Low-$J$ transitions in $\tilde{A}^2\Pi(0,0,0)-\tilde{X}^2\Sigma^+(0,0,0)$ band of buffer-gas-cooled CaOH

TL;DR

This study provides high-resolution spectroscopic data on low-J transitions of CaOH, improving frequency measurements and expanding known transitions, which supports astrophysical detection efforts.

Contribution

It reports new low-J transition data for CaOH using buffer-gas cooling, with improved measurement accuracy and identification of previously unreported lines.

Findings

40 transitions assigned, including 27 new ones

Rotational constants match previous data, with improved frequency accuracy

Buffer-gas cooling effectively probes low-J transitions in astrophysical molecules

Abstract

Calcium monohydroxide radical (CaOH) is receiving an increasing amount of attention from the astrophysics community as it is expected to be present in the atmospheres of hot rocky super-Earth exoplanets as well as interstellar and circumstellar environments. Here, we report the high-resolution laboratory absorption spectroscopy on low-$J$ transitions in $\tilde{A}^2\Pi(0,0,0)-\tilde{X}^2\Sigma^+(0,0,0)$ band of buffer-gas-cooled CaOH. In total, 40 transitions out of the low-$J$ states were assigned, including 27 transitions which have not been reported in previous literature. The determined rotational constants for both ground and excited states are in excellent agreement with previous literature, and the measurement uncertainty for the absolute transition frequencies was improved by more than a factor of three. This will aid future interstellar, circumstellar, and atmospheric identifications of CaOH. The buffer-gas-cooling method employed here is a particularly powerful method to probe low-$J$ transitions and is easily applicable to other astrophysical molecules.