# H2-Induced Pressure Broadening and Pressure Shift in the P-Branch of the v3 Band of CH4 from 300 to 700 K

## TL;DR

This study provides detailed measurements of pressure broadening and shifts in methane's v3 band at high temperatures, improving models of exoplanet atmospheres.

## Contribution

It offers new high-temperature pressure broadening and shift data for methane's v3 band, enhancing atmospheric modeling accuracy.

## Key findings

- Measured linewidths for 116 transitions between 300 and 700 K.
- Derived rotation- and tetrahedral-symmetry-dependent broadening coefficients.
- Data will improve radiative-transfer models for exoplanet atmospheres.

## Abstract

For accurate modelling of observations of exoplanet atmospheres, quantification of the pressure broadening of infrared absorption lines for and by a variety of gases at elevated temperatures is needed. High-resolution high-temperature H2-pressure-broadened spectra are recorded for the CH4 v3-band P-branch. Measured linewidths for 116 transitions between 2840 and 3000 cm^{-1} with temperature and pressures ranging between 300 and 700 K, and 10 and 933 Torr, respectively, were used to find rotation- and tetrahedral-symmetry-dependent coefficients for pressure and temperature broadening and pressure-induced lineshifts. The new pressure-broadening data will be useful in radiative-transfer models for retrieving the properties of observed expolanet atmospheres.