Theoretically predicted CO2 lines near 700 nm not observed

Authors:Balashov, Aleksandr – ORCID: 0000-0001-9537-1805 – Nicolaus Copernicus University – ROR: https://ror.org/0102mm775Raj, Ankit – ORCID: 0000-0002-2495-3354 – National Yang Ming Chiao Tung University – ROR: https://ror.org/00se2k293Wójtewicz, Szymon – ORCID: 0000-0001-8600-0543 – Nicolaus Copernicus University – ROR: https://ror.org/0102mm775Ciuryło, Roman – ORCID: 0000-0003-2638-0403 – Nicolaus Copernicus University – ROR: https://ror.org/0102mm775Lisak, Daniel – ORCID: 0000-0001-5545-7989 – Nicolaus Copernicus University – ROR: https://ror.org/0102mm775Bielska, Katarzyna – ORCID: 0000-0002-4218-9193 – Nicolaus Copernicus University – ROR: https://ror.org/0102mm775Contact person:Szymon Wójtewicz – Institute of Physics, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, Grudziądzka 5, PL-87-100 Toruń, Poland – ROR: https://ror.org/0102mm775.Data set related to the publication "Theoretically predicted CO2 lines near 700 nm not observed".The data is available under a CC BY 4.0 license.Link to related publication: https://doi.org/10.1063/5.0152996DOI: 10.1063/5.0152996All data were collected in 2023 at temperature 296 K and pressures 150 or 200 Torr using the optical frequency comb assisted, Pound–Drever–Hall locked, frequency-stabilized cavity ring-down spectrometer.Deposited data:Data_experimental_spectra - folder containing files with experimental data for three carbon dioxide bands lying between 14300 and 14550 cm^(-1). The first column in the file is the frequency, and the second column are losses (1/(c*tau)).