Rotational spectroscopy is one of the most outstanding techniques for investigating the structure and dynamics of gas-phase molecules. Pure rotational spectra are primarily observed in the frequency range from 300 MHz to 1 THz, spanning the centimeter to submillimeter wave regions. Over the past five decades, significant advances in radiation sources, detectors, and digital electronics have led to substantial improvements in experimental methodologies in this field. As a result, modern rotational spectroscopic measurements benefit from markedly enhanced sensitivity and resolution, enabling the study of an ever-increasing number of molecular species with growing structural complexity. These developments have expanded the scope of rotational spectroscopy from simple diatomic molecules to moderately large systems containing up to approximately 50 atoms. Rotational spectroscopy is widely applied to the investigation of molecules of atmospheric relevance and astrophysical interest, as well as biomolecules, weakly bound complexes, transient or unstable species, and metal-bearing or ionic clusters. In this work, recent laboratory spectroscopic studies employing rotational spectroscopy to probe biomolecules, atmospheric species, and molecules of astrophysical significance are reviewed. Particular attention is given to the experimental techniques employed, the strategies used to characterize the observed species, and the broader implications of the reported results.




