HI absorption studies are effective in probing the HI content in high redshift (z > 0.1) galaxies, where HI emission is too faint to be detected. Although Ly alpha absorption can be used to probe
In this study, we demonstrated cold gas-phase spectroscopy of chemical intermediates produced in solution. Herein, we combined an electrospray ion source with a T-shaped solution mixer for introducing
Fourier transform infrared spectra of isolated 1-propenol and 2-propenol in the gas-phase have been collected in the range of 900–3800 cm–1, and the absolute infrared absorption cross sections reporte
