The near-infrared experimental investigation of greenhouse gases and their spectroscopic parameters finds a wide range of applications in the field of atmospheric science, astrophysics, and climate change research. Carbon dioxide (CO2), an important greenhouse gas, has been the subject of various spectroscopic studies due to its pivotal role in climate change, as well as in the atmospheric and astrophysical sciences. In this study, we present the spectroscopic investigation of ro-vibrational lines of P- and R-branches of the weak 31112–01101 band (f-symmetry) of CO2 lying in 1.57 μm spectral region. The study was carried out by high-sensitive off-axis integrated cavity output spectroscopy (OA-ICOS) coupled with a continuous wave-external cavity diode laser (CW-ECDL) source. The study focuses on the experimental measurement of vital spectroscopic parameters, such as air-broadening coefficients (γair), line intensities and self-broadening coefficients (γself) of various interference free lines (8 ≤ J ≤ 28) in the P- and R-branches of the hot band. The OA-ICOS absorption lines were modeled using the Voigt profile function to retrieve the parameters, which accurately reproduced the line shapes within the spectral noise level. The obtained γair were compared with empirical values present in HITRAN2020 and theoretical values in CDSD, showing mean discrepancies of about 3.20% and 1.25%, respectively. The retrieved line intensities and γself were also compared with previously reported values, revealing mean discrepancies of about 1.99% and 1.34%, respectively. Additionally, rotational dependency, the Einstein-A21 coefficient, effective collision diameter and cross-sections for CO2-CO2 and CO2-air binary systems have also been explored and presented. The molecular spectroscopic parameters retrieved in this study will find various applications in the field of atmospheric science, astrophysical science, and climate change research.
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