Journal of Quantitative Spectroscopy and Radiative Transfer

These data reflect night sky brightness in the areas where the monitoring stations are located. The brightness of the night sky is an important factor in astronomical observation, which is also closely related to the local environment and economic development level.

Table 1: Speed-dependent Voigt line-shape parameters for air-broadened CO2 lines, deduced from rCMDS-calculated spectra. gamma0, gamma2 are in cm-1/atm and Y as first-order line-mixingin atm-1. In parenthesis there are the statistical uncertainty in the unit of the last quoted digit. Table 2: The revised line shape parameters of CO2-air and CO2-CO2 using the Voigt and speed dependent Voigt profiles. The update on the Voigt parameters group is included in the '.par' file as in HITRAN 2016 plus the first two extra columns for the temperetaure dependence of self- half width (n_air) and self shifts (delta-self) for the Voigt profile. The next columns are the update of speed dependent Voigt parameters as follows: air- half width (gamma_SDV_0_air_296), self- half width (gamma_SDV_0_self_296), temperature dependence of air- half width (n_SDV_air_296), temperature dependence of self- half width (n_SDV_self_296), air- speed dependence of width (gamma_SDV_2_air_296)/(gamma_SDV_0_air_296), self- speed dependence of width (gamma_SDV_2_self_296)/(gamma_SDV_0_self_296), air- first-orderline mixing (Y_SDV_air_296), self- first-order line mixing (Y_SDV_self_296), temperature dependence of air- speed dependence of width (n_gamma_SDV_2_air_296), and temperature dependence of air- first-orderline mixing (n_Y_SDV_air_296), respectively.

The spin-allowed A1Sigma+-X1Sigma+ and b3Pi-a3Sigma+ TDM functions of the RbCs molecule obtained by the scalar-relativistic CI-CPP calculations. The fully relativistic (2,3)0+ - (1)0+ curves are the original TDM functions obtained using FSRCC-FF method in the framework of the conventional adiabatic representation. And their quasi-diabatic A0+ - X0+, b0+ - a1, b1 - a0- TDM functions derived from the relativistic FSRCC-FF data.

Data for: High-resolution Fourier-transform spectroscopy and deperturbation analysis of the A1Π(v = 1) level in 12C18O. Log file of the final 12C18O deperturbation fit together with line list, results (constants and terms with uncertainties) and correlation matrix.

Tables from the paper in Excel

1.MODIS_M3_08data 2. BCC_RAD radiation transfer model

Description of supplementary material for : Ab initio calculations of collisional line–shape parameters and generalized spectroscopic cross-sections for rovibrational dipole lines in HD perturbed by He by Kamil Stankiewicz, Hubert Jóźwiak, Maciej Gancewski, Nikodem Stolarczyk, Franck Thibault, Piotr Wcisło The generalized spectroscopic cross-sections as a function of collision relative kinetic energy defined by Eq.4 are given in files HD_HeXS*.txt. The values in subsequent columns are the kinetic energy, the real part of σ0q (PBXS), the imaginary part of σ0q (PSXS), the real part of σ1q (RDXS), the imaginary part of σ1q (IDXS) and the inelastic contribution to the PBXS (Inel. Contr.). Kinetic energy is given in cm-1, the cross-sections and inelastic contribution in Å2. For example the file HD_HeXS2_0R_4.txt provides the cross-sections for the electric dipole R(4) line of the 2-0 band. The thermally averaged pressure broadening and shift coefficients (PBC and PSC), real and imaginary parts of the optical frequencies of velocity-changing collisions (Re(νopt) and Im(νopt)), defined by Eqs. 6 and 7, are given in the HD_Heline_shape*.txt files. Temperature is given in K and the values of the coefficients in 10-3 cm-1/atm. For example file HD_Heline_shape5_0P_3.txt contains data for electric dipole P(3) line of 5-0 band.

Polymers are widely used in many fields such as radiative cooling, infrared stealth, optical fibers and solar cells. In this work, the complex refractive indices of seven polymers such as polydimethylsiloxane (PDMS), polymethyl methacrylate (PMMA), polycarbonate (PC), polystyrene (PS), polyethylene terephthalate (PET), polyvinyl chloride (PVC), and polyetherimide (PEI) are measured by spectroscopic ellipsometry (SE) combined with the ray tracing method (RTM) from near-infrared to mid-infrared bands (2-20 micro). The measured results of PDMS have been proved to be accurate by comparing them with previous data in the literature. The obtained refractive indices of polymers in this paper have been compared with the results calculated by the Kramers-Kronig relations. Finally, we analyze the reasons of absorption peaks of these materials in infrared bands by the vibration of chemical bonds in molecules.

The complex refractive index as shown in Fig.2 - 8 can be seen in Data File 1 - 7.

Supplementary data to Empirical rovibrational energy levels of ammonia up to 7500 cm-1