@article{97deaae584a7444a9174d50f89abb53b,
title = "VIS and VUV spectroscopy of 12C17O and deperturbation analysis of the A1Π, ν = 1-5 levels",
abstract = "High-accuracy dispersive optical spectroscopy measurements in the visible (VIS) region have been performed on the less-abundant 12C17O isotopologue, observing high-resolution emission bands of the B1Σ+ (ν = 0) → A1Π (ν = 3, 4, and 5) {\AA}ngstr{\"o}m system. These are combined with high-resolution photoabsorption measurements of the 12C17O B1Σ+ (ν = 0) ← X1Σ+ (ν = 0) and C1Σ+ (ν = 0) ← X1Σ+ (ν = 0) Hopfield-Birge bands recorded with the vacuum-ultraviolet (VUV) Fourier transform spectrometer, installed on the DESIRS beamline at the SOLEIL synchrotron. The frequencies of 429 observed transitions have been determined in the 15 100-18 400 cm-1 and 86 900-92 100 cm-1 regions with an absolute accuracy of up to 0.003 cm-1 and 0.005 cm-1 for the B-A, and B-X, C-X systems, respectively. These new experimental data were combined with data from the previously analysed C → A and B → A systems. The comprehensive data set, 982 spectral lines belonging to 12 bands, was included in a deperturbation analysis of the A1Π, ν = 1-5 levels of 12C17O, taking into account interactions with levels in the d3Δi, e3Σ-, a′3Σ+, I1Σ- and D1Δ states. The A1Π and perturber states were described in terms of a set of deperturbed molecular constants, spin-orbit and L-uncoupling interaction parameters, equilibrium constants, 309 term values, as well as isotopologue-independent spin-orbit and rotation-electronic perturbation parameters.",
author = "R. Hakalla and Niu, {M. L.} and Field, {R. W.} and Salumbides, {E. J.} and Heays, {A. N.} and G. Stark and James Lyons and M. Eidelsberg and Lemaire, {J. L.} and Federman, {S. R.} and M. Zachwieja and W. Szajna and P. Kolek and I. Piotrowska and M. Ostrowska-Kope{\'c} and R. Kepa and {De Oliveira}, N. and W. Ubachs",
note = "Funding Information: R. Hakalla expresses his gratitude to the LASERLAB-EUROPE for support of this research (grant no. 284464 within the EC's Seventh Framework Programme). R. W. Field thanks the US National Science Foundation (grant no. CHE-1361865) for support of this research. A. Heays was supported by grant no. 648.000.002 from the Netherlands Organisation for Scientific Research (NWO) via the Dutch Astrochemistry Network. J. Lyons and G. Stark acknowledge support from the NASA Origins program. S. Federman was supported by NASA grants NNG 06-GG70G and NNX10AD80G to the University of Toledo. We are grateful to the general and technical staff of SOLEIL synchrotron for providing beam time under projects no. 20090021, 20100018, 20110121, and 20120653. The Rzesz{\'o}w group would like to express their gratitude for the support of the European Regional Development Fund and the Polish state budget within the framework of the Carpathian Regional Operational Programme (RPPK.01.03.00-18-001/10) for the period of 2007-2013 through the funding of the Centre for Innovation and Transfer of Natural Science and Engineering Knowledge of the University of Rzesz{\'o}w. Publisher Copyright: {\textcopyright} The Royal Society of Chemistry 2016.",
year = "2016",
doi = "10.1039/c6ra01358a",
language = "English (US)",
volume = "6",
pages = "31588--31606",
journal = "RSC Advances",
issn = "2046-2069",
publisher = "Royal Society of Chemistry",
number = "38",
}