively), (iii) a few lines of the 4-0 band of 12C17O and of the 5-1 hot band of 12C...
$^{h}$J.-P. Bouanich, D. Bermejo, J.L. Domenech, R.Z. Martinez, J. Mol. Spectrose. 179,22 (1996) $^{...
The room temperature absorption spectrum of 17O enriched carbon dioxide is investigated by high sens...
Three bands 4003i–00001 (i=2, 3, 4) of the Fermi pentad of 12C16O2 near 830 nm have been recorded wi...
The room temperature spectrum of carbon monoxide in natural isotopic abundance is recorded by Cavity...
International audienceThe room temperature spectrum of the very weak third overtone band of carbon m...
International audienceThe room temperature absorption spectrum of highly 18O enriched carbon dioxide...
We have measured several carbon monoxide transitions in the (3$rightarrow$0) and (4$rightarrow$1) ba...
The room temperature absorption spectrum of 18O enriched carbon dioxide has been recorded by very hi...
CO is the second most abundant molecule in the universe. Precise spectrum of the carbon monoxide mol...
International audienceThe absorption spectrum of highly enriched 13C carbon dioxide has been investi...
International audienceIn a previous contribution (Kassi S, Song KF, Campargue A. High sensitivity CW...
We have measured several carbon monoxide transitions in the (3$rightarrow$0) and (4$rightarrow$1) ba...
CO is the second most abundant molecule in the universe. Precise spectrum of the carbon monoxide mol...
doppler-free laser spectroscopy; perturbation analysis; carbon monoxide The (2,0) (3,0) and (4,0) ba...
The line parameters (line position, line intensity, self-broadening coefficient) of the 3-0 bands of...
$^{h}$J.-P. Bouanich, D. Bermejo, J.L. Domenech, R.Z. Martinez, J. Mol. Spectrose. 179,22 (1996) $^{...
The room temperature absorption spectrum of 17O enriched carbon dioxide is investigated by high sens...
Three bands 4003i–00001 (i=2, 3, 4) of the Fermi pentad of 12C16O2 near 830 nm have been recorded wi...
The room temperature spectrum of carbon monoxide in natural isotopic abundance is recorded by Cavity...
International audienceThe room temperature spectrum of the very weak third overtone band of carbon m...
International audienceThe room temperature absorption spectrum of highly 18O enriched carbon dioxide...
We have measured several carbon monoxide transitions in the (3$rightarrow$0) and (4$rightarrow$1) ba...
The room temperature absorption spectrum of 18O enriched carbon dioxide has been recorded by very hi...
CO is the second most abundant molecule in the universe. Precise spectrum of the carbon monoxide mol...
International audienceThe absorption spectrum of highly enriched 13C carbon dioxide has been investi...
International audienceIn a previous contribution (Kassi S, Song KF, Campargue A. High sensitivity CW...
We have measured several carbon monoxide transitions in the (3$rightarrow$0) and (4$rightarrow$1) ba...
CO is the second most abundant molecule in the universe. Precise spectrum of the carbon monoxide mol...
doppler-free laser spectroscopy; perturbation analysis; carbon monoxide The (2,0) (3,0) and (4,0) ba...
The line parameters (line position, line intensity, self-broadening coefficient) of the 3-0 bands of...
$^{h}$J.-P. Bouanich, D. Bermejo, J.L. Domenech, R.Z. Martinez, J. Mol. Spectrose. 179,22 (1996) $^{...
The room temperature absorption spectrum of 17O enriched carbon dioxide is investigated by high sens...
Three bands 4003i–00001 (i=2, 3, 4) of the Fermi pentad of 12C16O2 near 830 nm have been recorded wi...