Infrared astronomy relies on specialised instruments designed to detect and analyse radiation from approximately 1 µm to several hundred microns in wavelength. Key components include cooled detector ...

Far-infrared spectroscopy probes the cold and dust-enshrouded regions of the Universe by measuring electromagnetic radiation in the 30–300 μm band. This regime encompasses the principal cooling lines ...

IR spectroscopy, or infrared spectroscopy, is an analytical technique used to identify and study chemical substances based on their interaction with infrared radiation. It measures the absorption of ...

The Fourier Transform Infrared Spectroscopy is an exceptional analytical tool that has changed the ways in which scientists and researchers of various fields understand the molecular world. It is a ...

PiFM and PiF-IR are the next generation of infrared spectroscopy techniques. PiFM brought a major shift to atomic force microscopy by adding chemical mapping capabilities. PiF-IR, its sister technique ...

The sample preparation before conducting an infrared spectroscopy (IR) study is as critical as the study itself, and the samples which are difficult to dissolve in any IR-transparent solvent are mixed ...